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Page 1: Appendix B3 – Saturn Model Development Report

Appendix B3 – Saturn Model Development Report

Page 2: Appendix B3 – Saturn Model Development Report

Sheffield & Rotherham District SATURN Model 2008

Model Development Report

Report for Sheffield City Council

September 2009

Page 3: Appendix B3 – Saturn Model Development Report

Document Control

Project Title: Sheffield and Rotherham District SATURN Model 2008

MVA Project Number: C37272

Document Type: Model Development Report

Directory & File Name: M:\tp\C37272 FC 36842 Sheffield Model

Update\Word\LMVR\Report\Final\Main Report v8.0.doc

Document Approval

Primary Author: Andrew Ford

Reviewer: John Allan

Formatted by: Andrew Ford

Distribution

Issue Date Distribution Comments

1 03/07/2009 SCC, MVA Draft

2 05/08/2009 SCC Draft Version 2

3 08/09/2009 SCC, Workspace Final

4

Page 4: Appendix B3 – Saturn Model Development Report

Contents

1 Introduction 1.1 1.1 Background 1.1 1.2 Model History 1.1 1.3 Structure of the Report 1.2

2 Model Overview And Dimensions 2.1 2.1 Introduction 2.1 2.2 The Study Area and Zone System 2.1 2.3 Base Year 2.3 2.4 Time Periods 2.3 2.5 User Classes 2.3 2.6 Network and Junction Characteristics 2.2

3 Data Collection and Collation 3.1 3.1 Introduction 3.1 3.2 Roadside Interview Surveys 3.1 3.3 Count Data 3.3 3.4 Independent Count Set 3.4 3.5 Journey Time Survey Data 3.4

4 Road Network 4.1 4.1 Introduction 4.1 4.2 Network Coverage 4.1 4.3 Data Required for SATURN 4.1 4.4 Range and Logic Checks 4.3

5 Road Traffic Demand Matrices 5.1 5.1 Introduction 5.1 5.2 Summary of the Matrix Building Process 5.1 5.3 Expand RIS 5.2 5.4 Reverse Synthesis 5.3 5.5 Calibrate gravity model and estimate unobserved car trips 5.9 5.6 Estimate LGV and OGV trips within study area sectors 5.12 5.7 Estimate external to external trips 5.12 5.8 Apply Growth to 2006 Matrices 5.13 5.9 Assignment 5.13

6 Model Assignment and Calibration 6.1 6.1 Introduction 6.1 6.2 Assignment Procedure and Convergence 6.1 6.3 User Classes 6.2

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Contents

Sheffield and Rotherham District SATURN Model 2008 2

6.4 Generalised Cost Formulation 6.2 6.5 Calibration Procedure 6.4 6.6 Development of the 6 User Class Models 6.4

7 Validation 7.6 7.1 Introduction 7.6 7.2 Calibration count comparisons 7.6 7.3 Cordon Validation 7.14 7.4 Important Count Sets 7.16 7.5 Independent Count Validation 7.18 7.6 Journey Time Comparison 7.21 7.7 Inspection of Typical O-D Routes 7.24 7.8 Matrix Characteristics 7.25 7.9 Trip Length Distribution 7.26 7.10 Trip Ends 7.31 7.11 Origin Destination pairs 7.36

8 Summary and Conclusions 8.1 8.1 Summary 8.1 8.2 Conclusions 8.2

Tables

Table 3.1 Description of Journey Time survey routes 3.4 Table 5.1 Transpose 12 hour to Modelled Hour Percentages – by Purpose 5.4 Table 5.2 Trip-rates used in the Gravity Model 5.10 Table 5.3 Estimated Trip-end Totals and Fully Observed Demand 5.12 Table 5.4 ATC Traffic Growth Factors 5.13 Table 6.1 Convergence Statistics 6.2 Table 6.2 Generalised Cost Parameters – Six User Class 6.3 Table 7.1 Validation against all Calibration Counts prior to Matrix Estimation 7.9 Table 7.2 Validation against all Calibration Counts after Matrix Estimation 7.10 Table 7.3 Comparison of modelled flows against observed counts (All vehicles combined)7.11 Table 7.4 Screenline Flows across Sheffield and Rotherham Cordons – Before Matrix

Estimation 7.15 Table 7.5 Screenline Flows across Sheffield and Rotherham Cordons – After Matrix

Estimation 7.16 Table 7.6 Validation against Important Count Sets after Matrix Estimation 7.17 Table 7.7 Independent Count Validation Statistics 7.21 Table 7.8 Journey Times within 15% (or 1 minute if greater) 7.22 Table 7.9 Percentage of Routes passing DfT criteria 7.23 Table 7.10 Summary of Hourly 6 user class Trip Matrices (pcus) 7.25 Table 7.11 Average Car Trip Lengths Before and After Matrix Estimation 7.28 Table 7.12 Average Car Trip Lengths Before Matrix Estimation – All User Classes, to, from

and within Study Area 7.30 Table 7.13 Correlation between Trip end totals before and after matrix estimation 7.31 Table 7.14 Changes in Trip Ends Before and After Matrix Estimation 7.35

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Contents

Sheffield and Rotherham District SATURN Model 2008 3

Table 7.15 Correlation between Origin-Destination pairs before and after matrix

estimation 7.36

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Contents

Sheffield and Rotherham District SATURN Model 2008 4

Table of Figures

Figure 2.1 Sheffield and Rotherham SATURN Model Zone system 2.2

Figure 2.2 Sheffield and Rotherham SATURN Model zone system between Sheffield and Rotherham

urban centres 2.2

Figure 2.3 Sheffield and Rotherham SATURN Model zone system - Penistone Rd 2.3

Figure 2.4 Sheffield and Rotherham SATURN Model zone system - Sheffield City Centre 2.3

Figure 3.1 Location of Roadside Interview Surveys 3.2

Figure 3.2 Location of Classified Counts 3.3

Figure 3.3 Location of Independent Counts 3.4

Figure 3.4 Journey Time Survey Routes 3.6

Figure 4.1 Extent of Buffer and Simulation Networks 4.2

Figure 5.1 Matrix Building Flowchart 5.2

Figure 5.2 Schematic showing ‘observed’, ‘unobserved’ and ‘partially observed’ movements

5.7

Figure 5.3 Sector system used for matrix building 5.7

Figure 5.4 Various Observations of a particular O-D trip 5.8

Figure 7.1 Link Flow Validation Plot - Morning Peak 7.13

Figure 7.2 Link Flow Validation Plot - Inter-peak 7.14

Figure 7.3 Link Flow Validation Plot - Evening Peak 7.14

Figure 7.4 Location of Key Counts 7.15

Figure 7.5 Independent Count Validation Plot – Morning Peak 7.26

Figure 7.6 Independent Count Validation Plot – Inter-peak 7.26

Figure 7.7 Independent Count Validation Plot – Evening peak 7.27

Figure 7.8 Trip Length Distribution – Morning peak 7.28

Figure 7.9 Trip Length Distribution – Inter-peak 7.28

Figure 7.10 Trip Length Distribution – Evening-peak 7.29

Figure 7.11 Morning Peak Origin Trip Ends 7.33

Figure 7.12 Morning Peak Destination Trip Ends 7.33

Figure 7.13 Inter Peak Origin Trip Ends 7.34

Figure 7.14 Inter Peak Destination Trip Ends 7.34

Figure 7.15 Evening Peak Origin Trip Ends 7.35

Figure 7.16 Evening Peak Destination Trip Ends 7.35

Appendices

A Roadside Interview Programmes

B Roadside Interview Survey Variables and Value Labels

C Model Bandwidth Plots

D Counts Comparisons

E Journey Time Comparisons

F Route Checking

G Trip Matrix Summaries

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Contents

Sheffield and Rotherham District SATURN Model 2008 5

H Trip Length Distributions

I Index of Important Files

J Method for Controlling Matrices to TEMPRO

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Sheffield and Rotherham District SATURN Model 2008 i

Summary

Background

In autumn 2008, Sheffield City Council appointed MVA Consultancy to update their multi-

modal model for Sheffield and Rotherham. The new model will be used to support Major

Scheme Business Case submissions and inform future transport policy and strategy

development, post Local Transport Plan 2 (LTP2), within the Sheffield and Rotherham

districts.

The updated multi-modal model SRTM3 has a base year of 2008. It was developed from its

predecessor SRTM2, which had a base year of 2007. It includes three sub-models– a

demand model (SRDM3), a public transport model (SRPTM3) and a highway model (SRHM3).

All three sub-models have been updated – their predecessors were SRDM2, SRPTM2, and

SRHM2.

This report concerns the update of the highway model to form the 2008 highway model of

Sheffield and Rotherham - SRHM3. It describes the data sources and processes used to

calibrate and validate the model. It also presents the results of the validation and seeks to

demonstrate that the model is fit for the purpose of appraising transport schemes and

developments within the area of detailed modelling, an area that encompasses the entire

districts of Sheffield and Rotherham.

The update of the multi-modal model to 2008 had less effect on the highway model than the

other models. Unlike the other two, the highway model has remained on the same software

platform (SATURN) as its predecessor. It was built from the same set of origin-destination

surveys and it retains the same geographical coverage. The key changes is that it has been

calibrated to a set of counts that now include data in the city centre gathered after the

completion of the Northern Inner Relief Road major scheme in the city centre. It has

changed in other ways, with finer zoning on Penistone Road to the north of the city and

refinements made to the network in the City Centre. These changes were made in

preparation for forthcoming studies centred on those areas.

SRHM3 has been built from the following data sources:

2008 Vehicle Occupancy Counts;

2008 Manual Classified Counts – undertaken by SCC and RMBC;

2008 Roadside Interview Survey Data – undertaken in the Waverley area;

2008 Manual Classified Counts – undertaken by Sky High and Nationwide Data

Collection;

2008 to 2006 journey time data;

2007 to 2005 Roadside Interview Survey Data;

2007 to 2003 ATC Data;

2007 to 2003 Manual Classified Counts – undertaken by SCC, RMBC and other

sponsors; and

2001 Census data for all zones within the model updated to 2007 mid-year population

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Summary

Sheffield and Rotherham District SATURN Model 2008 ii

Fitness for Purpose

The fitness for purpose of the model is demonstrated through:

the comparison of modelled and observed flows;

− the correlation between modelled and observed flows is good for all time periods

and user classes, with the number of links with a GEH value less than 5 falling

just short of the stringent 85% level. The R squared value, showing the match

between modelled and observed counts, is greater than 0.97 in all time periods.

the comparison of modelled and observed journey times;

− the journey time validation is satisfactory in the morning and evening peaks,

although the inter-peak is less satisfactory due to limitations with the data. This

is further described below;

the inspection of routes between key areas in the model;

− analysis of origin-destination routes between key centres shows that the routing

taken by traffic through the network are plausible;

the description of the processes used to build the model;

− a thorough description of the network and matrix building process is provided,

highlighting the tasks that have been undertaken to ensure the underlying data

behind the model is accurate and robust.

DMRB sets out different criteria for comparison of modelled and observed flows depending on

the magnitude of the flows. Its main guideline is that 85% or more flows pass the criteria.

Against the set of counts used in calibration, our model performs well, with flows in all time

periods passing the guidelines. For the morning peak, inter-peak and evening peaks

respectively 88%, 92% and 89% of flows pass the DMRB guidelines.

For journey times the DMRB requires that 85% of modelled times be within 15% of observed

times (or 1 minute if greater). Our model performs acceptably, almost attaining the

stringent DMRB standard in the morning and evening peak periods. In both the morning and

evening peak 81% of routes pass the DMRB criteria. The inter-peak validation looks poor,

with many routes running too fast. However, we consider that the inter-peak journey time

data is not a valid representation of true inter-peak journey times. This is because many of

the journeys on which it was based span the peak and inter-peak periods. Thus the

observed inter-peak journeys are slower than the average inter-peak would be. Compared

to these slow observations – the inter-peak model appears to run too quickly. However, we

believe the inter-peak model as it stands replicates routings successfully during the inter-

peak period

The validation is good along all corridors of the schemes being brought forward to MSBC

submission, namely Penistone Road Smart Route and the Sheffield to Rotherham BRT routes

(via Meadowhall and Waverley). Both the count and journey time validation along these key

routes is good, enabling us to confidently use the model to appraise future transport

interventions. Further details will be provided in bespoke model development reports that

will accompany each MSBC submission.

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Summary

Sheffield and Rotherham District SATURN Model 2008 iii

Model Features

This Model Development Report describes the development and validation of the base year

(2008) Sheffield and Rotherham highway models (SRHM3) for the following three weekday

time periods:

weekday morning peak hour : 0800-0900;

weekday average inter-peak hour : 1000-1200 and 1400-1600; and

weekday evening peak hour : 1700-1800.

The six user class assignment segments the travel demand by income, a requirement of

models used for bids to the Transport Innovation Fund. The six user classes are as follows:

cars – employer’s business;

cars – commute and other – low income;

cars – commute and other – medium income;

cars – commute and other – high income;

light goods vehicles (LGVs); and

other goods vehicles (OGVs).

There are also fixed flows on the network which represent buses and trams.

Summary of Main Data Sources

The main data sources used to build the SATURN highway model were:

Roadside Interview Surveys (RIS) undertaken in 2005, 2006, 2007 and 2008

specifically for this model;

road traffic counts from 2005, 2006, 2007 and 2008;

journey time surveys 2008 (2 routes), 2007 (10 routes) and 2006 (4 routes);

traffic signal timings;

bus timetables; and

tram timetables.

Page 12: Appendix B3 – Saturn Model Development Report

Sheffield and Rotherham District SATURN Model 2008 1.1

1 Introduction

1.1 Background

1.1.1 In autumn 2008, Sheffield City Council appointed MVA Consultancy to recalibrate the existing

Sheffield and Rotherham Multi-Modal Model (referred to as SRTM2) to create a new 2008

base year model (referred to as SRTM3). SRHM3 will be used for several highway studies as

well as forming an integral part of the Sheffield and Rotherham District Multi-Modal Model

(called SRTM3) and the new South Yorkshire / Sheffield City Region Strategic Transport

Model (SYSTM+).

1.1.2 This report covers the highway element of SRTM3, called SRHM3. Separate validation reports

area available for the Demand model (SRDM3) and the Public Transport Model (SRPTM3).

1.2 Model History

1.2.1 The parent model for SRHM3 is SRHM1. This was the first version of the highway model to

form part of a multi-modal model. It extended the geographical coverage of the earlier

highway-only models to cover the whole of the two districts. It was built in 2006, from a

combination of new data and data gathered over the previous 5 years. It was calibrated

concentrating on Sheffield and Rotherham town centres, and also focussing on the Lower

Don Valley corridor. It was developed to support the development of the Sheffield &

Rotherham Bus Rapid Transit (Northern & Southern Routes) and Penistone Road Smart

Route Outline Business Case submissions to the Regional Transport Board and to undertake

initial option testing for the River Don District Masterplan.

1.2.2 By 2007, some of the roadside interview survey (RIS) data on the Sheffield city centre

cordon was 5 years old, too old to be used according to the DfT guidance. New RIS data

were gathered in 2007 for the update to SRHM2.

1.2.3 In 2007, traffic patterns had not yet fully settled down after opening of the Northern Inner

Relief Route in Sheffield City Centre. The update of the other components of the multi-

modal model to 2008 offered the chance to update the highway model again to reflect the

latest traffic patterns.

1.2.4 The development of the 2008 model (SRHM3) drew on a number of existing data sources:

the validated 2006 base year Sheffield and Rotherham SATURN model (SRTM1);

the validated 2007 base year Sheffield and Rotherham SATURN model (SRTM2);

existing RIS data;

manual classified counts and automatic traffic counts;

journey time survey data;

bus routes and frequencies; and

traffic signal timings.

1.2.5 The model required new data collection in the form of:

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1 Introduction

Sheffield and Rotherham District SATURN Model 2008 1.2

3 roadside interview survey sites in Rotherham;

manual classified counts; and

new journey time data.

1.2.6 This version of the model, SRHM3, has a base year of 2008 and has the same coverage as

SRHM1 and SRHM2 i.e. the entire area covered by the districts of Sheffield and Rotherham.

It contains trip origin and destination data obtained from a programme of Roadside Interview

Surveys (RIS);

3 sites surveyed in Rotherham in 2008;

50 sites surveyed in Sheffield in autumn 2007;

42 sites surveyed in Sheffield during 2006; and

11 sites surveyed in 2005 in Rotherham.

1.3 Structure of the Report

1.3.1 Following this introductory chapter, the remainder of the Model Development Report is set

out as follows:

Chapter 2 gives an overview of the model covering the study area, zone system, time

periods and vehicle types;

Chapter 3 provides details on the collection of new data and the collation of new and

existing data;

Chapter 4 describes the modelled representation of the Sheffield and Rotherham

highway network;

Chapter 5 outlines the construction of the trip matrices;

Chapter 6 presents details of the model assignment and calibration statistics;

Chapter 7 presents the model validation statistics;

Chapter 8 summarises the main elements of the report and the conclusions drawn.

1.3.2 Supplementary and more detailed information is provided in a series of appendices:

Appendix A details the dates and locations of the Roadside Interview Surveys;

Appendix B details the variable names of the data collected in the Roadside Interview

Surveys;

Appendix C shows SATURN bandwidth plots of vehicle flows in the model;

Appendix D details the counts that make up the validation count cordons and how the

modelled flows match them;

Appendix E shows, both graphically and numerically, the comparison between

observed and modelled journey times;

Appendices F1 to F3 shows the routes assigned by the model for important O-D

movements;

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1 Introduction

Sheffield and Rotherham District SATURN Model 2008 1.3

Appendix G summarises the trip matrices before and after matrix estimation at sector

level;

Appendix H compares the distribution of trip lengths before and after matrix

estimation;

Appendix I is an index of the key files used in the model; and

Appendix J is a Technical Note documenting the process used to control matrices to

TEMPRO.

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Sheffield and Rotherham District SATURN Model 2008 2.1

2 Model Overview And Dimensions

2.1 Introduction

2.1.1 This chapter provides an overview of the SATURN highway model (SRHM3), presenting the

study area and zone system, the highway users that are represented in the model, and the

time periods modelled.

2.2 The Study Area and Zone System

2.2.1 The SRHM1 zone system is the basis for the SRH3 zone system, and was originally devised

with 500 zones. Ten zones were added in the Manor Top area for use in appraising a new

development in that area, taking the number of zones to 510.

2.2.2 For SRHM2 a further twenty new zones were added enabling us to forecast demand using the

Park and Ride sub-model of the multi-modal model. Of these zones, five were coded into the

network at locations where we would be required to test future year park and ride

interventions, and the remaining zones coded as dummy zones. This took the number of

zones to 530.

2.2.3 The SRTM2 park and ride sub-model has now been merged into the SRDM3 Demand Model,

removing the need for Park and Ride zones in the network. These zones (20 in total) were

removed from the network.

2.2.4 For SRHM3 the zoning system has been revised along the Penistone Rd corridor, in order to

enhance the detail to support a proposed Major Scheme Business Case submission. This

process involved splitting several large zones into smaller zones, resulting in a net addition

of 15 zones.

2.2.5 Following these changes, all components of SRTM3 now consists of 525 zones. The zone

boundaries make use of natural or man-made barriers such as rivers, railways and roads.

The boundaries do not, however, match political boundaries.

2.2.6 The current SRTM3 zone system is shown overleaf;

Figure 2.1 shows the zone system for the whole study area;

Figure 2.2 shows the zone system focussed on Sheffield and Rotherham Urban

Centres;

Figure 2.3 shows the zone system focussed on Penistone Road;

Figure 2.4 shows the zone system in detail for Sheffield City Centre.

2.2.7 The level of detail is sufficient to provide an accurate representation of vehicle flows on the

network and model run times are in the region of 60 minutes using the latest processors.

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Sheffield and Rotherham District SATURN Model 2008 2.1

Figure 2.1 Sheffield and Rotherham SATURN Model Zone system

Figure 2.2 Sheffield and Rotherham SATURN Model zone system between Sheffield

and Rotherham urban centres

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2 Model Overview And Dimensions

Sheffield and Rotherham District SATURN Model 2008 2.2

Figure 2.3 Sheffield and Rotherham SATURN Model zone system - Penistone Rd

Figure 2.4 Sheffield and Rotherham SATURN Model zone system – Sheffield City

Centre

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2 Model Overview And Dimensions

Sheffield and Rotherham District SATURN Model 2008 2.3

2.3 Base Year

2.3.1 SRHM3 has been calibrated to a base year of 2008.

2.4 Time Periods

2.4.1 SRHM3 has retained the three time periods from all previous versions of the model:

weekday morning peak hour : 0800-0900;

weekday average inter-peak hour : 1000-1200 and 1400-1600; and

weekday evening peak hour : 1700-1800.

2.5 User Classes

2.5.1 The model is calibrated at a 3 user class level, as manual classified counts are only available

for cars, LGV and OGV. The final validated model is then segmented into six user class

versions, as required by WebTAG.

2.5.2 The rationale for segmenting the demand in this fashion is that the segments have quite

different values of time and/or vehicle operating costs. The values affect their choice of

routes in the highway model, their response to changes in costs in the demand model, and

also the economic evaluation of time savings in the cost benefits analysis.

Six User Class

2.5.3 The model employs the six segments of highway demand as recommended in the current

DfT guidance on highway modelling (webTAG):

Car – employer’s business;

cars – commute and other - low income;

cars – commute and other - medium income;

cars – commute and other - high income;

light goods vehicles (LGVs); and

other goods vehicles (OGVs).

2.5.4 The full range of validation checks were run on the six user class assignments, to ensure that

the splitting of the car demand into the 3 separate car user classes did not adversely affect

the validation of the model.

2.5.5 SATURN models route choice for cars and goods vehicles. It models buses and trams on

fixed routes, but does not model the number of passengers.

2.5.6 The model uses the following passenger car unit (PCU) factors:

cars and light goods vehicles 1.0;

other goods vehicles 1.7;

standard buses 2.0; and

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2 Model Overview And Dimensions

Sheffield and Rotherham District SATURN Model 2008 2.2

trams 6.0

2.5.7 The pcu factor for other goods vehicles was calculated using a sample of five classified

counts at different locations within the Sheffield and Rotherham Districts. The counts had

other goods vehicles separated into two classes:

rigid vehicles over 3.5 tonnes with 2 or 3 axles, with an accepted PCU factor of 1.5;

and

rigid vehicles with 4 or more axles and all articulated vehicles, with an accepted PCU

factor of 2.3.

2.5.8 We took a weighted average of the two PCU factors using the counts for each type over all

movements for all five classified counts. This resulted in an average OGV factor of 1.7.

2.6 Network and Junction Characteristics

2.6.1 The model contains:

2982 simulation nodes;

4682 simulation links;

− 3272 two-way links

− 1410 one-way links

213 buffer links;

571 signalised nodes;

76 roundabouts;

2263 priority junctions; and

661 external nodes.

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Sheffield and Rotherham District SATURN Model 2008 3.1

3 Data Collection and Collation

3.1 Introduction

3.1.1 The following data had been collected for previous versions of the model and were included

in the model building and validation:

traffic signal data from the Urban Traffic Control (UTC) teams of both councils;

bus service patterns;

journey time survey data;

roadside interview surveys; and

manual classified vehicle counts.

3.1.2 In addition to previous data, the following data were collected in Sheffield and used

specifically for this version of the model, SRHM3:

manual classified counts along Penistone Rd;

manual classified counts along Ecclesall Rd;

manual classified counts along the Northern Inner Relief Road;

manual classified counts in other key locations around the city centre;

3 roadside interview surveys undertaken in Rotherham;

2 updated journey time survey routes; and

vehicle occupancy survey count data.

3.2 Roadside Interview Surveys

3.2.1 We used RIS data undertaken for the following projects to create nine cordons in Sheffield

and Rotherham Districts:

2008 RIS data from surveys undertaken around the Waverley area;

2007 RIS data from surveys undertaken around Sheffield City Centre, Rotherham

Town Centre and motorway approach roads; and

2006 and 2005 RIS data from interview sites around Sheffield and Rotherham

Districts.

3.2.2 Surveys undertaken prior to 2007 were expanded to 2008 counts to give a consistent

baseline for 2008. The 106 sites constitute an extensive programme of roadside interview

surveys for a medium sized conurbation. The cordons are shown in Figure 3.1 along with

their constituent interview sites. Sector 8 is the rest of the United Kingdom outside of the

cordons pictured overleaf.

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3 Data Collection and Collation

Sheffield and Rotherham District SATURN Model 2008 3.2

Figure 3.1 Location of Roadside Interview Surveys

3.2.3 The survey programmes and example coding forms for the surveys are presented in

Appendix A. Each of these surveys involved asking drivers to identify the characteristics of

their current journey including:

time of interview (or receipt of postcard);

type of vehicle;

number of occupants;

origin address;

origin purpose;

destination address; and

destination purpose;

parking location; and

parking tariff (if applicable).

3.2.4 The roadside interviews included manual classified counts in both directions at each site on

the day of the survey and automatic traffic counts in both directions for the week during

which the survey was performed. The manual classified counts were factored in line with the

variation in the traffic volumes over the week of the survey. The ATC’s were carried out at

every location for 1 week, and were used to factor up the MCC’s from the survey day to an

average weekday. We did this as it is expected that the survey reduces the capacity of the

road at the survey site and thus lower flows are often observed on the day of the survey.

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3 Data Collection and Collation

Sheffield and Rotherham District SATURN Model 2008 3.3

3.3 Count Data

3.3.1 We had a collection of all counts undertaken in Rotherham and Sheffield for the 2007 version

of the model. In addition to those counts, Sheffield City Council had also conducted more up

to date counts in 2007 and 2008. All counts are from 2005 to 2008, with the vast majority

having been collected between 2006 and 2008. The locations of these counts are shown in

Figure 3.2.

Figure 3.2 Location of Classified Counts

3.3.2 The counts were gathered into the following specific count sets in order to calibrate the

model:

all model counts within both Sheffield and Rotherham Districts;

a cordon around Sheffield City Centre; and

a cordon around Rotherham Town Centre.

3.3.3 Along with the counts sets above, detailed analysis of the count calibration was undertaken

on the following subsets of counts along key corridors within Sheffield:

all counts along Penistone Road (proposed Smart Route);

counts on routes of the proposed Sheffield-Rotherham Bus Rapid Transit schemes; and

counts along Ecclesall Rd, Sheffield.

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3 Data Collection and Collation

Sheffield and Rotherham District SATURN Model 2008 3.4

3.4 Independent Count Set

3.4.1 In addition to the calibration counts, an independent count set was retained and not included

in matrix estimation. Figure 3.3 shows the location of the independent counts.

Figure 3.3 Location of Independent Counts

3.5 Journey Time Survey Data

3.5.1 Journey time information was obtained for 17 two-way routes, which are presented in Table

3.1 and Figure 3.4. Information was collected several times for each route in order to be

confident that the times recorded were representative of average traffic conditions.

Table 3.1 Description of Journey Time survey routes

Route Description Year

1 Abbeydale Road 2007

2 Ecclesall Road 2006

3 Sandygate 2007

4 Nether Green 2007

5 Meadowhead 2007

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3 Data Collection and Collation

Sheffield and Rotherham District SATURN Model 2008 3.5

6 Sheffield to Rotherham via

Junction 34 north

2006

7 Sheffield to Rotherham via

Junction 34 south

2006

8 Penistone Road / Neepsend

Lane

2007

9 Middlewood Road /

Penistone Rd

2007

10 Chapeltown 2007

11 Crystal Peaks 2006

12 Inner Ring Road 2008

13 Outer Ring Road 2007

14 Sheffield Parkway 2007

15 Mosborough Parkway 2007

16 Crookes 2007

17 Penistone Rd - extended 2008

The routes that are highlighted are key routes that lay on or near major schemes that the

model will be used to test and appraise.

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3 Data Collection and Collation

Sheffield and Rotherham District SATURN Model 2008 3.6

Figure 3.4 Journey Time Survey Routes

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Sheffield and Rotherham District SATURN Model 2008 4.1

4 Road Network

4.1 Introduction

4.1.1 This chapter summarises the development of the highway definition for the SATURN road

traffic assignment model.

4.2 Network Coverage

4.2.1 Road traffic assignment models require a computerised representation of the highway

network with the following structure:

nodes – the points where roads intersect;

links – the sections of highway between the nodes; and

bus and tram flows on fixed routes.

4.2.2 SATURN offers two levels of network detail:

simulation network, in which capacity restraint is based on gap acceptance (which

represents the extent to which vehicles on minor arms of priority junctions give way to

vehicles on the major arms) applied to the interaction between movements at

junctions; and

buffer network, in which capacity restraint is based on flow delay curves, where

increased flows on a particular link result in increased travel times along that link.

4.2.3 The basis of the SRTM2 network was, broadly speaking, Motorways, A roads, B roads and C

roads plus all bus routes within Sheffield and Rotherham.

4.2.4 This basic structure was amended to add detail in the following areas;

Amendments to incorporate the recently opened Northern Inner Relief Road (NIRR);

Changes to zone connectors within Sheffield City Centre, to ensure a closer match with

the City Centre ‘AIMSUN’ model;

Network detail was added along Penistone Rd to accompany the re-zoning which

occurred in this area; and

Improvements were made to several roundabouts in the vicinity of Rotherham Town

centre.

4.2.5 A skeletal buffer network was added outside of the study area (Sheffield and Rotherham

District) to provide realistic routes for longer distance trips entering the study area. The

extent of the buffer and simulation network is shown in Figure 4.1.

4.3 Data Required for SATURN

4.3.1 The information required for simulation coding encompasses the following attributes:

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Sheffield and Rotherham District SATURN Model 2008 4.2

link length;

link speed;

permitted movements;

saturation flows for each movement;

priorities for each movement;

lane usage and sharing;

flare lengths and stacking capacity;

signal staging; and

signal timings.

4.3.2 The information required for the buffer network coding requires the following attributes:

link length;

speed at capacity;

speed at free flow;

flow at capacity; and

a measure of the steepness of the flow delay curve.

Figure 4.1 Extent of Buffer and Simulation Networks

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4.4 Range and Logic Checks

SATNET Errors and Warnings

4.4.1 The SATURN network-building program SATNET produces error and warning messages which

were dealt with individually. All network errors that resulted in fatal errors and semi-fatal

errors were corrected and all the warning messages were inspected and the network was

corrected where necessary.

Bandwidth Plots

4.4.2 Bandwidth plots were used to check that the largest modelled flows occur on the expected

links and network changes were made as necessary. Appendix C presents the bandwidth

plots for total traffic in units of pcu’s.

Queues and Delays

4.4.3 Queues and delays predicted by the model were checked for plausibility in terms of size and

location, and network changes were made where necessary.

Crow-fly Distances

4.4.4 The crow-fly distance between the nodes specifying each link were compared to the coded

link length and any discrepancies checked using the GIS system and corrected where

necessary.

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5 Road Traffic Demand Matrices

5.1 Introduction

5.1.1 This chapter describes the production of the 2008 Sheffield and Rotherham base year

demand matrices which represent the origins and destinations of the trips in the model.

5.1.2 The production of the base year demand matrices was one of the major tasks in the study.

They were built using data from the 2005, 2006, 2007 and 2008 Roadside Interview Survey

Programmes, which collected travel patterns at 106 locations across Sheffield and

Rotherham.

5.1.3 The study area in this context means Sectors 1 to 7 and Sector 9, which lie within Sheffield

and Rotherham District. Sector 8 is the external area, consisting of some zones on the

periphery of Sheffield and Rotherham Districts and all the zones that cover the remainder of

the UK. Figure 3.1 in Chapter 3 shows the study area.

5.2 Summary of the Matrix Building Process

5.2.1 This section describes the process of building the highway demand matrices. In brief, these

tasks are:

Task 1 - the RIS data is processed to create car, lgv and ogv matrices for fully

observed movements:

Task 2 – the non fully observed cells are in-filled for car using a gravity model:

Task 3 - LGV and OGV non-fully observed cells within the study area are in-filled using

data from SRHM1:

Task 4 - All trips passing through the study area are taken from SRHM1 for all three

user classes.

Task 5 - Finally, these separate components are factored up to the base year of 2008

(if required) and combined, forming the prior matrices.

5.2.2 Figure 5.1 presents the matrix building process in the form of a flow-chart. It uses

parallelograms to represent data and boxes to represent tasks and processes, which are

numbered in the figure and the text. The tasks and sub-tasks are set out as follows:

Task 1 – create matrices from RIS data;

− Task 1a - synthesise missing data;

− Task 1b - expand to counts;

− Task 1c - select fully observed data;

Task 2 – create infill intra sector (study area sectors only) car matrices using gravity

model;

− Task 2a – create trip ends for zones within study area;

− Task 2b – adjust trip ends to match required purpose splits;

− Task 2c – calibrate gravity model;

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− Task 2d – create 2008 car infill matrices;

Task 3 – create infill intra sector (study area sectors only) lgv and ogv matrices;

Task 4 – create infill external to external matrices for car, lgv and ogv;

Task 5 – factor up matrices created in Task 3 and 4;

Task 6 – combine matrices;

Task 7 – assign and calibrate.

Task 1 Task 3Task 2

Task 6

Task 5

Task 7

4Create Infill 2008Car, LGV and OGV

Matrices – ExternalTrips

1aSynthesise

Missing Data

5Add Appropriate

Growth

1cSelect Fully

Observed Data

1bExpand

to Counts

6Combine Matrices

2dCreate 2008

Car Infill Matrices

2cCalibrate Gravity Model

2aCreate Trip Ends for

Study Area

2bAdjust trip ends to

match required purpose splits

3Create Infill 2008

LGV and OGVMatrices – Sectors 1

to 7 and Sector 9

7Assign andCalibrate

Task 4

Figure 5.1 Matrix Building Flowchart

5.3 Expand RIS

5.3.1 We expanded the RIS data using 14 different journey purposes – twelve for cars and one

each for LGVs and OGVs. These journey purposes were then aggregated to the six user-

classes used in the model. The fourteen journey purposes for car trips were:

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1 home to work;

2 work to home;

3 home to shopping;

4 shopping to home;

5 home to education;

6 education to home;

7 home to employer’s business;

8 employer’s business to home;

9 home to other;

10 other to home;

11 non-home based employer’s business;

12 non-home based other;

13 LGV; and

14 OGV

Synthesise Missing Data

5.3.2 There are three main reasons why we have to synthesise missing data in the roadside

interview surveys:

the surveys are only conducted in one direction at each site because they are very

expensive and at some sites it would be logistically impossible to survey in both

directions;

small roads with limited traffic flow are not surveyed because the extra expense

cannot be justified in terms of the extra data obtained; and

the Police occasionally close sites for a period of time because of safety or to avoid

excessive queues forming on strategic routes.

5.4 Reverse Synthesis

5.4.1 Reverse synthesis is a process allowing RIS data in the survey direction to be used to

estimate the journeys in the reverse direction. The process can be summarised as:

transpose origin and destination zone;

reverse journey purpose;

factor to observed purpose splits by hour; and

factor to observed counts.

5.4.2 The basis for the method is that:

Over the 12 hour survey period, traffic passing the site in the surveyed direction will

be a mirror image of the traffic in the reverse direction (ie it is assumed that issues

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such as route variation by direction, single direction journeys, and travel outside the

12 hour period are relatively unimportant);

Information from the forward direction at the site provides the distribution and trip

purpose proportions for the transposed data for the 12 hour period taken as a whole;

and

Information from the RIS observed forward purpose profiles is used to proportion

transposed survey records by hourly period.

Transposition of Origin and Destination and Reversal of Journey Purpose

5.4.3 The first step is simply swapping the origin and destination zones and then reversing the

journey purpose. For the car home-based purposes the journey purpose is reversed (ie

“from home” becomes “to home”), while the non home based and lgv and ogv purposes are

maintained with the same purpose.

5.4.4 We cannot simply transpose morning peak forward direction trips to form evening peak

reverse direction trips because the mix of journey purposes is very different in the two. For

example the inter peak contains lots of shopping trips and the evening peak contains very

few. Therefore we match the journey purpose split in each modelled hour to a target split.

Factoring to Observed Purpose Splits by Hour

5.4.5 The proportion of each purpose’s trips within each hour is calculated from the forward data.

For example 38% of all work to home trips may occur in the hour 1700-1800. These profiles

are built for all purposes and for all hours.

5.4.6 The 12 hour transposed matrix is then factored to the modelled hour by reference to the

profile for that purpose. Thus if there are a total of 100 trips from work to home in a 12

hour period, assuming the profile mentioned above would give 38 trips in the pm peak hour.

This is applied by hour and purpose at all sites. The percentages used are shown in Table

5.2.

Table 5.1 Transpose 12 hour to Modelled Hour Percentages – by Purpose

Purpose AM IP PM

Home to Work 58% 6% 3%

Work to Home 2% 8% 38%

Home to Educ 3% 1% 1%

Educ to Home 0% 1% 1%

Home to Shop 3% 9% 5%

Shop to Home 0% 7% 4%

Home to EB 7% 2% 1%

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Purpose AM IP PM

EB to Home 0% 3% 5%

Home to Other 9% 13% 13%

Other to Home 2% 10% 11%

NHBEB 7% 18% 5%

NHBO 9% 21% 13%

Total 100% 100% 100%

5.4.7 This process also has the effect of smoothing the reverse matrix as all 12 hour survey

records for each purpose are used for each period.

Factoring to Observed Reverse Counts

5.4.8 The transposed and factored records were then summed by site, hour, and vehicle type and

factors calculated to get from these totals to the observed RIS non-survey direction counts

for each hour. These factors were created by site, vehicle type, and hour, and then applied

to the reverse matrix.

5.4.9 This gives the reverse matrix with:

Origin zone – original destination zone;

Destination zone – original origin zone;

Purpose – reverse of original purpose;

Period – from period profiles; and

Expansion factor – from 12 hour forward totals factored to modelled hour, factored to

observed counts by site and vehicle type.

5.4.10 Once the transposed matrix is created it is treated the same as the directly observed RIS

matrix and the two are simply added together.

Small Unsurveyed Roads

5.4.11 We have not surveyed every road, as some roads are lightly trafficked and it was not

deemed cost effective to survey these locations. It is important, however, to accurately

estimate the overall level of trip making.

5.4.12 Often the counts for smaller roads are simply added to the count of a nearby road which has

been surveyed. Whilst the counts of vehicles crossing a screenline will be correct, it is

unlikely that the origins and destinations will be truly representative. Vehicles on smaller

roads generally are making shorter trips.

5.4.13 We believe this can be improved upon by making sure that we don’t factor up trips that

would be very unlikely to use the unsurveyed road. We therefore took a sensible view on the

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Sheffield and Rotherham District SATURN Model 2008 5.6

likely range of vehicles using the unsurveyed roads and limited our synthesised trips to those

areas.

Temporary Site Closures

5.4.14 We expanded all the records in each time period to match the modelled hour count so there

was no need to synthesise data for missing individual half hour periods. There was only one

instance where a site was closed for a prolonged period of time leading to a sample size

which was unusable as a set of survey records. Site 616 on Sheffield Parkway was closed

outbound between 5pm and 7pm. We synthesised the records between 4pm and 5pm to

cover the remainder of the time period, and factored up to match the required traffic counts.

Similarly, Site 410 on Penistone Rd was closed between 5pm and 7pm and was synthesised

accordingly.

Expand to Counts

5.4.15 We expanded all the RIS data in a period to match the modelled hour counts for cars, LGVs

and OGVs. The classified counts were performed on the day of the survey and then factored

up using a one week ATC at the survey location. We did this as it is expected that the

survey reduces the capacity of the road at the survey site and thus lower flows are often

observed on the day of the survey.

Select Fully Observed Data

5.4.16 Figure 5.2 presents a schematic sector system to show examples of trips made within the

modelled area. The black lines represent the cordons that are made up of the surveys. Each

time a trip crosses a cordon it is said to be observed. Trips were classified as being:

observed once (shown in green);

unobserved or partially observed (in red); and

observed multiple times (in blue).

5.4.17 We excluded any data which was only partially observed and retained and fully observed

data.

5.4.18 Figure 5.3 presents the sector system applied to the zones in the model.

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Figure 5.2 Schematic showing ‘observed’, ‘unobserved’ and ‘partially observed’

movements

Figure 5.3 Sector system used for matrix building

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Multiple Observations

5.4.19 For trips that were observed multiple times, we needed to factor them so that they were only

included once in the trip matrix. Figure 5.4 shows that this is not straightforward as a trip

between sectors 2 and 5 (both within Sheffield District), for example, could be observed two

or three times between its origin and destination. Only using a process called barrier

factoring could we estimate the proportion of trips that use each of the three routes,

however this process is not appropriate where there are motorway based cordons. Since we

have several cordons, we decided not to use this method; we decided to use a more robust

method of dealing with multiple observations, as detailed below.

5.4.20 We know that all three routes are common in the fact that they all cross the cordons

surrounding sectors 2 and 5 (the three different route variants are shown in red, blue and

green respectively). Therefore, for such trips, we only included observations crossing both

the origin and destination sector cordons. As every trip between these sectors is observed

twice by these cordons, we simply halved all these observations.

5.4.21 Different routes taken for trips within sector 7 have also been shown in Figure 5.4 below,

giving an example of multiple observed trips for both Sheffield and Rotherham.

Figure 5.4 Various Observations of a particular O-D trip

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5.5 Calibrate gravity model and estimate unobserved car trips

5.5.1 Roadside Interview Surveys cannot feasibly capture all the movements made by travellers in

an area the size of Sheffield and Rotherham. Some movements remain wholly or partially

unobserved. These movements were estimated using a gravity model. A gravity model is

one of two methods suggested in DMRB for in-filling trip matrices the alternative being to in-

fill using data from another model.

5.5.2 We ran a separate gravity model for each journey purpose and time period combination. The

first task was to calibrate the gravity model to reproduce the demand in the fully observed

cells of the trip matrices. The calibration produced the parameters that determine the shape

of the deterrence function applied in the model – which helps to determine the trip length

distribution in the output. The parameters were calibrated using functions built into the

gravity model software. The trip-length distributions in the observed data were checked for

plausibility and the trip-length distributions estimated by the gravity model were checked for

their fit to the observed data.

5.5.3 Once the model parameters have been calibrated, gravity models can be applied in two

different modes. In trip-end mode, the user estimates the demand generated in each zone

using independent data on population, trip-rates and land-use. In partial matrix mode, the

gravity model attempts to infer the trip-ends from the same data used to calibrate the model

parameters.

5.5.4 We tried both modes and opted for the trip-end mode because it produced trip matrices that

provided a much better fit to the observed flows of traffic.

5.5.5 Trip-length distributions for the observed and estimated data were checked carefully. They

were checked for the matrices as a whole and for sub-areas – fully observed cells, non-

observed cells.

5.5.6 We estimated trip-ends for the gravity model from zonal population data and trip-rates. The

zonal population data came from the 2001 Census, having been adjusted to match the latest

mid-year population estimates (2007). Table 5.2 overleaf shows the trip-rate values used,

which were derived from TEMPRO by dividing the trip-ends by the population. The process

for undertaking the calculation of the trip-ends is described in Appendix J.

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Table 5.2 Trip-rates used in the Gravity Model

From-home To-home Purpose Trip Rate

Denominator AM IP PM AM IP PM

HBW Workers 0.139 0.008 0.007 0.003 0.017 0.124

HBEB Workers 0.012 0.003 0.001 0.000 0.004 0.010

HBED Population *

households with

car / Total

households 0.015 0.003 0.003 0.002 0.005 0.005

HBShop Population *

households with

car / Total

households 0.003 0.011 0.006 0.000 0.011 0.008

HBOther Population *

households with

car / Total

households 0.012 0.016 0.015 0.003 0.017 0.124

NHBEB Jobs 0.004 0.008 0.003 N/A N/A N/A

NHBO Population 0.005 0.012 0.011 N/A N/A N/A

5.5.7 Following the first pass of the gravity model, we improved the fit of the output matrix to the

fully observed data using K-Factors. Trips between the 9 sectors, identified Figure 5.3, were

fully observed in the surveys. The function of the gravity model is to estimate the trips

within each sector. By controlling the gravity model to reproduce the observed totals

between sectors we can ensure that the estimate of the trips within each sector accounts

exactly for the shortfall between the fully observed trips and the total trips. The K-factors

are the method by which we control the gravity model to match the fully observed demand.

K-factors are calculated at sector-level, one is calculated for origin-sector to destination-

sector pairing. The same K-factor is applied to every zonal origin-destination pair that

correspond to the sector level origin-destination pair.

5.5.8 The fully observed cells were eventually overwritten with the demand from the roadside

interview surveys. Thus the estimated demand from the gravity model was used only to in-

fill intra-sector movements.

5.5.9 The gravity model was used to infill only the cells within the study area. Trips with one end

outside the area and one end inside the area were fully observed in the surveys. Trips with

both ends outside the study area were taken from SRHM1.

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5.5.10 For the most part the calibration worked well, but for employer’s business there was a

mismatch between the observed demand and the demand estimated from the trip-ends. The

observed demand exceeded the trip-ends totals. For employers business, we retained the

fully observed demand in the inter-sector cells and used the gravity model’s initial estimate

of demand for the intra-sector cells.

5.5.11 Table 5.3 below shows the split between fully observed and estimated trip ends, over a 12

hour period. There are overall about the same number of fully observed trips as there are

estimated trips. Within the individual journey purposes, the percentage of trips that are fully

observed ranges from 45% (Work to Home) to 63% (Non Home Based Employers Business),

with the following exceptions:

Education trips have the shortest trip length distribution of all the trips, as many will

be very short journeys between home and school. Hence it is unsurprising that many

of these trips are intra-sector trips, and fully observed trips make up only 30% of the

total trips; and

Only 30% of OGV trips are fully observed. This is because a large proportion of the

trips in the matrix are through trips along the M1 / M18, which are estimated from the

previous SRHM1 highway model.

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Table 5.3 Estimated Trip-end Totals and Fully Observed Demand

Journey Purpose Estimated

Trip-ends

Fully

Observed

% Fully

Observed

Home to Work 86,624 80,004 48%

Work to Home 89,335 73,076 45%

Home to Employers Business 9,845 11,289 53%

Employers Business to Home 14,319 15,551 52%

Home to Education 31,513 14,208 31%

Education to Home 18,466 8,440 31%

Home to Shopping 19,801 30,127 60%

Shopping to Home 20,260 30,290 60%

Home to Other 49,951 56,265 53%

Other to Home 50,878 50,318 50%

Non Home Based Employers Business 32,624 55,205 63%

Non Home Based Other 53,169 77,657 59%

LGV 74,794 73,298 49%

OGV 102,115 44,718 30%

Total 653,693 620,445 49%

5.6 Estimate LGV and OGV trips within study area sectors

5.6.1 The LGV and OGV intra sector trips for sectors 1 to 7 and sector 9 were taken from SRHM1.

5.7 Estimate external to external trips

5.7.1 The Car, LGV and OGV external to external trips were taken from SRHM1.

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5.8 Apply Growth to 2006 Matrices

5.8.1 Our starting point was the matrices from the 2006 calibrated version of the Sheffield and

Rotherham model, SRHM1. These matrices were already segmented into the same user

classes as SRHM3 and had the same zone system at the matrix building stage. Therefore we

simply needed to factor the matrices to represent the expected growth in traffic between

2006 and 2008.

5.8.2 We used growth factors from ATC data provided by Sheffield City Council. The data covered

over 50 routes between 2003 and 2007. We only analysed routes which contained data for

all of the observed years, and worked out an average growth rate based upon this data for

each time period. For 2008 we did not have a full set of comparable data to undertake this

comparison. We therefore extrapolated the 2003 to 2007 data to obtain a projected trend for

growth between 2007 and 2008.

5.8.3 Table 5.4 presents these growth rates.

Table 5.4 ATC Traffic Growth Factors

2004 -

2008

2005 -

2008

2006 -

2008

2007 -

2008 2008

AM 0.986 1.000 1.003 1.003 1.000

IP 1.005 1.009 1.001 0.995 1.000

PM 0.989 0.997 1.005 0.996 1.000

12-hour 1.004 1.007 1.005 0.999 1.000

5.8.4 The following elements were factored from 2006 to 2008;

Unobserved car trips for trips within Sector 8 – from existing Car 2006 matrices.

Unobserved LGV and OGV trips within all sectors – from existing LGV and OGV 2006

matrices,.

5.8.5 Having factored the above matrices up to a 2008 base year, they were combined with the

following components to create 2008 prior matrices to be assigned by SATURN:

Unobserved car trips – from gravity model from Sectors 1 through to 9 (excluding

Sector 8); and

Observed car, LGV and OGV trips – from expanded roadside interview surveys.

5.9 Assignment

5.9.1 The first task in calibrating the model was to eliminate network errors. We highlighted these

using several techniques. We looked for excessive delays at junctions and peculiar routes

between origins and destinations. We compared modelled and observed flows on individual

links and turns and the modelled and observed journey times on key routes.

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5.9.2 Once we thought we had eliminated all the network errors we moved on to matrix

estimation. This is a powerful but potentially dangerous technique because it can disguise

weaknesses in the model. It makes changes to the trip matrix to try to get the modelled

flows to match the counts, so it implicitly assumes that all the model error lies in the matrix.

It will therefore introduce compensating errors where there are still errors in the network.

5.9.3 The matrix estimation process was iterative with network deficiencies gradually eliminated

during the calibration. Each time a network error was identified we corrected it, assigned the

original matrix, and then re-ran the matrix estimation process. This ensured that any

amendments which were made to the trip matrix as a result of network errors were not

retained once the network error had been corrected.

5.9.4 Several rounds of matrix estimation were run end on end, with the following key points

included in the approach:

fully observed data was frozen in the first iteration, in order to only estimate upon the

non-fully observed (infilled) cells in the first instance;

another iteration was undertaken where only the Sheffield and Rotherham cordon

counts were used, individually and as a cordon set. From our experience in other

projects, this method works well in helping to validate a cordon; and

some iterations were performed only on cars after we observed LGVs and OGVs had

already reached satisfactory levels of calibration.

5.9.5 The SATURN Matrix Estimation program SATME2 is much better behaved when presented

with a good quality prior matrix. Use of the program with matrices that contain partial

observations in some cells produces poor results and is not recommended. We were

confident that our prior matrix was of good quality since all the cells were either fully

observed in the surveys or derived from the recommended gravity model approach.

5.9.6 We set parameters within SATME2 to limit the changes that the program could make to

matrices. The trip ends were capped at a value 50% greater than in the prior matrix, in

order to prevent distortion of the matrix and the creation of many short distance trips, which

SATURN has a tendency to do in order to match counts.

5.9.7 The following checks were undertaken before and after matrix estimation, to ensure that the

matrices had not been overly distorted, and are reported in Chapter 7;

Trip length distribution plots;

Average trip lengths;

Changes in sector to sector movements;

Correlation between trip ends before and after matrix estimation; and

Correlation at an O-D level before and after matrix estimation.

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Sheffield and Rotherham District SATURN Model 2008 6.1

6 Model Assignment and Calibration

6.1 Introduction

6.1.1 The objective of this chapter is to present a summary of the steps undertaken to calibrate

and validate the SATURN model. It covers convergence levels, user classes, generalised cost

formulation, calibration procedures, comparison with counts, comparison with journey time

information and characteristics of the final matrices.

6.1.2 Calibration and validation is primarily undertaken using the 3 user class model (Car, LGV and

OGV), as traffic counts cannot be split into different car user classes.

6.1.3 Following calibration and validation using the 3 user class model, the out-turn car matrices

are segmented into 6 user classes as required by the DfT. This process is described in

Section 6.6.6.

6.2 Assignment Procedure and Convergence

6.2.1 There are three iterative loops in SATURN: one within the assignment process, one within

the simulation process and finally an outer loop of assignment followed by simulation. Each

loop runs until it reaches the stopping criteria. The stopping criteria are defined as either the

maximum number of iterations or as a measure of convergence.

6.2.2 The standard Wardrop Equilibrium, using the Frank-Wolfe algorithm, has been used as the

assignment procedure for this model. We set the maximum number of assignment loops

(NITA) to 30, the maximum number of simulation loops (NITS) to 99 and the maximum

number of outer loops (MASL) to 199.

6.2.3 The outer loop convergence criteria have been set to stop the procedure when 99% of the

links (ISTOP) change their flow or delay by 1% (PCNEAR). We set the number of

consecutive iterations for which these criteria had to be met (NISTOP) to four. This is a very

exacting level of convergence compared to the default values in SATURN of 95% of links with

a change of less than 5%. The level of convergence is very important in economic appraisal

as model noise can swamp the scheme benefits if the convergence is not tight.

6.2.4 SATURN produces a number of convergence statistics for the iterative procedures (the

results for the model are shown in Table 6.1):

Delta is reported from the assignment iterations. It is the difference between the

times along the actual routes and the minimum cost routes, summed across the whole

network and expressed as a percentage of the minimum cost times. DELTA is

expected to be below 1%. Table 6.1 shows that the model convergence is well within

the target range;

Epsilon is reported from the simulation iterations. It is a measure of the degree to

which the area under the speed/flow curves is minimised and is expected to be below

2%. Table 6.1 shows that the model convergence is well within the target range; and

P is the proportion of links on which the flows or delays change by less than PCNEAR

% (which has been set to 1% for this model) between outer loop iterations. The final

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Sheffield and Rotherham District SATURN Model 2008 6.2

loop has been quoted, although we ensure that the 99% stopping criteria is achieved

on 4 consecutive loops to ensure the network is converged. Note that SATURN rounds

to the nearest integer and that 98.5 is rounded up to match the 99% stopping

criterion.

Table 6.1 Convergence Statistics

Modelled Hour Model Assignment

Delta (%)

Simulation

Epsilon (%)

Outer Loop (P)

(PCNEAR=1%)

Morning Peak 6 user class 0.018 0.024 98.9 (45 loops)

Inter-peak 6 user class 0.020 0.012 99.0 (34 loops)

Evening Peak 6 user class 0.055 0.032 98.8 (47 loops)

6.3 User Classes

6.3.1 The final versions of the model employs six segments of demand, but the matrix estimation

stage was undertaken with only a single segment for cars because counts are not available

separately for the three classes of cars.

6.3.2 The six user class version consists of:

cars – employer’s business;

cars – commute and other - low income;

cars – commute and other - medium income;

cars – commute and other - high income;

light goods vehicles (LGVs); and

other goods vehicles (OGVs).

6.3.3 Flows can be output separately by user class for each version of the model, to be used for

economic and environmental appraisal purposes.

6.3.4 Bus and tram flows, operated on fixed routes, are pre-loaded onto the road network prior to

the assignment of the trip matrices.

6.4 Generalised Cost Formulation

6.4.1 The SATURN assignment procedure builds paths through the network based on a behavioural

generalised cost formulation. This is a linear combination of time and distance with the

following form:

Cost (in pence) = PPM * time (in minutes) + PPK * distance (in km)

6.4.2 The values for PPM, PPK, time and distance are presented in Table 6.2

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6.4.3 The actual values used in the model are in the columns titled PPM and PPK, which is an

equivalent, and possibly more familiar, method of formulating the generalised cost in units of

“in-vehicle” time rather than pence. Units of pence have been chosen because tolls and

parking charges can be directly input in pence, with the result that the numbers in the

SATURN output print files are in the correct units.

6.4.4 The values have been calculated for 2008 using the data and formulae in WebTAG (as

published in June 2004).

6.4.5 The advantage of calculating PPM and PPK using published figures is that they are consistent

with the published values of time for considering tolls or charging regimes as well as the

other models in the South Yorkshire LTP area. The values of time are also consistent with

those in the other modules of SRTM 3 (the PT and demand models).

6.4.6 The following points can be made about the six user class values:

The PPM values vary by time period, as the percentage of Commute / Other trips

within the High / Medium / Low income bands varies from one time period to the next;

The inter-peak values of time are the highest (out of the 3 separate income bands),

followed by the Evening Peak and Morning Peak. This is because, as mentioned earlier,

‘Other’ has a higher PPM value than ‘Commute’. Therefore the time period where the

ratio between ‘other’ and ‘commute’ is at its highest (Inter-peak) will have the highest

PPM values for the different income bands. Accordingly, this ratio is lowest in the

Morning Peak, which has the lowest PPM values.

The higher income users have a higher value of time, hence a higher value for PPM.

Table 6.2 Generalised Cost Parameters – Six User Class

Morning Peak Inter-peak Evening Peak

User Class PPM PPK PPM PPK PPM PPK

Cars Employer’s

Business

48.40 12.20 48.40 12.20 48.40 12.20

Car Other – Low Income 7.88 6.28 9.91 6.28 8.85 6.28

Car Other – Medium

Income

10.73 6.28 12.66 6.28

11.70 6.28

Car Other – High Income 14.25 6.28 15.45 6.28 14.78 6.28

LGV 19.53 13.62 19.53 13.62 19.53 13.62

OGV 16.28 40.17 16.28 40.17 16.28 40.17

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Calibration Procedure

6.4.7 Calibration is the process of adjusting the model to improve the fit to the observed data in

two main areas:

adjustments to the coded links and junctions in the network; and

adjustments to the elements of the matrix that were synthesised.

6.4.8 The calibration process was guided by comparison of link flows with observed flows at

individual survey sites, and through comparing modelled journey times with those observed

in surveys.

6.4.9 Adjustments to network specifications were made in order to improve the fit between

modelled estimates and observed link flows and journey times. Care was taken to ensure

that any changes made improved the situation by making the model a better representation

of conditions on the ground. Unrealistic changes to improve the fit were avoided.

6.4.10 After changes were made to the network, the full cycle of matrix estimation (commencing

with the original matrix) was repeated. This avoided retaining matrix changes that occurred

as a result of errors in the network that were subsequently corrected. Each stage of matrix

estimation concentrated on a specific user class.

6.5 Development of the 6 User Class Models

6.5.1 Matrix estimation used matrices of cars, LGVs and OGVs, the three journey purposes for cars

having been summed to match the level at which counts are available. After calibration we

split the car matrix back into the 14 journey purpose level at which the fully observed

matrices were built and at which the gravity model was run.

6.5.2 This process was run as follows:

Prior car matrices were created for all 12 car journey purpose segments, along with

LGV and OGV, from the roadside interview survey data and the synthetic data.

The journey purpose segments were then combined to create the prior car matrices,

which were run through matrix estimation to produce the final car matrices.

Using a 100 sector system, the difference between the prior and final car matrices was

calculated. These factors were then applied to the original 12 journey purpose matrices

prior to matrix estimation, creating 12 final car matrices, segmented by the

appropriate journey purposes.

6.5.3 This process ensures that we have the same split after matrix estimation as before, and that

this is consistent with the DfT guidelines.

6.5.4 The benefit of using a 100 sector system is that whilst splitting at a zonal level may result in

some zero cell values creating errors in the process, and splitting at the 9 sector level is too

coarse, the 100 sector level provides a good compromise. This sector system is the same

system that was used to smooth the original fully observed highway demand matrices.

6.5.5 These 12 out-turn were required for input into Demand Model (SRDM3).

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6.5.6 The 12 car matrices after matrix estimation, as detailed in 6.6.5, were then put into the

relevant income band – low, medium and high. It should be noted that the “Car - home-

based employer’s business” and “Car - non home-based employer’s business” segments were

not segmented by income, as these are simply combined to produce the final ‘Car –

employer’s business’ matrix.

6.5.7 A procedure was developed to calculate income segmentation for consumer purposes by re-

weighting a sample of National Travel Survey (NTS) data to make it representative of

Sheffield and Rotherham zones

6.5.8 The process works as follows:

For each zone in Sheffield and Rotherham, the NTS sample was re-weighted to the

particular population and economic characteristics of the zone;

For each zone, each trip in the NTS sample was allocated to a demand segment

(purpose, car availability, income group) and distance band, enabling a table to be

produced of the form ‘Zone, Segment, Distance Band, Trips’;

In this way, the shares of trips for the three income categories (low, medium and high

income) were calculated for each zone, purpose, car availability and distance segment.

6.5.9 The final step was to combine the income segmented journey purpose matrices to create low

income, medium income and high income matrices.

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7 Validation

7.1 Introduction

7.1.1 This chapter presents the results of the 6 user class model validation, with the results

presented under the following headings:

calibration count comparisons;

cordon validation;

important count sets;

independent count validation;

journey time comparison;

inspection of typical O-D routes;

matrix characteristics;

trip length distributions;

trip ends; and

origin – destination pairs.

7.2 Calibration count comparisons

7.2.1 A key tool in presenting how well a model performs is to compare the modelled flows against

observed vehicle flows from traffic counts.

7.2.2 As almost all counts were used in calibration of the model, this section is correctly entitled

calibration count comparisons. The comparison of counts to the model flows was undertaken

at a detailed site level using three measures of model performance against observed data,

which are described in turn within this section:

R-squared (R2);

GEH statistic; and

DMRB guideline;

7.2.3 This section presents the comparisons of modelled flows against observed flows. The

comparisons are grouped into a number of categories to highlight different areas of the

model’s performance:

all calibration counts – a headline figure that provides a summary of the goodness of

fit of the modelled flows to observed counts;

cordon totals – these examine whether the model exhibits any systematic bias; and

independent counts – these are a subset of counts that were excluded from matrix

estimation.

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R-Squared Statistic

7.2.4 The R2 coefficient is a measure of the goodness-of-fit of a linear regression model of the

form Y = A + BX, relating the modelled flow Y to the observed flow X. The regression line

has intercept A and slope B. The R2 coefficient takes a value between zero and one and it

represents the proportion of the variability in the data that is explained by the linear

regression model.

7.2.5 In the case of a traffic assignment model, we are aiming for a situation where the modelled

flows match the counts directly. The R2 coefficient is therefore only valid as a measure of

the goodness-of-fit of the traffic model if the intercept of the regression line is not

significantly different from zero and the slope of the regression line is not significantly

different from one. Therefore an adjusted version, based on a model of the form Y = X, is

presented, which is always lower than or equal to the standard version of the statistic.

GEH Statistic

7.2.6 The analysis of the modelled and observed flows also makes use of the standard GEH

statistic, which is defined as:

)flow modelledflow observed(5.0)flow modelledflow observed( 2

+×−

=GEH

7.2.7 The reason that the GEH statistic is used is the inability of either the absolute or relative

difference measure to cope over a wide range of flows. The GEH statistic is a measure that

looks at both the difference between count and modelled flows, and at the size of each

observation. Thus, where flows are high a low value of GEH can only be achieved where the

percentage difference between observed and modelled flows are small. However, where

flows are very low even quite sizeable percentage discrepancies are considered acceptable.

7.2.8 Note that all GEH values have been calculated based on vehicle flows, by dividing the OGV

count and flow by 2 to move from pcu’ which the assignment uses, to vehicles.

DMRB Guidelines

7.2.9 The DfT guidelines for the validation of highway models are based on those laid out in the

Design Manual for Roads and Bridges (DMRB) Volume 12, Section 2, Part 1, Chapter 4. In

respect of the count comparisons presented in this section there are two separate sets of

criteria against which the counts and modelled flow comparison should be measured. In

both cases the criteria are expected to be met in 85% of cases. The two sets of criteria are:

GEH Statistic:

− links should have a GEH value of less than 5;

DMRB Vehicle Flow Comparison. A link passes the DMRB guidelines if;

− where observed flow is less than 700 vehicles per hour, the modelled flow

should be within 100 vehicles of the observed flow;

− where observed flow is between 700 and 2700 vehicles per hour, the modelled

flow should be within 15% of observed flow; and

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− where observed flow is greater than 2700 vehicles per hour, the modelled flow

should be within 400 vehicles of the observed flow.

7.2.10 In Tables 7.1 and 7.2 overleaf, we have reported on:

The R squared value – a measure of the goodness of fit between modelled flows and

observed counts;

GEH statistics – the % of all links with a GEH value less than 5;

DMRB guideline – the percentage of links that pass the ‘DMRB Vehicle Flow

Comparison’, as detailed in section 7.7.9; and

Modelled / Observed – the ratio of total modelled flows to total observed counts across

the whole modelled area.

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All Calibration Counts

7.2.11 The calibration counts are the ones that were used in matrix estimation. We used a total of

2,200 counts, a mixture of turn counts and link counts.

Table 7.1 Validation against all Calibration Counts prior to Matrix Estimation

(all figures expressed as percentages)

R2 GEH <5 DMRB

Guideline countedmodelled

Morning Peak

Car 0.88 41 57 100

LGV 0.88 87 99 93

OGV 0.89 91 98 123

Total 0.90 41 56 101

Inter-peak

Car 0.86 42 63 91

LGV 0.81 82 96 108

OGV 0.93 87 98 138

Total 0.90 43 61 97

Evening Peak

Car 0.88 41 56 97

LGV 0.89 91 100 93

OGV 0.91 96 98 177

Total 0.91 42 55 98

7.2.12 The car user classes for the 2008 model have been derived solely from the observed data,

using a gravity model to infill the non-fully observed movements. The GEH statistic of

between 41% and 44% links with a GEH less than 5 for all time periods is broadly consistent

with other models of large urban areas that MVA have developed and subsequently used

successfully.

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7.2.13 It is difficult to obtain accurate gravity model estimates of non-fully observed LGV and OGV

trip patterns, and for these user classes we took the 2006 final matrix (factored to 2008) and

used this to infill the 2008 matrix.

Table 7.2 Validation against all Calibration Counts after Matrix Estimation

(all figures expressed as percentages)

R2 GEH <5 DMRB

countedmodelled

Morning Peak

Car 0.98 82 90 98

LGV 0.95 95 100 96

OGV 0.90 95 99 102

Total 0.98 79 88 98

Inter-peak

Car 0.98 86 94 99

LGV 0.93 95 99 97

OGV 0.92 95 100 104

Total 0.98 82 91 99

Evening Peak

Car 0.98 81 91 98

LGV 0.95 96 100 95

OGV 0.92 99 99 101

Total 0.98 79 89 97

7.2.14 The DMRB guidelines are met for all three time periods – the actual figures are 88%, 91%

and 89% for Morning Peak, Inter-peak and Evening Peak respectively. Whilst the three time

periods have very similar networks, the inter-peak has the lowest demand, followed by the

morning peak and then the evening peak, which has the highest demand.

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7.2.15 The GEH guidelines are almost met for the three time periods – the actual figures for all

vehicles are 79%, 82% and 79%. The figures look a little better when we consider cars on

their own: 82%, 85% and 81%. LGV and OGV are excellent ranging between 96% and

100%.

Table 7.3 Comparison of modelled flows against observed counts (All vehicles

combined)

Y = ax

(Slope)

DMRB

Pass / Fail

R squared DMRB

Pass /

Fail

Total 0.98 Pass 0.98 Pass

Car 0.99 Pass 0.98 Pass

LGV 0.95 Pass 0.95 Pass

Morning

Peak

OGV 0.90 Pass 0.90 Fail

Total 0.98 Pass 0.98 Pass

Car 0.99 Pass 0.99 Pass

LGV 0.95 Pass 0.95 Pass

Inter-peak

OGV 0.91 Pass 0.91 Fail

Total 0.98 Pass 0.98 Pass

Car 0.98 Pass 0.98 Pass

LGV 0.94 Pass 0.95 Pass

Evening

Peak

OGV 0.80 Pass 0.92 Fail

7.2.16 Table 7.3 above details the count correlation against DMRB guidelines. Looking at total

vehicle flows, all time periods exceed the DMRB criteria for both the slope and R squared

value, apart from OGV.

7.2.17 Given that all of the time periods exceed the DMRB guidelines stated in Table 7.2 and Table

7.3, we are pleased with the model performance. Every attempt is made to perform counts

when network conditions are consistent, such as avoiding school holidays and periods where

roadworks are being undertaken. However it is inevitable that there are inconsistencies

between counts, arising from:

day to day variability in traffic;

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short term changes in traffic capacity due to weather conditions, accidents and vehicle

breakdowns;

land use changes in the area such as a new factory or a housing estate being built;

and

traffic in the vicinity of older counts not growing at the average rate we have used in

factoring up the count.

7.2.18 Because some counts are inconsistent, calibrating the model to satisfy one set of counts can

lead to comparisons with other counts deteriorating. Therefore, as models become larger

and use more counts, they become harder to calibrate to meet the DMRB guidelines. It is a

paradox that as we use more counts in calibration in an attempt to improve the model, it

becomes harder to match all the counts used, and therefore the validation statistics can look

poorer (despite our belief that the model is in fact a better representation of reality).

Link Count Plots

7.2.19 Figure 7.1 to Figure 7.3 show the validation of all the link counts with respect to the DMRB

guidelines. Green flows indicate acceptable flows, with blue representing a degree of under-

assignment and red representing some over-assignment.

Figure 7.1 Link Flow Validation Plot - Morning Peak

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Figure 7.2 Link Flow Validation Plot - Inter-peak

Figure 7.3 Link Flow Validation Plot - Evening Peak

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7.2.20 We can conclude from the figures above that the vast majority of links are coloured green,

meaning that they pass the DMRB guidelines. For those links that fail, there is a balance

between red (flow too high) and blue (flow too low) in all networks, which suggests there is

no systematic bias whereby the model over-estimates or under-estimates flows.

7.2.21 Furthermore, those links that fail are spread across the conurbation, signifying that there is

no specific area where the model validates poorly.

7.2.22 Given the large number of counts that we have in the model, and the limiting criteria that

were applied to each zone during matrix estimation to stop unrealistic growth in trips, we are

satisfied that the model validates acceptably.

7.3 Cordon Validation

7.3.1 The DMRB refers to the GEH statistics, requiring it to be less than 4 for the total flows across

screenlines or cordons for “all (or nearly all) screenlines”.

7.3.2 We have two cordons used for the calibration and validation of the model;

Sheffield City Centre Cordon – 18 sites, in general just outside of the Inner Ring Road;

and

Rotherham Town Centre Cordon – 11 sites, just outside of Rotherham Town Centre.

7.3.3 Figure 7.4 shows the locations of these cordons, together with the other key count sets.

7.3.4 Several counts, particularly on the BRT corridors, are in multiple key count sets.

Figure 7.4 Location of Key Counts

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7.3.5 Tables 7.4 and 7.5 below show the total volume of vehicles crossing each cordon, by time

period and by direction, before and after matrix estimation. The GEH statistic compares the

total modelled flow with the total observed flow.

Table 7.4 Screenline Flows across Sheffield and Rotherham Cordons – Before

Matrix Estimation

Morning Peak Inter-peak Evening Peak

Screenline Mod Obs Links GEH Mod Obs Links GEH Mod Obs Links GEH

Sheffield City -

Inbound

14,064

14,940 6% 7.3

8,648

9,310 8% 7.0

9,625

10,893 13% 12.5

Sheffield City -

Outbound

8,922

8,955 0% 0.3

8,965

8,963 0% 0.0

13,109

13,482 3% 3.2

Rotherham Town

- Inbound

7,179

6,493 -10% 8.3

5,188

4,784 -8% 5.7

5,659

5,082 -10% 7.9

Rotherham Town

- Outbound

4,931

4,512 -9% 6.1

5,465

4,732 -13% 10.3

7,871

7,068 -10% 9.3

7.3.6 The flows across each screenline are generally satisfactory before matrix estimation, ranging

from 13% under assignment to 13% over-assignment.

7.3.7 The percentage of links across each screenline with individual GEH values less than 5 are, for

the morning peak, inter-peak and evening peak respectively:

Sheffield City – Inbound – 50%, 35% and 35%;

Sheffield City – Outbound – 39%, 33%, 33%;

Rotherham Town Centre – Inbound – 73%, 82%, 73%; and

Rotherham Town Centre – Outbound – 55%, 73%, 36%.

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Table 7.5 Screenline Flows across Sheffield and Rotherham Cordons – After Matrix

Estimation

Morning Peak Inter-peak Evening Peak

Screenline Mod Obs Links GEH Mod Obs Links GEH Mod Obs Links GEH

Sheffield City -

Inbound

14,064

13,820 -2% 2.1

8,648

8,590 -1% 0.6

9,625

9,826 2% 2.0

Sheffield City -

Outbound

8,922

9,075 2% 1.6

8,965

8,914 -1% 0.5

13,109

13,125 0% 0.1

Rotherham Town

- Inbound

7,179

7,330 2% 1.8

5,188

5,483 6% 4.0

5,659

5,908 4% 3.3

Rotherham Town

- Outbound

4,931

5,072 3% 2.0

5,465

5,486 0% 0.3

7,871

7,658 -3% 2.4

7.3.8 The GEH value for the screenline crossings is less than or equal to 4 for all directions and

time periods.

7.3.9 The percentage of links across each screenline with individual GEH values less than 5 are;

Sheffield City – Inbound – 75%, 80%, 90%;

Sheffield City – Outbound – 72%, 94%, 78%;

Rotherham Town Centre – Inbound – 91%, 91%, 82%;

Rotherham Town Centre – Outbound – 91%, 91%, 91%.

7.3.10 Analysis of the links crossing each cordon where the GEH value is greater than 5 shows that

most of these links are minor roads where the observed flow is low, typically less than 700

vehicles per hour.

7.4 Important Count Sets

7.4.1 Whilst we calibrated the model for all counts in Sheffield and Rotherham, we made special

effort to ensure the model would be fit for forthcoming applications of the model. With this

in mind, attention was paid to the count validation along the following corridors;

Sheffield to Rotherham via Waverley – BRT Southern Route;

Sheffield to Rotherham via Meadowhall – BRT Northern Route;

Penistone Rd;

Ecclesall Rd;

Sheffield City Centre Cordon; and

Rotherham Town Centre cordon.

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7.4.2 The results of the validation for these count sets are shown in Table 7.6.

Table 7.6 Validation against Important Count Sets after Matrix Estimation

(all figures expressed as percentages)

Morning

Peak

Inter-peak Evening

Peak

DMRB GEH

< 5

DMRB GEH

< 5

DMRB GEH

< 5

Sheffield to Rotherham –

BRT Southern 84% 89% 95% 100% 84% 100%

Rotherham to Sheffield –

BRT Southern 94% 94% 94% 94% 100% 100%

Sheffield to Rotherham –

BRT Northern 100% 100% 91% 91% 82% 82%

Rotherham to Sheffield –

BRT Northern 92% 92% 83% 75% 100% 100%

Penistone Rd - Inbound 94% 94% 88% 88% 75% 81%

Penistone Rd - Outbound 79% 86% 93% 86% 86% 86%

Eccdelsall Rd - Inbound 80% 90% 100% 100% 80% 100%

Eccdelsall Rd - Outbound 89% 89% 100% 100% 100% 100%

Rotherham Town Centre

Cordon - Inbound 91% 91% 91% 91% 82% 82%

Rotherham Town Centre

Cordon - Outbound 91% 91% 91% 100% 91% 100%

Sheffield City Centre

Cordon - Inbound 75% 75% 80% 75% 90% 90%

Sheffield City Centre

Cordon - Outbound 72% 94% 94% 94% 78% 83%

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7.4.3 Table 7.6 shows that all the routes that pass through areas for which major schemes are

planned validate well;

Rotherham to Sheffield (via Waverley) – BRT Southern Route;

− This route validates well across all time periods and directions;

Rotherham to Sheffield (via Lower Don Valley) – BRT Northern Route;

− This route validates well across all time periods and directions;

Penistone Rd;

− Penistone Rd generally validates well in all time periods, with the AM (Outbound)

and PM (Inbound) narrowly missing the GEH criteria;

Sheffield City Centre;

− As mentioned previously, the links with GEH values greater than 5 are generally

minor roads with low traffic flows. The major arterial routes from / to Sheffield

City Centre generally validate well.

Rotherham Town Centre;

− The Rotherham Town centre cordon validates well, meeting the GEH criteria in

every time period and direction apart from the Evening Peak (Inbound).

7.4.4 Appendix D shows the validation statistics for all individual links that comprise these key

routes and cordons.

7.5 Independent Count Validation

7.5.1 We kept behind an independent count set from the calibration process, in order to

independently verify our matrices.

7.5.2 Figure 3.3 showed the locations of the independent counts set.

7.5.3 Figures 7.5 to 7.7 show the validation against this independent count set. Unsurprisingly,

this validation is not as good as the main count set.

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Figure 7.5 Independent Count Validation Plot – Morning Peak

Figure 7.6 Independent Count Validation Plot – Inter-peak

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Figure 7.7 Independent Count Validation Plot – Evening peak

7.5.4 Table 7.7 shows the percentage of links in the independent count set with the following

characteristics, for each time period;

Modelled Flow;

Observed Flow;

Percentage Difference;

R squared value;

R squared pass / or fail (criteria – 0.90)

Percentage of Links with GEH less than 5 ( criteria – greater than 85%); and

Percentage of Links passing DMRB criteria ( criteria – greater than 85%);.

7.5.5 The independent count validation is not as good as the calibration count set across all time

periods. The percentage difference between the modelled and observed flow is acceptable

and there is also a good correlation between the modelled and observed across the time

periods. Some of the counts are in areas towards the periphery of the model, where the

network is sparse and there are fewer zones. The plots on Figures 7.5 to 7.7 above show

that the counts closer to the centre of Sheffield, where we have a more detailed network

representation, validate more satisfactorily than those counts located on the periphery of the

model.

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Table 7.7 Independent Count Validation Statistics

Screenline Mod Obs Abs

Diff

% Diff % GEH

<5

DMRB Slope R

squared

Pass /

Fail R2

Morning Peak Car

34,325 36,719 2,394 7% 42%

51

1.11 0.87 Fail

LGV

5,531 4,733 (798) -14% 80%

94

0.91 0.87 Fail

OGV

2,575 2,234 (341) -13% 88%

100

0.89 0.95 Pass

Total

42,431 43,686 1,255 3% 40%

51

1.07 0.9 Pass

Inter-peak Car

22,521 26,713 4,192 19% 43%

69

1.18 0.89 Fail

LGV

5,147 5,065 (82) -2% 78%

94

1.11 0.87 Fail

OGV

2,914 2,769 (145) -5% 91%

100

0.94 0.96 Pass

Total

30,582 34,547 3,965 13% 49%

68

1.15 0.93 Pass

Evening Peak Car

39,600 40,544 944 2% 39%

48

1.01 0.90 Pass

LGV

3,918 3,933 15 0% 96%

100

1.02 0.95 Pass

OGV

1,006 1,090 84 8% 97%

100

1.11 0.95 Pass

Total

44,524 45,567 1,043 2% 40%

46

1.02 0.92 Pass

7.6 Journey Time Comparison

7.6.1 Sheffield City Council undertook journey time surveys along 17 two-way routes as presented

in Figure 3.4. Several independent surveys were performed for each route and direction to

provide an average of the journey times. All the journey time routes were fully contained

within the simulation network.

7.6.2 The journey times were also tested against confidence intervals of ±15% (or 1 minute if

greater), which is the standard DMRB guideline.

7.6.3 Table 7.8 presents the results for all journey time routes and time periods, showing the

percentage difference between modelled and observed times and whether they are ‘Fast’,

‘Slow’ or ‘OK’ in relation to the DMRB guidelines.

7.6.4 Table 7.9 summarises the route data, showing overall what percentage of routes within each

time period are ‘Fast’, ‘Slow’ or ‘OK’ in relation to the DMRB guidelines.

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Table 7.8 Journey Times within 15% (or 1 minute if greater)

Morning Peak Inter-peak Evening Peak

Route Mod Obs %Diff DMRB Mod Obs %Diff DMRB Mod Obs %Diff DMRB

1 In 13:51 15:44 -12% OK 13:01 17:22 -25% FAST 13:18 11:46 13% OK

1 Out 11:33 10:21 12% OK 11:00 15:41 -30% FAST 12:19 13:49 -11% OK

2 In 9:30 11:21 -16% FAST 9:08 10:59 -17% FAST 9:03 9:51 -8% OK

2 Out 6:26 6:09 5% OK 9:15 13:36 -32% FAST 9:18 19:49 -53% FAST

3 In 11:31 10:21 11% OK 8:49 10:23 -15% FAST 10:13 9:26 8% OK

3 Out 7:44 6:49 14% OK 7:22 8:17 -11% OK 9:13 9:57 -7% OK

4 In 11:05 10:03 10% OK 9:00 11:24 -21% FAST 11:10 12:41 -12% OK

4 Out 8:01 7:02 14% OK 7:57 9:23 -15% FAST 10:16 10:27 -2% OK

5 In 16:45 20:00 -16% FAST 15:08 21:33 -30% FAST 16:46 14:01 20% SLOW

5 Out 13:24 12:16 9% OK 12:17 21:07 -42% FAST 17:16 20:02 -14% OK

6 In 17:46 16:56 5% OK 16:24 14:58 10% OK 15:19 14:26 6% OK

6 Out 17:29 15:19 14% OK 14:32 14:30 0% OK 14:32 17:12 -16% FAST

7 In 26:45 24:34 9% OK 26:27 27:41 -4% OK 26:30 23:40 12% OK

7 Out 26:50 23:19 15% SLOW 26:44 25:07 6% OK 27:44 26:45 4% OK

9 In 13:17 14:13 -7% OK 12:37 10:47 17% SLOW 13:44 12:53 7% OK

9 Out 11:14 8:20 35% SLOW 10:47 12:03 -10% OK 13:53 19:49 -30% FAST

10 In 21:56 22:12 -1% OK 20:01 30:36 -35% FAST 21:48 21:27 2% OK

10 Out 17:43 16:08 10% OK 17:37 19:03 -8% OK 21:57 22:00 0% OK

11 In 17:45 16:22 8% OK 15:19 15:55 -4% OK 16:23 14:18 15% OK

11 Out 13:53 12:17 13% OK 13:39 13:22 2% OK 15:40 15:15 3% OK

12 In 17:22 16:19 6% OK 14:28 12:09 19% SLOW 19:49 27:30 -28% FAST

12 Out 16:25 16:51 -3% OK 13:03 14:12 -8% OK 16:10 16:19 -1% OK

13 In 29:38 27:53 6% OK 28:23 34:02 -17% FAST 38:00 43:20 -12% OK

13 Out 30:17 32:23 -6% OK 29:39 31:45 -7% OK 33:33 32:31 3% OK

14 In 11:14 15:07 -26% FAST 8:36 11:32 -25% FAST 9:02 10:37 -15% OK

14 Out 10:10 9:22 9% OK 9:21 9:05 3% OK 10:43 10:49 -1% OK

15 In 13:58 16:41 -16% FAST 10:48 15:14 -29% FAST 12:07 13:42 -11% OK

15 Out 12:38 11:24 11% OK 11:38 16:32 -30% FAST 15:36 13:50 13% OK

16 In 11:03 10:25 6% OK 8:26 9:22 -10% OK 11:53 13:37 -13% OK

16 Out 8:49 6:43 31% SLOW 6:09 7:39 -19% FAST 8:52 10:01 -11% OK

17 In 20:01 21:04 -5% OK 14:31 18:07 -20% FAST 19:55 21:04 -5% OK

17 Out 14:19 14:03 2% OK 12:11 12:54 -6% OK 17:30 19:03 -8% OK

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7 Validation

Sheffield and Rotherham District SATURN Model 2008 7.23

Table 7.9 Percentage of Routes passing DfT criteria

Screenline Slow OK Fast

Morning Peak 9 % (3) 78 % (25) 13 % (4)

Inter-peak 6 % (2) 44 % (14) 44 % (14)

Evening Peak 3 % (1) 84 % (27) 13 % (4)

Overall 6 % (6) 69 % (66) 23 % (22)

7.6.5 When judging by DMRB guidelines, 78% of all routes are considered to be acceptable within

the Morning Peak and 84% within the Evening Peak. This is slightly below the DMRB

guidelines which state that 85% of routes should have a modelled journey time within 15%

of the observed journey time.

7.6.6 In the Inter-peak it was discovered that a lot of the journey times crossed into the peak

periods, whereby a route may start at 3.40pm but and finish at 4.30pm, and be classified as

‘Inter-peak’ whereas in reality the delays and journey times were more representative of

peak period traffic conditions. The journey times were altered to reflect the perceived delays

and journey times in the true inter-peak, which was also required because the inter-peak

network speeds would be used within the PT model.

7.6.7 In summary, the problem routes in each time period are as follows;

Morning Peak

− Middlewood (Outbound) – surveyed in 2007, this route is too slow. Shares part

of route with Penistone Rd (Outbound), surveyed in 2008, which validates

satisfactorily.

− Crookes (Outbound) – delays at Glossop Rd / Fulwood Rd not replicated in the

model.

Inter –peak – covered in Section 7.6.6 above.

Evening Peak

− Ecclesall Rd Outbound is too fast. There is a slow moving queue of traffic from

Moore Street roundabout to Hunters Bar Roundabout, which takes 10 minutes to

cover approximately 1 mile. The delay is caused by side roads and ‘friction’

effects on the link, which the more strategic SATURN network does not replicate

effectively. If we did replicate this, traffic would simply re-route around the area

giving un-realistic flows on parallel routes.

− Inner Ring Road Clockwise is too fast. This is again due to slow moving traffic

along a long link creating large delays which are hard for SATURN to model. If

this were modelled correctly, traffic would simply re-route and create problems

elsewhere in the network.

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7 Validation

Sheffield and Rotherham District SATURN Model 2008 7.24

− Middlewood (Outbound) – surveyed in 2007, this route is too fast. Shares part of

route with Penistone Rd (Outbound), surveyed in 2008, which validates

satisfactorily.

7.6.8 Given the size of this model and the difficulties that large models experience in obtaining the

GEH statistics given by the DfT (that were designed with smaller models in mind) we can

conclude that the journey time validation is acceptable.

7.6.9 Appendix E presents the journey time summary table in more detail. For each route and time

period combination, the following information is presented for the whole route and by route

section:

DMRB Criteria – OK (pass), Fast (fail) or Slow (fail);

modelled journey time;

observed journey time;

absolute difference between modelled and observed; and

percentage difference between modelled and observed.

7.7 Inspection of Typical O-D Routes

7.7.1 Just as important as the count and journey time validation is the routing within the model.

It is vital that key strategic routes are well represented within the model. Appendices F 1 to

F3 show the results of the routing between given origin and destination zones. The following

routes have been chosen to demonstrate that routings are plausible. All routes are on or

near to major highways and / or land developments for which the model will be used to

appraise.

7.7.2 The routes in each Appendix (F1 – Morning Peak, F2 – Inter peak and F3 – Evening Peak) are

as follows:

Figs 1 and 2 - Sheffield City Centre Zone 17 to Ecclesall Rd (and vice versa);

Figs 3 and 4 - Sheffield City Centre Zone 7 to Ecclesall Rd (and vv);

Figs 5 and 6 - Sheffield City Centre to Hillsborough (and vv);

Figs 7 and 8 – North access to Lower Don Valley (and vv);

Figs 9 and 10 – South access to Lower Don Valley (and vv);

Figs 11 and 12 - Sheffield City Centre to Rotherham (and vv);

Figs 13 and 14 - Through trips across Sheffield City Centre – North to South (and vv);

Figs 15 and 16 - Through trips across Sheffield City Centre – East to West (and vv); &

Figs 17 and 18 - Sheffield City Centre to Waverley.

7.7.3 The Green bandwidths alongside the red lines represent the proportion of traffic assigned to

that particular route; the thicker the green line the larger the proportion of traffic on that

route.

7.7.4 The plots show that the model has assigned traffic to sensible routes for the given origins

and destinations.

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7 Validation

Sheffield and Rotherham District SATURN Model 2008 7.25

7.8 Matrix Characteristics

7.8.1 Matrices before and after matrix estimation have been aggregated into 8 sectors to allow

comparison at this aggregate level. The trips matrix summaries are presented in Appendix

G. The larger changes are concentrated around trips within the Sheffield urban area, which

is to be expected as 50% of the data has been derived from synthetic data sources.

Considering this, we believe that the changes in sector-to-sector matrix movements are

reasonable.

7.8.2 Tables 7.10 summarises the hourly 6 user class trip matrices after matrix estimation.

Table 7.10 Summary of Hourly 6 user class Trip Matrices (pcus)

Before Matrix

Estimation

After Matrix

Estimation

Percentage

Difference

Morning Peak

Car – Employers Business 11,634 12,943 11%

Car – Commute and Other - Low

income 18,367 19,722 7%

Car – Commute and Other -

Medium income 31,078 32,481 5%

Car – Commute and Other - High

Income 33,870 33,986 0%

Car Total 94,949 99,132 4%

LGV 12,349 13,078 6%

OGV 11,721 9,981 -15%

Total 119,019 122,196 3%

Inter-peak

Car – Employers Business 13,606 15,319 13%

Car – Commute and Other - Low

income 17,071 19,735 16%

Car – Commute and Other -

Medium income 18,623 21,415 15%

Car – Commute and Other - High

Income 19,967 22,063 10%

Car Total 69,267 78,532 13%

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Sheffield and Rotherham District SATURN Model 2008 7.26

Before Matrix

Estimation

After Matrix

Estimation

Percentage

Difference

LGV 13,296 13,035 -2%

OGV 13,801 11,579 -16%

Total 96,368 103,151 7%

Evening Peak

Car – Employers Business 9,182 10,104 10%

Car – Commute and Other - Low

income 24,532 27,015 10%

Car – Commute and Other -

Medium income 34,910 37,500 7%

Car – Commute and Other - High

Income 37,522 38,469 2%

Car Total 106,146 113,028 6%

LGV 10,628 10,964 3%

OGV 7,365 4,672 -37%

Total 124,143 128,730 4%

7.8.3 As previously mentioned, approximately 50% of trips within the matrix were derived from

synthetic data. Given this, and the substantial number of traffic counts used for matrix

estimation which can produce large numbers of short distance trips, the changes in matrix

totals for cars after matrix estimation are reasonable.

7.8.4 The OGV matrices have decreased, particularly in the Evening Peak. This decrease is due to

an excessive number of trips along the M1 passing through the study area, which matrix

estimation has factored down. The changes in OGV flows for trips to / from and within the

study area after matrix estimation is below 10%.

7.9 Trip Length Distribution

7.9.1 The distributions of trip lengths within the model are shown in Figures 7.8 to 7.10 for all

vehicles combined, by time period. The variation in trip length distribution, for Car, LGV and

OGV, are provided in Appendix H.

7.9.2 Table 7.11 below also shows the variation in average trip length distribution for car trips

between the prior and post ME matrices. This includes all trips within the network, including

trips that travel through the study area.

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7 Validation

Sheffield and Rotherham District SATURN Model 2008 7.27

Morning Peak Trip Length Distribution - All Vehicles

0

5

10

15

20

25

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure 7.8 Trip Length Distribution – Morning peak

Inter Peak Trip Length Distribution - Total Vehicles

0

5

10

15

20

25

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure 7.9 Trip Length Distribution – Inter-peak

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Sheffield and Rotherham District SATURN Model 2008 7.28

Evening Peak Trip Length Distribution - Total Vehicles

0

2

4

6

8

10

12

14

16

18

20

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure 7.10 Trip Length Distribution – Evening-peak

7.9.3 Matrix estimation has a tendency to create many short distance trips in order to match the

traffic counts it is presented with. Given that we applied matrix estimation first to the

synthetic cells within the matrix, which tend to have a shorter trip length than the longer

distance trips that cross the cordons and will hence be fully observed, we would expect the

average trip length to be reduced.

Table 7.11 Average Car Trip Lengths Before and After Matrix Estimation

Average Trip Length

(kilometres)

Before ME After ME

Morning Peak 26.8 25.6

Inter-peak 26.5 22.9

Evening Peak 23.4 23.2

7.9.4 Overall, the average trip length has been reduced in all time periods. This is in part to be

expected, given the reasons listed above. The reduction in trip length, however, is relatively

small and we are confident that matrix estimation has not un-realistically altered the trip

lengths within the model.

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Sheffield and Rotherham District SATURN Model 2008 7.29

7.9.5 Table 7.12 below shows the average trip lengths in the prior matrices, segmented into the 14

journey purposes from which the matrices were built and what is required for the demand

model. This data in Table 7.12 is only for trips to, from and within the study area, and hence

the average trip lengths presented in Table 7.11 above will be greater than an aggregate of

the data in Table 7.12

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Sheffield and Rotherham District SATURN Model 2008 7.30

Table 7.12 Average Car Trip Lengths Before Matrix Estimation – All User Classes,

to, from and within Study Area

Morning Peak Inter-peak Evening Peak

No of

Trips

Average

Trip

Length

(km)

No of

Trips

Average

Trip

Length

(km)

No of

Trips

Average

Trip

Length

(km)

Home to Work

53,556 14 3,113 14 2,738

13

Work to Home

1,495 15 6,189 13

47,197

14

Home to EB

5,552 33 1,326 33

448

29

EB to Home

229 22 1,638 30 4,298

34

Home to

Education 5,873 9 1,012 9 1,253

7

Education to

Home 937 8 1,833 8 2,106

10

Home to

Shopping 1,368 10 5,589 10 3,019

10

Shopping to

Home 172 8 5,738 10 4,128

11

Home to Other

5,877 14 7,769 14 7,759

13

Other to Home

1,933 14 9,014 13

10,549

13

Non Home

Based EB 3,900 25 7,198 26 2,910

28

Non Home

Based Other 5,271 12 11,562 12

11,484

13

LGV

5,875 25 5,869 22 4,297

25

OGV 3,716 43 4,673 43 1,353 42

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Sheffield and Rotherham District SATURN Model 2008 7.31

Total

(excluding

LGV and OGV) 86,163 15 61,980 14 97,888 12

7.10 Trip Ends

7.10.1 The trip ends before and after matrix estimation are presented in this section below. Table

7.13 shows the correlation between prior and post matrix estimation trip ends at Origin and

Destination levels.

Table 7.13 Correlation between Trip end totals before and after matrix estimation

Origin Trip Ends Destination Trip Ends

R Squared Y = ax R Squared Y = ax

Morning Peak 0.907 y = 0.94x 0.898 y =0.96x

Inter-peak 0.921 y = 1.00x 0.913 y =0.98x

Evening Peak 0.887 y = 0.97x 0.891 y = 0.98x

7.10.2 Matrix estimation will changes trip ends in order to match link counts, factoring up (and

down) relevant origin-destination movements. We have looked at trip ends to ensure that

these changes do not radically alter origin or destination totals and, importantly, do not

radically alter the distribution of trips.

7.10.3 Figures 7.11 to 7.16 plot this data for all three time periods, focussing on all user classes

combined. Appendix H contains individual plots showing the changes in trip ends before and

after matrix estimation for all time periods and user classes.

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Sheffield and Rotherham District SATURN Model 2008 7.32

Morning Peak Total - Differences between Prior and Post ME Origin Vehicle Trip Ends

y = 0.9426xR2 = 0.9072

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.11 Morning Peak Origin Trip Ends

Morning Peak Total - Differences between Prior and Post ME Destination Vehicle Trip Ends

y = 0.9552xR2 = 0.898

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.12 Morning Peak Destination Trip Ends

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Sheffield and Rotherham District SATURN Model 2008 7.33

Inter peak Total - Differences between Prior and Post ME Origin Vehicle Trip Ends

y = 1.0014xR2 = 0.921

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.13 Inter Peak Origin Trip Ends

Inter peak Total - Differences between Prior and Post ME Destination Vehicle Trip Ends

y = 0.9843xR2 = 0.9126

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.14 Inter Peak Destination Trip Ends

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Evening Peak Total - Differences between Prior and Post ME Origin Vehicle Trip Ends

y = 0.9772xR2 = 0.8872

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.15 Evening Peak Origin Trip Ends

Evening Peak Total - Differences between Prior and Post ME Destination Vehicle Trip Ends

y = 0.9757xR2 = 0.891

0

200

400

600

800

1000

1200

1400

0 200 400 600 800 1000 1200 1400

Pre ME

Post

ME

Figure 7.16 Evening Peak Destination Trip Ends

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Sheffield and Rotherham District SATURN Model 2008 7.35

7.10.4 The correlation is very good between the trip ends before and after matrix estimation. For all

time periods, the R2 value, and indication of the goodness of fit between two datasets, is

greater than 0.89. This suggests that whilst matrix estimation does change certain origin-

destination movements, it does not introduce large changes to the trip distribution and the

overall distribution of trips in the prior matrix is accurate.

7.10.5 Constraints where applied at a zonal trip end level to the prior matrix in order to prevent

unrealistic changes at a trip end level between the prior and post ME matrices. Whilst ME

attempts to stick to these constraints, sometimes it can’t.

7.10.6 Table 7.14 below shows, for Origins and Destinations for all time periods and user classes,

the percentage of all zones where the increase in the number of trips before and after matrix

estimation is greater than 50%, the percentage of zones where the decrease in the number

of trips after matrix estimation is greater than 50%, and the percentage of trip ends where

the change has a GEH value less than 5.

Table 7.14 Changes in Trip Ends Before and After Matrix Estimation

% of trip

ends > 50%

growth

% of trip

ends > 50%

decrease

% of trip

ends

changed by

less than

50%

% of trip

ends with

GEH less

than 5

Morning Peak Orig 26% 7% 67% 74%

Dest 16% 12% 72% 71%

Inter-peak Orig 12% 6% 82% 82%

Dest 15% 4% 81% 83%

Evening Peak Orig 16% 12% 82% 70%

Dest 19% 10% 71% 74%

7.10.7 Many of the zones where trips have changed by more than 50% are zones where the

existing demand is very low, and hence a large percentage change does not always equate

to a large absolute change in the number of trips.

7.10.8 The GEH value takes into account instances where there could be a large percentage change

in trips ends, greater than 50%, but a low absolute increase in flow. Overall, nearly three-

quarters of trips ends in the morning and evening peak are modified by matrix estimation

such that the GEH value is less than 5. This ratio increase to 80% for the inter-peak.

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Sheffield and Rotherham District SATURN Model 2008 7.36

7.10.9 From the data we can conclude that the trip end constraints have worked well, and that the

number of zones that have experienced large charges in trips between the prior and post ME

matrices have been minimised.

7.11 Origin Destination pairs

7.11.1 The analysis of the changes in trip ends shows a very good correlation between the trip ends

before and after matrix estimation. Taking this analysis one level further, we have looked at

changes between the prior and post ME matrices at an O-D level.

7.11.2 Table 7.15 shows these changes for Car, LGV and OGV.

Table 7.15 Correlation between Origin-Destination pairs before and after matrix

estimation

O-D Trips

R Squared Y = ax

Morning Peak Car 0.6513 0.893

LGV 0.8317 1.009

OGV 0.8191 0.511

Inter-peak Car 0.7635 0.941

LGV 0.7654 1.001

OGV 0.8649 0.670

Evening Peak Car 0.7059 1.058

LGV 0.8309 0.845

OGV 0.8673 0.640

7.11.3 As expected, this correlation (based upon the R squared value) is not as good as for the trip

ends, as in a lot of instances we are dealing with many small numbers in the prior matrix.

The table does show that there is a decent correlation between prior and post ME matrices at

the very detailed O-D level, showing that we are not radically altering the distribution and

magnitude of trips in the prior matrix in order to reach the DMRB criteria.

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Sheffield and Rotherham District SATURN Model 2008 8.1

8 Summary and Conclusions

8.1 Summary

8.1.1 This report has detailed the steps undertaken to update the SATURN Model of Sheffield and

Rotherham by rebasing it to 2008 and recalibrating it across the whole study area. The new

SRHM3 model represents the morning peak, inter-peak and evening peak modelled hours.

8.1.2 The overall geographic coverage has been retained from the 2007 versions of the model

(SRHM2), the network representing all motorways, A, B and C and bus routes in the districts

of Sheffield and Rotherham. The model has been slightly refined in some areas to aid

calibration.

8.1.3 Fully observed matrices were created from a series of 106 roadside interview surveys

undertaken between 2005 and 2008:

3 new sites surveyed in March 2008 in the Waverley area;

50 new sites conducted in Autumn 2007 to improve the capture of trips entering

Sheffield City Centre and Rotherham Town Centre, the Meadowhall screenline and the

motorway screenline (SWYMM’s update);

42 sites conducted in Spring 2006 to improve the capture of trips in the Sheffield

District; and

11 sites conducted in 2005 to improve the capture of trips in the Rotherham District.

8.1.4 Non-fully observed movements were obtained from a gravity model for car, and from a

previous version of the model for LGV and OGV.

8.1.5 Traffic signal timings were updated where necessary using information supplied by the Urban

Traffic Control (UTC) teams from Sheffield City Council and Rotherham Borough Council.

8.1.6 The model employs tight convergence criteria for the assignment, specifically ISTOP set to

99 and NISTOP set to 4. This is considerably tighter than what is required by the DfT for

economic appraisal.

8.1.7 The model has met or is very close to the guidelines in DMRB in the following areas:

count comparisons by vehicle type;

count comparisons for important count sets;

journey time comparisons;

link lengths compared to crow fly distances;

junction coding compared against aerial photographs and site visits; and

modelled routes checked by inspection for plausibility.

8.1.8 The model has been developed with 6 user classes including income segmentation for car

users. This is so that the model is sufficiently flexible that it can be used to support an

application to the Transport Innovation Fund (TIF), which requires demand to be income

segmented.

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8 Summary and Conclusions

Sheffield and Rotherham District SATURN Model 2008 8.2

8.1.9 A five user class model has also been created should Sheffield City Council require this

functionality. The model validates to the same level as the 6 user class model summarised in

this report, and will primarily be used to provide demand data for current or proposed

AIMSUN models within Sheffield District

8.1.10 The five user classes are;

Car – Employer’s Business;

Car – Commute;

Car – Other;

LGV; and

OGV.

8.2 Conclusions

8.2.1 It is considered that the Sheffield and Rotherham District SATURN model, SRHM3, has been

successfully developed and the models for all time periods are considered fit for purpose,

namely to appraise transport schemes and the effects of new developments within the

districts.

Page 81: Appendix B3 – Saturn Model Development Report

Appendices

Page 82: Appendix B3 – Saturn Model Development Report

Appendix A – Roadside Interview Programme

Table A.1 2005 Rotherham Inner/Outer Cordon

ID Location Date Type Sample

Size (%)

422 B6086 Grange Lane Wed 2 Nov 05 SG/PC 688 (71)

424 Meadowhall Road, Rotherham Tue 1 Nov 05 SG/PC 812 (55)

501 A629 New Wortley Road Tue 18 Oct 05 RIS 1235 (13)

502 Coronation Bridge, Rotherham Wed 19 Oct 05 RIS 1180 (24)

503 A6178 Sheffield Road Wed 19 Oct 05 RIS 1017 (17)

505 A631 Bawtry Road Thu 3 Nov 05 RIS 1121 (9)

506 A630 Doncaster Road Tue 18 Oct 05 RIS 1053 (10)

507 Barber's Avenue Thu 20 Oct 05 SG/PC 1253 (29)

508 Rawmarsh Hill Thu 20 Oct 05 RIS/PC 1047 (14)

511 B6086 Brook Hill Wed 2 Nov 05 RIS 774 (40)

512 Badsley Moor Lane Tue 1 Nov 05 SG/PC 1240 (68)

Page 83: Appendix B3 – Saturn Model Development Report

Table A.2 2006 Sheffield Outer Cordon & Screenlines

ID Location Date Type Sample

Size (%)

401 A6102 Manchester Road Wed 22 Mar 06 SG/PC 1303 (31)

403 A61 Penistone Road, Burncross Thu 23 Mar 06 PC 1507 (20)

404 Bracken Hill, Burncross Thu 23 Mar 06 SG/PC 1324 (47)

405 A6135 Chapeltown Rd, Chapeltown Mon 27 Mar 06 SG/PC 1049 (17)

408 Wincobank Avenue, High Wincobank Mon 27 Mar 06 SG/PC 1358 (46)

409 Shirecliffe Road Thu 30 Mar 06 SG 1212 (24)

410 A61 Penistone Road Thu 30 Mar 06 PC 1559 (13)

411 B6079 Middlewood Rd, Hillsborough Tue 18 Apr 06 RIS 935 (37)

412 B6077 Loxley Road, Malin Bridge Tue 18 Apr 06 SG/PC 1399 (33)

420 A6135 White Lane Tue 28 Mar 06 SG/PC 1292 (32)

421 Jumble Lane, Thorpe Common Tue 28 Mar 06 SG/PC 417 (73)

423 New Droppingwell Road Wed 29 Mar 06 SG/PC 1130 (54)

425 Blackburn Road Wed 29 Mar 06 RIS 1079 (21)

428 B0667 Worksop Road, Netherthorpe Thu 27 Apr 06 SG/PC 1277 (39)

429 A618 Mansfield Rd, Wales Common Fri 28 Apr 06 RIS 1314 (22)

430 B6058 Sheffield Road, Nether Green Tue 2 May 06 RIS 1290 (33)

431 B6053 Rotherham Rd, Windmill Hill Tue 2 May 06 RIS 1334 (20)

432 A6135 Sheffield Road Wed 3 May 06 SG/PC 1218 (34)

433 Ford Lane Wed 3 May 06 SG/PC 1078 (83)

435 B6057 Sheffield Road, Dronfield Mon 8 May 06 RIS 1330 (24)

436 A61 Dronfield By Pass Tue 9 May 06 RIS 1207 (12)

437 B6054 Greenhill Parkway Tue 9 May 06 RIS 1257 (28)

438 A621 Abbeydale Road Wed 10 May 06 RIS 1375 (19)

Page 84: Appendix B3 – Saturn Model Development Report

439 A625 Ecclesall Road, Whirlow Wed 10 May 06 SG/PC 1349 (32)

440 Ringinglow Road, Ringinglow Thu 11 May 06 SG/PC 1155 (58)

441 A57 Manchester Road Thu 11 May 06 SG/PC 1534 (60)

442 Carr Road, Deepcar Wed 22 Mar 06 SG/PC 902 (78)

443 B6088 Manchester Road Tue 21 Mar 06 SG/PC 1130 (35)

444 A616 Valley View Tue 21 Mar 06 RIS 1031 (17)

446 A629 Halifax Road Mon 20 Mar 06 RIS 1000 (23)

448 Tankersley Lane Mon 20 Mar 06 SG/PC 946 (60)

461 Europa Link Wed 19 Apr 06 RIS 1150 (30)

462 Handsworth Road Wed 19 Apr 06 RIS 1177 (16)

463 A6102 Prince of Wales Road Thu 20 Apr 06 RIS 1173 (11)

465 Harborough Avenue, Manor Park Thu 20 Apr 06 SG/PC 1282 (60)

466 A6135 City Road Mon 24 Apr 06 RIS 1274 (22)

467 East Bank Road Mon 24 Apr 06 SG/PC 1464 (45)

468 B6388 Gleadless Road Tue 25 Apr 06 SG/PC 1517 (37)

469 Blackstock Road Tue 25 Apr 06 SG/PC 1484 (48)

470 Hemsworth Road Wed 26 Apr 06 SG/PC 1571 (42)

471 A61 Meadowhead, Greenhill Mon 8 May 06 RIS 1274 (15)

472 Bocking Lane, Greenhill Wed 26 Apr 06 PC 2084 (25)

Page 85: Appendix B3 – Saturn Model Development Report

Table A.3 2007 Sheffield and Rotherham Motorway Corridor

ID Location Date Type Sample

Size (%)

609 A6109 Meadowhall Road Tue 27 Mar 07 PC 1122 (9)

616 A630 Sheffield Parkway Tue 27 Mar 07 PC 1043 (7)

612 A6178 Sheffield Road Wed 28 Mar 07 PC 892 (13)

614 A6102 Shepcote Lane Wed 28 Mar 07 PC 1127 (5)

Table A.4 2007 Surveys – Rotherham Town Centre

ID Location Date Type Sample

Size (%)

621 B6089 Greasbrough Road Tue 6 Nov 07 RIS 1155 (11)

622 A633 Rotherham Rd / Rawmarsh Rd Tue 6 Nov 07 PC 847 (12)

623 A630 Fitzwilliam Road Wed 7 Nov 07 RIS 1198 (19)

624 A630 Doncaster Road Wed 7 Nov 07 PC 1116 (25)

625 A6021 Broom Road Thu 8 Nov 07 RIS 1167 (18)

626 A618 Moorgate Road Thu 8 Nov 07 PC 1058 (24)

627 A630 Centenary Way Mon 12 Nov 07 RIS 1364 (12)

Table A.5 2007 Surveys – Sheffield/Meadowhall Screenline

ID Location Date Type Sample

Size (%)

628 B6082 Ecclesfield Road Mon 12 Nov 07 PC 795 (16)

629 A6102 Upwell Street Wed 21 Nov 07 PC 880 (11)

630 A6135 Barnsley Road Wed 21 Nov 07 PC 869 (16)

Page 86: Appendix B3 – Saturn Model Development Report

Table A.6 2007 Surveys – Sheffield City Centre

ID Location Date Type Sample

Size (%)

631 B6074 Mowbray Street Mon 10 Dec 07 PC 189 (5)

632 C426 Pitsmoor Road Mon 10 Dec 07 PC 160 (6)

633 A6135 Spital Hill Tue 11 Dec 07 PC 111 (4)

634 A6109 Savile Street Tue 11 Dec 07 PC 496 (7)

635 B6073 Furnival Road Wed 12 Dec 07 PC 295 (9)

636 A57 Sheffield Parkway Wed 12 Dec 07 PC 1091 (5)

637 B6072 Broad Street Tue 27 Nov 07 PC 334 (8)

639 B6071 Shrewsbury Road Tue 27 Nov 07 PC 337 (12)

640 B6070 Granville Road Wed 28 Nov 07 PC 433 (10)

642 A61 Queens Road Wed 28 Nov 07 PC 285 (4)

643 UNC Shoreham Street Tue 13 Nov 07 PC 528 (16)

644 A621 Bramall Lane Thu 13 Nov 08 PC 909 (12)

645 B6388 London Road Mon 3 Dec 07 PC 375 (4)

647 A625 Ecclesall Road Mon 3 Dec 07 PC 1449 (12)

648 B6069 Glossop Road Tue 4 Dec 07 PC 332 (4)

649 A57 Western Bank Tue 4 Dec 07 PC 568 (8)

650 C431 Bolsover Street Thu 22 Nov 07 PC 592 (13)

651 UNC Meadow Street Thu 29 Nov 07 PC 219 (13)

652A A61 Penistone Road (Main Road) Thu 13 Dec 07 PC 359 (2)

652B A61 Penistone Road (Subsidiary Rd) Thu 13 Dec 07 PC 72 (11)

653 A61 Netherthorpe Road Thu 29 Nov 07 PC 751 (6)

654 A57 Broad Lane Wed 5 Dec 07 PC 952 (10)

656 UNC Leopold Street Mon 26 Nov 07 PC 159 (13)

Page 87: Appendix B3 – Saturn Model Development Report

657 A621 Arundel Gate Thu 22 Nov 07 PC 307 (4)

658 A61 Sheaf Street Wed 5 Dec 07 PC 339 (3)

659 UNC Upper Allen Street Mon 26 Nov 07 PC 187 (13)

Table A.7 2007 Surveys – Motorway Surveys

ID Location Date Type Sample

Size (%)

713 A618 Pleasley Road Tue 20 Nov 07 PC 1350 (25)

714 A630 Rotherway Mon 19 Nov 07 PC 1449 (12)

715 A631 Bawtry Road Mon 19 Nov 07 PC 696 (11)

716 A6178 Sheffield Road Thu 15 Nov 07 PC 562 (9)

717 A6109 Meadow Bank Road Thu 15 Nov 07 PC 688 (10)

718 A629 Cowley Hill Wed 14 Nov 07 PC 1058 (17)

719 A629 Upper Wortley Road Wed 14 Nov 07 RIS 1372 (21)

720 A616 Roundabout leading to M1 J35A Thu 6 Dec 07 PC 590 (7)

721 A61 Westwood New Road Thu 6 Dec 07 PC 879 (9)

733 A57 Aston Way Tue 20 Nov 07 RIS 774 (10)

Table A.8 2008 RSI Surveys – Waverley Area

ID Location Date Type Sample

Size (%)

801 Treeton Road Tuesday 8th July 2008 PC 1341 (38)

802 Retford Road Thu 6 Dec 07 PC 1452 (23)

803 Chesterfield Road Tue 20 Nov 07 PC 1747 (22)

Page 88: Appendix B3 – Saturn Model Development Report

1.1 Roadside interview survey forms are shown overleaf. The 2007 form is similar to the 2005

and 2006 forms, except there is an extra set of questions regarding (if applicable) asking

respondents which car parks they used and, if a public car park, what charge they paid.

Page 89: Appendix B3 – Saturn Model Development Report

Figure A1 Example Roadside Interview Survey form from MVA Surveys in 2002, 2005 and 2006

Page 90: Appendix B3 – Saturn Model Development Report

Figure A2 Example Roadside Interview Survey form from MVA Surveys in 2007

Page 91: Appendix B3 – Saturn Model Development Report

Appendix B – Roadside Interview Survey Variables

MVA Roadside Interview Surveys – Origin / Destination Purposes

1 Home

2 Usual Workplace

3 Employer’s Business

4 Education

5 Shopping

6 Personal Business

7 Visit Friends

8 Recreation/Leisure

9 Other

Common Vehicle Types

1 Car

2 LGV

3 OGV

MVA Surveys Vehicle Types

1 Car

2 Taxi

3 LGV

4 OGV 1

5 OGV 2

6 Bus/Coach

7 Minibus

8 Motorcycle/Moped

9 Pedal Cycle

10 Other

Notes

OGV 1 is defined as a rigid goods vehicle greater than 3.5 tonnes with 2 or 3 axles.

OGV 2 is defined as a rigid or articulated vehicles with 4 or more axles.

Page 92: Appendix B3 – Saturn Model Development Report

Table B1 Value Labels for All Surveys

Description MVA 2006 MVA 2007

Original Site Number Site Site

New Site Number

Date Date Date

Half hour time period Time Time

Serial_No Serial_No

Interview_No Interview_No

Original Vehicle Type Type Type

VehOther VehOther

Occupancy Occupancy Occupancy

Origin

Origin Postcode Sector

Origin Postcode Opostcode Opostcode

Origin Purpose Opurpose Opurpose

Alternative Origin Purpose Oother Oother

Origin X Coordinate

Origin Y Coordinate

Destination

Destination Postcode Sector

Destination Postcode Dpostcode Dpostcode

Destination Purpose Dpurpose Dpurpose

Alternative Destination Purpose Dother Dother

Destination X Coordinate

Destination Y Coordinate

Parking Location

Origin Check Results_O Results_O

Destination Check Results_D Results_D

Illogical Flag Illogical Illogical

Page 93: Appendix B3 – Saturn Model Development Report

Appendix C – Bandwidth Plots

Page 94: Appendix B3 – Saturn Model Development Report

Figure C1 Morning Peak Model Bandwidth Plot

Page 95: Appendix B3 – Saturn Model Development Report

Figure C2 Inter-Peak Model Bandwidth Plot

Page 96: Appendix B3 – Saturn Model Development Report

Figure C3 Evening Peak Model Bandwidth Plot

Page 97: Appendix B3 – Saturn Model Development Report

Appendix D - Count Comparisons

1 Key

1.1 Table D1 shows the count comparison (total vehicles) for the individual links along each of the key routes, namely BRT North, BRT South,

Penistone Rd, and Eccdesall Rd, and across both the Sheffield City Cordon and the Rotherham Town centre Cordon

1.2 The data is presented for Morning Peak, Inter-peak and Evening Peak

1.3 Figure D1 to D6 show scatter-plots of the observed counts against modelled flows, again focussed on total vehicles.

1.4 They are presented for all three times periods, with one plot for each time period showing the correlation with respect to the DMRB

guidelines, and another plot showing the correlation with respect to the GEH guidelines.

Page 98: Appendix B3 – Saturn Model Development Report

Table D 1 Count Comparison for Key Count Sets

Morning Peak Inter-peak Evening Peak Obs Mod GEH DMRB Obs Mod GEH DMRB Obs Mod GEH DMRB

Penistone Rd - Outbound 853

571

10.6 LOW

889

817

2.5 OK

1,365

1,169

5.5 OK

Penistone Rd - Outbound 569

523

2.0 OK

657

674

0.6 OK

1,129

1,093

1.1 OK

Penistone Rd - Outbound 1,449

1,246

5.5 OK

1,512

1,313

5.3 OK

2,022

1,773

5.7 OK

Penistone Rd - Outbound 901

944

1.4 OK

1,039

1,098

1.8 OK

1,372

1,545

4.5 OK

Penistone Rd - Outbound 996

1,128

4.1 OK

1,182

1,212

0.9 OK

1,570

1,764

4.8 OK

Penistone Rd - Outbound 1,131

1,159

0.8 OK

1,097

1,115

0.5 OK

1,334

1,515

4.8 OK

Penistone Rd - Outbound 1,208

1,389

5.0 HIGH

1,279

1,348

1.9 OK

1,526

1,753

5.6 OK

Penistone Rd - Outbound 1,433

1,452

0.5 OK

1,432

1,449

0.4 OK

1,894

1,853

0.9 OK

Penistone Rd - Outbound 1,707

1,686

0.5 OK

1,518

1,528

0.3 OK

1,996

1,864

3.0 OK

Penistone Rd - Outbound 1,683

1,735

1.3 OK

1,571

1,600

0.7 OK

2,033

1,883

3.4 OK

Penistone Rd - Outbound 1,601

1,636

0.9 OK

1,809

1,827

0.4 OK

2,162

2,039

2.7 OK

Penistone Rd - Outbound 1,431

1,462

0.8 OK

1,466

1,559

2.4 OK

1,929

1,983

1.2 OK

Penistone Rd - Outbound 1,535

1,547

0.3 OK

1,665

1,678

0.3 OK

2,213

2,172

0.9 OK

Penistone Rd - Outbound 1,726

1,780

1.3 OK

1,887

1,896

0.2 OK

2,329

2,325

0.1 OK

Penistone Rd - Outbound 1,762

1,714

1.1 OK

1,749

1,790

1.0 OK

2,194

2,149

1.0 OK

Penistone Rd - Outbound 1,554

1,529

0.6 OK

1,349

1,422

2.0 OK

1,544

1,527

0.4 OK

Penistone Rd - Outbound 1,527

1,529

0.1 OK

1,469

1,422

1.2 OK

1,664

1,527

3.4 OK

Penistone Rd - Outbound 963

937

0.8 OK

973

974

0.0 OK

842

814

1.0 OK

Penistone Rd - Outbound 1,556

1,556

0.0 OK

1,325

1,332

0.2 OK

1,455

1,469

0.4 OK

Penistone Rd - Inbound 1,587

1,602

0.4 OK

1,239

1,278

1.1 OK

1,602

1,650

1.2 OK

Penistone Rd - Inbound 868

938

2.3 OK

892

877

0.5 OK

975

978

0.1 OK

Penistone Rd - Inbound 1,458

1,619

4.1 OK

1,347

1,266

2.2 OK

1,558

1,530

0.7 OK

Page 99: Appendix B3 – Saturn Model Development Report

Penistone Rd - Inbound 1,665

1,619

1.1 OK

1,283

1,266

0.5 OK

1,503

1,530

0.7 OK

Penistone Rd - Inbound 2,290

2,249

0.8 OK

1,659

1,642

0.4 OK

1,772

1,746

0.6 OK

Penistone Rd - Inbound 2,252

2,348

2.0 OK

1,596

1,670

1.8 OK

1,820

1,892

1.7 OK

Penistone Rd - Inbound 1,724

1,848

2.9 OK

1,087

1,143

1.7 OK

1,163

1,173

0.3 OK

Penistone Rd - Inbound 1,846

1,898

1.2 OK

1,230

1,214

0.5 OK

1,367

1,274

2.6 OK

Penistone Rd - Inbound 2,215

2,387

3.6 OK

1,650

1,585

1.6 OK

1,492

1,517

0.7 OK

Penistone Rd - Inbound 2,011

2,112

2.2 OK

1,485

1,413

1.9 OK

1,359

1,387

0.7 OK

Penistone Rd - Inbound 2,037

1,998

0.9 OK

1,362

1,351

0.3 OK

1,551

1,401

3.9 OK

Penistone Rd - Inbound 1,948

2,158

4.6 OK

1,306

1,420

3.1 OK

1,482

1,502

0.5 OK

Penistone Rd - Inbound 1,911

2,104

4.3 OK

1,358

1,383

0.7 OK

1,498

1,592

2.4 OK

Penistone Rd - Inbound 1,628

1,675

1.2 OK

1,131

1,123

0.2 OK

1,257

1,319

1.7 OK

Penistone Rd - Inbound 1,411

1,489

2.0 OK

988

1,001

0.4 OK

1,066

1,109

1.3 OK

Penistone Rd - Inbound 2,123

2,096

0.6 OK

1,281

1,310

0.8 OK

1,438

1,482

1.2 OK

Penistone Rd - Inbound 2,307

1,960

7.5 LOW

1,458

1,236

6.0 LOW

1,628

1,542

2.1 OK

Penistone Rd - Inbound 1,383

1,486

2.7 OK

990

1,024

1.1 OK

1,192

1,288

2.7 OK

Ecclesall Rd - Outbound 990

979

0.3 OK

891

889

0.1 OK

1,044

1,043

0.0 OK

Ecclesall Rd - Outbound 871

979

3.6 OK

786

889

3.6 OK

883

1,043

5.2 HIGH

Ecclesall Rd - Outbound 638

587

2.0 OK

589

510

3.4 OK

646

646

0.0 OK

Ecclesall Rd - Outbound 580

673

3.7 OK

580

552

1.2 OK

722

748

0.9 OK

Ecclesall Rd - Outbound 477

456

1.0 OK

560

429

5.9 LOW

615

622

0.3 OK

Ecclesall Rd - Outbound 810

891

2.8 OK

887

914

0.9 OK

1,180

1,202

0.6 OK

Ecclesall Rd - Outbound 676

751

2.8 OK

727

716

0.4 OK

946

1,003

1.8 OK

Ecclesall Rd - Outbound 733

679

2.0 OK

666

636

1.2 OK

832

876

1.5 OK

Ecclesall Rd - Outbound 996

948

1.5 OK

1,095

1,059

1.1 OK

1,654

1,283

9.7 LOW

Ecclesall Rd - Outbound OK OK OK

Page 100: Appendix B3 – Saturn Model Development Report

685 586 3.9 671 591 3.2 1,015 943 2.3

Ecclesall Rd - Outbound 563

530

1.4 OK

565

553

0.5 OK

890

894

0.1 OK

Ecclesall Rd - Inbound 589

562

1.1 OK

564

529

1.5 OK

628

624

0.1 OK

Ecclesall Rd - Inbound 730

698

1.2 OK

695

654

1.6 OK

734

734

0.0 OK

Ecclesall Rd - Inbound 1,010

899

3.6 OK

1,043

1,008

1.1 OK

951

978

0.9 OK

Ecclesall Rd - Inbound 452

413

1.9 OK

667

656

0.4 OK

783

732

1.8 OK

Ecclesall Rd - Inbound 610

545

2.7 OK

742

747

0.2 OK

745

813

2.4 OK

Ecclesall Rd - Inbound 761

962

6.8 HIGH

850

1,056

6.7 HIGH

824

894

2.4 OK

Ecclesall Rd - Inbound 633

563

2.8 OK

482

370

5.4 LOW

351

411

3.1 OK

Ecclesall Rd - Inbound 811

851

1.4 OK

669

668

0.1 OK

582

622

1.6 OK

Ecclesall Rd - Inbound 661

708

1.8 OK

599

590

0.4 OK

515

542

1.2 OK

Ecclesall Rd - Inbound 1,046

1,171

3.8 OK

874

1,006

4.3 HIGH

795

897

3.5 OK

Ecclesall Rd - Inbound 1,197

1,172

0.7 OK

1,016

1,006

0.3 OK

916

898

0.6 OK

Ecclesall Rd - Inbound 3,127

3,048

1.4 OK

2,432

2,425

0.1 OK

2,281

2,131

3.2 OK

BRT North - Outbound 824

770

1.9 OK

559

531

1.2 OK

657

282

17.3 LOW

BRT North - Outbound 1,176

1,159

0.5 OK

910

884

0.9 OK

1,234

866

11.3 LOW

BRT North - Outbound 690

637

2.0 OK

505

475

1.4 OK

478

440

1.8 OK

BRT North - Outbound 703

760

2.1 OK

528

533

0.2 OK

561

620

2.4 OK

BRT North - Outbound 319

402

4.4 OK

272

300

1.7 OK

220

336

7.0 HIGH

BRT North - Outbound 294

315

1.2 OK

358

353

0.2 OK

392

353

2.0 OK

BRT North - Outbound 514

549

1.5 OK

527

496

1.4 OK

619

613

0.2 OK

BRT North - Outbound 778

749

1.0 OK

682

674

0.3 OK

823

808

0.5 OK

BRT North - Outbound 931

937

0.2 OK

777

838

2.1 OK

928

934

0.2 OK

BRT North - Outbound 488

700

8.7 HIGH

570

725

6.1 HIGH

624

660

1.4 OK

BRT North - Outbound 1,223

1,077

4.3 OK

1,379

973

11.9 LOW

2,003

1,722

6.5 OK

Page 101: Appendix B3 – Saturn Model Development Report

BRT North - Outbound 780

730

1.8 OK

1,250

1,209

1.2 OK

1,978

1,881

2.2 OK

BRT North - Outbound 615

623

0.4 OK

490

543

2.3 OK

618

678

2.4 OK

BRT North - Outbound 540

568

1.2 OK

565

610

1.8 OK

1,196

1,181

0.4 OK

BRT North - Outbound 799

793

0.2 OK

528

516

0.5 OK

822

838

0.5 OK

BRT North - Outbound 181

138

3.4 OK

176

155

1.7 OK

218

153

4.8 OK

BRT North - Inbound 417

163

14.9 LOW

381

172

12.6 LOW

471

150

18.3 LOW

BRT North - Inbound 555

543

0.5 OK

471

472

0.0 OK

568

543

1.0 OK

BRT North - Inbound 1,097

1,105

0.2 OK

486

518

1.4 OK

469

470

0.0 OK

BRT North - Inbound 607

648

1.6 OK

431

478

2.2 OK

560

496

2.8 OK

BRT North - Inbound 1,924

1,928

0.1 OK

1,279

1,246

0.9 OK

1,323

1,271

1.5 OK

BRT North - Inbound 1,853

1,582

6.5 OK

1,336

1,202

3.7 OK

1,492

1,375

3.1 OK

BRT North - Inbound 778

757

0.7 OK

622

667

1.8 OK

693

701

0.3 OK

BRT North - Inbound 993

969

0.8 OK

834

886

1.8 OK

1,074

1,110

1.1 OK

BRT North - Inbound 775

768

0.3 OK

696

805

4.0 HIGH

791

822

1.1 OK

BRT North - Inbound 427

473

2.2 OK

348

385

2.0 OK

223

341

7.0 HIGH

BRT North - Inbound 478

507

1.3 OK

367

390

1.2 OK

242

281

2.4 OK

BRT North - Inbound 385

413

1.4 OK

319

337

1.0 OK

384

403

1.0 OK

BRT North - Inbound 628

679

2.0 OK

483

502

0.8 OK

596

611

0.6 OK

BRT North - Inbound 707

514

7.8 LOW

583

627

1.8 OK

722

727

0.2 OK

BRT South - Outbound 1,773

1,804

0.7 OK

1,448

1,503

1.4 OK

2,491

2,496

0.1 OK

BRT South - Outbound 1,519

1,489

0.8 OK

1,156

1,091

1.9 OK

2,109

1,945

3.6 OK

BRT South - Outbound 1,539

1,469

1.8 OK

1,172

1,123

1.4 OK

2,242

1,997

5.3 OK

BRT South - Outbound 1,108

1,442

9.3 HIGH

1,076

1,090

0.4 OK

1,778

1,546

5.7 OK

BRT South - Outbound 2,213

2,512

6.2 OK

1,899

2,078

4.0 OK

3,195

3,085

2.0 OK

BRT South - Outbound OK OK OK

Page 102: Appendix B3 – Saturn Model Development Report

1,193 1,162 0.9 865 832 1.2 1,101 1,199 2.9

BRT South - Outbound 985

965

0.6 OK

893

860

1.1 OK

1,372

1,357

0.4 OK

BRT South - Outbound 873

877

0.2 OK

428

448

1.0 OK

441

442

0.0 OK

BRT South - Outbound 470

484

0.6 OK

353

376

1.2 OK

425

372

2.6 OK

BRT South - Outbound 446

455

0.4 OK

429

450

1.0 OK

477

440

1.7 OK

BRT South - Inbound 532

544

0.5 OK

424

438

0.7 OK

709

715

0.3 OK

BRT South - Inbound 514

523

0.4 OK

385

393

0.4 OK

596

600

0.2 OK

BRT South - Inbound 484

488

0.2 OK

492

496

0.2 OK

834

859

0.9 OK

BRT South - Inbound 1,203

1,189

0.4 OK

862

875

0.4 OK

996

1,018

0.7 OK

BRT South - Inbound 1,174

1,083

2.7 OK

934

960

0.8 OK

1,087

1,094

0.2 OK

BRT South - Inbound 3,047

2,920

2.3 OK

1,634

1,693

1.4 OK

1,955

1,985

0.7 OK

BRT South - Inbound 1,706

1,240

12.1 LOW

1,086

937

4.7 OK

1,020

952

2.2 OK

BRT South - Inbound 2,120

1,915

4.6 OK

1,523

1,462

1.6 OK

1,962

1,810

3.5 OK

BRT South - Inbound 2,323

2,231

1.9 OK

1,857

1,875

0.4 OK

2,379

2,361

0.4 OK

Rotherham City Cordon - Inbound 615

623

0.4 OK

490

543

2.3 OK

618

678

2.4 OK

Rotherham City Cordon - Inbound 687

702

0.6 OK

528

532

0.2 OK

604

573

1.3 OK

Rotherham City Cordon - Inbound 1,047

1,045

0.1 OK

777

788

0.4 OK

864

838

0.9 OK

Rotherham City Cordon - Inbound 1,144

1,093

1.5 OK

740

706

1.3 OK

907

830

2.6 OK

Rotherham City Cordon - Inbound 574

781

8.0 HIGH

607

773

6.3 HIGH

584

812

8.6 HIGH

Rotherham City Cordon - Inbound 774

722

1.9 OK

547

572

1.0 OK

538

528

0.4 OK

Rotherham City Cordon - Inbound 560

570

0.4 OK

320

314

0.4 OK

295

307

0.7 OK

Rotherham City Cordon - Inbound 261

258

0.2 OK

196

186

0.7 OK

244

226

1.1 OK

Rotherham City Cordon - Inbound 983

975

0.2 OK

479

498

0.9 OK

447

460

0.6 OK

Rotherham City Cordon - Inbound 446

455

0.4 OK

429

450

1.0 OK

477

440

1.7 OK

Rotherham City Cordon - Inbound 89

103

1.5 OK

74

123

4.9 OK

82

214

10.9 HIGH

Page 103: Appendix B3 – Saturn Model Development Report

Rotherham City Cordon - Outbound 607

648

1.6 OK

431

478

2.2 OK

560

496

2.8 OK

Rotherham City Cordon - Outbound 506

523

0.8 OK

527

560

1.4 OK

772

786

0.5 OK

Rotherham City Cordon - Outbound 725

714

0.4 OK

847

824

0.8 OK

1,128

1,163

1.0 OK

Rotherham City Cordon - Outbound 707

722

0.6 OK

823

829

0.2 OK

1,165

1,065

3.0 OK

Rotherham City Cordon - Outbound 461

473

0.5 OK

622

608

0.6 OK

691

685

0.2 OK

Rotherham City Cordon - Outbound 482

586

4.5 HIGH

609

635

1.1 OK

790

712

2.9 OK

Rotherham City Cordon - Outbound 267

293

1.6 OK

412

423

0.6 OK

665

655

0.4 OK

Rotherham City Cordon - Outbound 133

134

0.1 OK

189

174

1.1 OK

270

307

2.2 OK

Rotherham City Cordon - Outbound 414

405

0.4 OK

484

502

0.8 OK

989

1,015

0.8 OK

Rotherham City Cordon - Outbound 532

544

0.5 OK

424

438

0.7 OK

709

715

0.3 OK

Rotherham City Cordon - Outbound 96

29

8.5 OK

98

15

11.0 OK

133

58

7.6 OK

Sheffield City Cordon - Inbound 3,047

2,920

2.3 OK

1,634

1,693

1.4 OK

1,955

1,985

0.7 OK

Sheffield City Cordon - Inbound 370

376

0.3 OK

253

234

1.3 OK

366

342

1.2 OK

Sheffield City Cordon - Inbound 215

264

3.2 OK

208

284

4.8 OK

384

477

4.5 OK

Sheffield City Cordon - Inbound 722

677

1.7 OK

229

236

0.4 OK

217

231

0.9 OK

Sheffield City Cordon - Inbound 175

284

7.2 HIGH

73

230

12.8 HIGH

67

281

16.2 HIGH

Sheffield City Cordon - Inbound 594

575

0.8 OK

152

144

0.7 OK

133

110

2.1 OK

Sheffield City Cordon - Inbound 1,036

1,151

3.5 OK

691

668

0.9 OK

685

690

0.2 OK

Sheffield City Cordon - Inbound 713

651

2.4 OK

543

487

2.5 OK

621

555

2.7 OK

Sheffield City Cordon - Inbound 1,046

1,171

3.8 OK

874

1,006

4.3 HIGH

795

897

3.5 OK

Sheffield City Cordon - Inbound 352

314

2.1 OK

269

319

2.9 OK

241

270

1.8 OK

Sheffield City Cordon - Inbound 972

954

0.6 OK

909

752

5.5 LOW

808

696

4.1 OK

Sheffield City Cordon - Inbound 697

673

0.9 OK

242

249

0.5 OK

254

254

0.0 OK

Sheffield City Cordon - Inbound 307

418

5.9 HIGH

125

106

1.7 OK

145

206

4.6 OK

Sheffield City Cordon - Inbound LOW LOW OK

Page 104: Appendix B3 – Saturn Model Development Report

2,307 1,960 7.5 1,458 1,236 6.0 1,628 1,542 2.1

Sheffield City Cordon - Inbound 764

821

2.0 OK

512

553

1.8 OK

746

637

4.1 OK

Sheffield City Cordon - Inbound 433

431

0.1 OK

196

188

0.6 OK

271

326

3.2 OK

Sheffield City Cordon - Inbound 317

180

8.7 LOW

278

205

4.7 OK

312

325

0.7 OK

Sheffield City Cordon - Outbound 2,213

2,512

6.2 OK

1,899

2,078

4.0 OK

3,195

3,085

2.0 OK

Sheffield City Cordon - Outbound 125

127

0.1 OK

138

152

1.2 OK

160

142

1.5 OK

Sheffield City Cordon - Outbound 275

330

3.2 OK

201

231

2.0 OK

224

378

8.9 HIGH

Sheffield City Cordon - Outbound 173

184

0.9 OK

203

221

1.3 OK

239

300

3.7 OK

Sheffield City Cordon - Outbound 221

144

5.7 OK

257

249

0.5 OK

550

555

0.2 OK

Sheffield City Cordon - Outbound 48

117

7.6 OK

33

51

2.9 OK

26

32

1.2 OK

Sheffield City Cordon - Outbound 119

128

0.8 OK

194

225

2.1 OK

301

354

2.9 OK

Sheffield City Cordon - Outbound 499

515

0.7 OK

792

852

2.1 OK

1,115

1,046

2.1 OK

Sheffield City Cordon - Outbound 430

445

0.7 OK

460

387

3.6 OK

736

693

1.6 OK

Sheffield City Cordon - Outbound 871

979

3.6 OK

786

889

3.6 OK

883

1,043

5.2 HIGH

Sheffield City Cordon - Outbound 353

207

8.7 LOW

341

344

0.2 OK

320

343

1.2 OK

Sheffield City Cordon - Outbound 1,003

1,037

1.1 OK

942

797

4.9 LOW

1,258

1,258

0.0 OK

Sheffield City Cordon - Outbound 305

264

2.4 OK

365

326

2.1 OK

963

884

2.6 OK

Sheffield City Cordon - Outbound 141

141

0.0 OK

195

224

2.0 OK

346

465

5.9 HIGH

Sheffield City Cordon - Outbound 1,449

1,246

5.5 OK

1,512

1,313

5.3 OK

2,022

1,773

5.7 OK

Sheffield City Cordon - Outbound 268

313

2.7 OK

204

186

1.3 OK

222

197

1.7 OK

Sheffield City Cordon - Outbound 213

180

2.4 OK

207

192

1.0 OK

373

350

1.2 OK

Sheffield City Cordon - Outbound 217

206

0.7 OK

238

197

2.7 OK

178

228

3.5 OK

Page 105: Appendix B3 – Saturn Model Development Report

Figure D.1 Morning Peak Count Comparison – Total Vehicles

y = 0.9804xR2 = 0.9814

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow DMRB Criteria High Limit DMRB Criteria Low Limit Actual Flow = Count Linear (Model Flow) Linear (Model Flow)

Page 106: Appendix B3 – Saturn Model Development Report

Figure D.2 Inter-peak GEH Count Comparison – Total Vehicles

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow DMRB Criteria High Limit DMRB Criteria Low Limit Actual Flow = Count Linear (Model Flow)

Page 107: Appendix B3 – Saturn Model Development Report

Figure D.3 Evening Peak GEH Count Comparison – Total Vehicles

y = 0.9759xR2 = 0.9817

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow DMRB Criteria High Limit DMRB Criteria Low Limit Actual Flow = Count Linear (Model Flow)

Page 108: Appendix B3 – Saturn Model Development Report

Figure D.4 Morning Peak GEH Count Comparison – Total Vehicles

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow GEH Value = 5 GEH Value = - 5 GEH Value = 0

Page 109: Appendix B3 – Saturn Model Development Report

Figure D.5 Inter Peak GEH Count Comparison – Total Vehicles

y = 0.9829xR2 = 0.9855

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow GEH Value = 5 GEH Value = - 5 GEH Value = 0 Linear (Model Flow)

Page 110: Appendix B3 – Saturn Model Development Report

Figure D.6 Evening Peak GEH Count Comparison – Total Vehicles

0

1000

2000

3000

4000

5000

6000

7000

0 1000 2000 3000 4000 5000 6000 7000

Observed

Mod

el F

low

Model Flow GEH Value = 5 GEH Value = - 5 GEH Value = 0

Page 111: Appendix B3 – Saturn Model Development Report

Appendix E – Journey Time Comparisons

Table E 1 Morning Peak Journey Time – By Route Segment

By Route Section

Route Mod Obs Diff %Diff DMRB %

Slow

% Ok % Fast

Abbeydale Rd - Inbound 832 944 -112 -12% OK 27% 18% 55%

Abbeydale Rd - Outbound 694 621 73 12% OK 36% 27% 36%

Ecclesall Rd - Inbound 570 681 -111 -16% FAST 29% 14% 57%

Ecclesall Rd - Outbound 386 369 17 5% OK 43% 43% 14%

Crookes Rd / A57 Western Bank -

Inbound 686 621 65 10% OK 33% 22% 44%

Crookes Rd / A57 Western Bank -

Outbound 463 409 54 13% OK 38% 13% 50%

A57 Fulwood Rd / Glossop Rd -

Inbound 662 604 58 10% OK 44% 11% 44%

A57 Fulwood Rd / Glossop Rd -

Outbound 482 423 59 14% OK 56% 0% 44%

Chesterfield Rd / London Rd -

Inbound 1005 1200 -195 -16% FAST 7% 43% 50%

Chesterfield Rd / London Rd -

Outbound 804 736 68 9% OK 36% 43% 21%

Rotherham to Sheffield via

Meadowhall 1046 1016 30 3% OK 36% 5% 59%

Sheffield to Rotherham via

Meadowhall 1043 919 124 13% OK 35% 25% 40%

Rotherham to Sheffield via Lower

Don Valley 1609 1475 134 9% OK 46% 12% 42%

Sheffield to Rotherham via Lower

Don Valley 1610 1400 210 15% OK 38% 24% 38%

Middlewood Rd / Penistone Rd -

Inbound 795 853 -58 -7% OK 22% 17% 61%

Middlewood Rd / Penistone Rd -

Outbound 674 500 174 35% SLOW 44% 19% 38%

Chapeltown to Sheffield 1316 1333 -17 -1% OK 31% 23% 46%

Sheffield to Chapeltown 1064 969 95 10% OK 47% 7% 47%

Crystal Peaks / Manor Top to

Sheffield 1064 982 82 8% OK 36% 14% 50%

Sheffield to Manor Top / Crystal

Peaks 833 737 96 13% OK 33% 8% 58%

Inner Ring Rd - Clockwise 1042 980 62 6% OK 44% 16% 40%

Inner Ring Rd - Anticlockwise 983 1011 -28 -3% OK 43% 14% 43%

Outer Ring Rd - A6102 - Clockwise 1784 1673 111 7% OK 38% 25% 38%

Outer Ring Rd - A6102 - Anti-

Clockwise 1822 1944 -122 -6% OK 38% 25% 38%

Sheffield Parkway - Inbound 677 907 -230 -25% FAST 50% 25% 25%

Sheffield Parkway - Outbound 612 562 50 9% OK 13% 38% 50%

A57 Mosborough Parkway /

Sheffield Parkway - Inbound 836 1001 -165 -16% FAST 44% 22% 33%

A57 Mosborough Parkway / 759 684 75 11% OK 11% 22% 67%

Page 112: Appendix B3 – Saturn Model Development Report

Sheffield Parkway - Outbound

Walkley to Sheffield 668 625 43 7% OK 80% 0% 20%

Sheffield to Walkley 529 403 126 31% SLOW 50% 0% 50%

Penistone Rd - Inbound 1198 1265 -67 -5% OK 46% 8% 46%

Penistone Rd - Outbound 859 844 15 2% OK 41% 23% 36%

Overall 29407 28691 716 30% 25% 45%

Table E 2 Inter Peak Journey Time – By Route Segment

By Route Section

Route Mod Obs Diff %Diff DMRB %

Slow

% Ok %

Fast

Abbeydale Rd - Inbound 781 1042 -261 -25% FAST 27% 36% 36%

Abbeydale Rd - Outbound 661 941 -280 -30% FAST 55% 27% 18%

Ecclesall Rd - Inbound 549 659 -110 -17% FAST 29% 43% 29%

Ecclesall Rd - Outbound 556 816 -260 -32% FAST 57% 0% 43%

Crookes Rd / A57 Western

Bank - Inbound 529 623 -94 -15% FAST 56% 11% 33%

Crookes Rd / A57 Western

Bank - Outbound 442 497 -55 -11% OK 63% 13% 25%

A57 Fulwood Rd / Glossop Rd

- Inbound 539 684 -145 -21% FAST 56% 0% 44%

A57 Fulwood Rd / Glossop Rd

- Outbound 477 563 -86 -15% FAST 44% 22% 33%

Chesterfield Rd / London Rd -

Inbound 909 1293 -384 -30% FAST 57% 14% 29%

Chesterfield Rd / London Rd -

Outbound 737 1267 -530 -42% FAST 43% 36% 21%

Rotherham to Sheffield via

Meadowhall 981 898 83 9% OK 32% 18% 50%

Sheffield to Rotherham via

Meadowhall 862 870 -8 -1% OK 25% 15% 60%

Rotherham to Sheffield via

Lower Don Valley 1582 1661 -79 -5% OK 38% 19% 42%

Sheffield to Rotherham via

Lower Don Valley 1604 1508 96 6% OK 38% 21% 41%

Middlewood Rd / Penistone Rd

- Inbound 757 647 110 17% SLOW 17% 28% 56%

Middlewood Rd / Penistone Rd

- Outbound 648 723 -75 -10% OK 56% 13% 31%

Chapeltown to Sheffield 1201 1836 -635 -35% FAST 31% 38% 31%

Sheffield to Chapeltown 1057 1143 -86 -8% OK 33% 40% 27%

Crystal Peaks / Manor Top to

Sheffield 920 955 -35 -4% OK 50% 7% 43%

Sheffield to Manor Top /

Crystal Peaks 820 802 18 2% OK 33% 33% 33%

Inner Ring Rd - Clockwise 868 730 138 19% SLOW 24% 24% 52%

Inner Ring Rd - Anticlockwise 783 852 -69 -8% OK 38% 33% 29%

Outer Ring Rd - A6102 -

Clockwise 1692 2043 -351 -17% FAST 42% 17% 42%

Outer Ring Rd - A6102 - Anti-

Clockwise 1752 1905 -153 -8% OK 33% 33% 33%

Page 113: Appendix B3 – Saturn Model Development Report

Sheffield Parkway - Inbound 512 692 -180 -26% FAST 63% 25% 13%

Sheffield Parkway - Outbound 561 546 15 3% OK 25% 38% 38%

A57 Mosborough Parkway /

Sheffield Parkway - Inbound 649 914 -265 -29% FAST 56% 44% 0%

A57 Mosborough Parkway /

Sheffield Parkway - Outbound 698 992 -294 -30% FAST 33% 33% 33%

Walkley to Sheffield 506 562 -56 -10% OK 60% 20% 20%

Sheffield to Walkley 370 459 -89 -19% FAST 75% 25% 0%

Penistone Rd - Inbound 872 1087 -215 -20% FAST 54% 25% 21%

Penistone Rd - Outbound 732 774 -42 -5% OK 36% 27% 36%

Overall 26607 30984 -4377 39% 24% 37%

Table E 3 Evening Peak Journey Time – By Route Segment

By Route

Section

Route Mod Obs Diff %Diff DMRB % Slow % Ok % Fast

Abbeydale Rd - Inbound 798 706 92 13% OK 27% 18% 55%

Abbeydale Rd - Outbound 739 829 -90 -11% OK 36% 27% 36%

Ecclesall Rd - Inbound 543 591 -48 -8% OK 29% 14% 57%

Ecclesall Rd - Outbound 557 1190 -633 -53% FAST 43% 43% 14%

Crookes Rd / A57 Western

Bank - Inbound 613 566 47 8% OK 33% 22% 44%

Crookes Rd / A57 Western

Bank - Outbound 555 597 -42 -7% OK 38% 13% 50%

A57 Fulwood Rd / Glossop Rd

- Inbound 669 761 -92 -12% OK 44% 11% 44%

A57 Fulwood Rd / Glossop Rd

- Outbound 617 627 -10 -2% OK 56% 0% 44%

Chesterfield Rd / London Rd -

Inbound 1006 842 164 19% SLOW 7% 43% 50%

Chesterfield Rd / London Rd -

Outbound 1038 1202 -164 -14% OK 36% 43% 21%

Rotherham to Sheffield via

Meadowhall 917 866 51 6% OK 36% 5% 59%

Sheffield to Rotherham via

Meadowhall 865 1033 -168 -16% FAST 35% 25% 40%

Rotherham to Sheffield via

Lower Don Valley 1966 1420 546 38% SLOW 46% 12% 42%

Sheffield to Rotherham via

Lower Don Valley 1665 1606 59 4% OK 38% 24% 38%

Middlewood Rd / Penistone Rd

- Inbound 826 773 53 7% OK 22% 17% 61%

Middlewood Rd / Penistone Rd

- Outbound 833 1189 -356 -30% FAST 44% 19% 38%

Chapeltown to Sheffield 1308 1288 20 2% OK 31% 23% 46%

Sheffield to Chapeltown 1317 1320 -3 0% OK 47% 7% 47%

Crystal Peaks / Manor Top to

Sheffield 984 858 126 15% OK 36% 14% 50%

Sheffield to Manor Top /

Crystal Peaks 938 915 23 3% OK 33% 8% 58%

Inner Ring Rd - Clockwise 1189 1651 -462 -28% FAST 44% 16% 40%

Inner Ring Rd - Anticlockwise 969 979 -10 -1% OK 43% 14% 43%

Page 114: Appendix B3 – Saturn Model Development Report

Outer Ring Rd - A6102 -

Clockwise 2279 2600 -321 -12% OK 38% 25% 38%

Outer Ring Rd - A6102 - Anti-

Clockwise 2002 1952 50 3% OK 38% 25% 38%

Sheffield Parkway - Inbound 542 637 -95 -15% OK 50% 25% 25%

Sheffield Parkway - Outbound 644 649 -5 -1% OK 13% 38% 50%

A57 Mosborough Parkway /

Sheffield Parkway - Inbound 725 822 -97 -12% OK 44% 22% 33%

A57 Mosborough Parkway /

Sheffield Parkway - Outbound 936 830 106 13% OK 11% 22% 67%

Walkley to Sheffield 713 817 -104 -13% OK 80% 0% 20%

Sheffield to Walkley 532 601 -69 -11% OK 50% 0% 50%

Penistone Rd - Inbound 1196 1265 -69 -5% OK 46% 8% 46%

Penistone Rd - Outbound 1051 1143 -92 -8% OK 41% 23% 36%

Overall 31532 33125 -1593 37% 19% 44%

Page 115: Appendix B3 – Saturn Model Development Report

Appendix F1 – Route Checking – Morning Peak

Fig F1 - 1 Ecclesall Rd to City Centre Zone 17

Fig F1 - 2 City Centre Zone 17 to Ecclesall Rd

Page 116: Appendix B3 – Saturn Model Development Report

Fig F1 - 3 Ecclesall Rd to City Centre Zone 7

Fig F1 - 4 City Centre Zone 7 to Ecclesall Rd

Page 117: Appendix B3 – Saturn Model Development Report

Fig F1 - 5 Hillsborough to City Centre

Fig F1 - 6 City Centre to Hillsborough

Page 118: Appendix B3 – Saturn Model Development Report

Fig F1 - 7 North to Lower Don Valley

Fig F1 - 8 Lower Don Valley to North

Page 119: Appendix B3 – Saturn Model Development Report

Fig F1 - 9 South to Lower Don Valley

Fig F1 - 10 Lower Don Valley to South

Page 120: Appendix B3 – Saturn Model Development Report

Fig F1 - 11 Rotherham to Sheffield

Fig F1 - 12 Sheffield to Rotherham

Page 121: Appendix B3 – Saturn Model Development Report

Fig F1 - 13 Through Trip – North to South

Fig F1 - 14 Through Trip – South to North

Page 122: Appendix B3 – Saturn Model Development Report

Fig F1 - 15 Through Trip – East to West

Fig F1 - 16 Through Trip – West to East

Page 123: Appendix B3 – Saturn Model Development Report

Fig F1 - 17 Sheffield to Waverley

Fig F1 - 18 Waverley to Sheffield

Page 124: Appendix B3 – Saturn Model Development Report

Appendix F – Route Checking – Inter-peak

Fig F2 - 1 City Centre Zone 17 – Ecclesall Rd

Fig F2 - 2 Ecclesall Rd – City Centre Zone 17

Page 125: Appendix B3 – Saturn Model Development Report

Fig F2 - 3 City Centre Zone 7 – Ecclesall Rd

Fig F2 - 4 Ecclesall Rd – City Centre Zone 7

Page 126: Appendix B3 – Saturn Model Development Report

Fig F2 - 5 Hillsborough to City Centre Zone 17

Fig F2 - 6 City centre Zone 17 to Hillsborough

Page 127: Appendix B3 – Saturn Model Development Report

Fig F2 - 7 Lower Don Valley - North

Fig F2 - 8 North to Lower Don Valley

Page 128: Appendix B3 – Saturn Model Development Report

Fig F2 - 9 South to Lower Don Valley

Fig F2 - 10 Lower Don Valley to South

Page 129: Appendix B3 – Saturn Model Development Report

Fig F2 - 11 Sheffield to Meadowhall

Fig F2 - 12 Meadowhall to Sheffield

Page 130: Appendix B3 – Saturn Model Development Report

Fig F2 - 13 Rotherham to Sheffield

Fig F2 - 14 Sheffield to Rotherham

Page 131: Appendix B3 – Saturn Model Development Report

Fig F2 - 15 Through Trip – North to South

Fig F2 - 16 Through Trip – South to North

Page 132: Appendix B3 – Saturn Model Development Report

Fig F2 - 17 Through Trip – East to West

Fig F2 - 18 Through Trip – West to East

Page 133: Appendix B3 – Saturn Model Development Report

Fig F2 - 19 Sheffield to Waverley

Fig F2 - 20 Waverley to Sheffield

Page 134: Appendix B3 – Saturn Model Development Report

Appendix F3 – Route Checking – Evening Peak

Fig F3 - 1 Ecclesall Rd to City Centre Zone 17

Fig F3 - 2 City Centre Zone 17 to Ecclesall Rd

Page 135: Appendix B3 – Saturn Model Development Report

Fig F3 - 3 City centre Zone 17 to Ecclesall Rd

Fig F3 - 4 Ecclesall Rd – City Centre Zone 7

Page 136: Appendix B3 – Saturn Model Development Report

Fig F3 - 5 Hillsborough to City Centre

Fig F3 - 6 City Centre to Hillsborough

Page 137: Appendix B3 – Saturn Model Development Report

Fig F3 - 7 North to Lower Don Valley

Fig F3 - 8 Lower Don Valley to North

Page 138: Appendix B3 – Saturn Model Development Report

Fig F3 - 9 South to Lower Don Valley

Fig F3 - 10 Lower Don Valley to South

Page 139: Appendix B3 – Saturn Model Development Report

Fig F3 - 11 Meadowhall to Rotherham

Fig F3 - 12 Rotherham to Meadowhall

Page 140: Appendix B3 – Saturn Model Development Report

Fig F3 - 13 Rotherham to Sheffield

Fig F3 - 14 Sheffield to Rotherham

Page 141: Appendix B3 – Saturn Model Development Report

Fig F3 - 15 Through Trip – North to South

Fig F3 - 16 Through Trip – South to North

Page 142: Appendix B3 – Saturn Model Development Report

Fig F3 - 17 Through Trip – South to North

Fig F3 - 18 Through Trip North to South

Page 143: Appendix B3 – Saturn Model Development Report

Fig F3 - 19 Sheffield to Waverley

Fig F3 - 20 Waverley to Sheffield

Page 144: Appendix B3 – Saturn Model Development Report

Appendix G – Trip Matrix Summaries

1 Key

1.1 For each of the three time periods, the prior matrix and post matrix estimation trip totals ( in

pcu’s) are shown, together with the absolute difference, percentage difference and GEH

value (a composite measure taking both absolute and percentage difference into account).

1.2 Any cells where the percentage change is greater than 50% is also highlighted in red.

1.3 Similarly, for the GEH tables, anything with a GEH value greater than 5 is highlighted in red.

Page 145: Appendix B3 – Saturn Model Development Report

Table G1 Initial Morning Peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 829 31 111 825 211 27 41 346 24 2,445

2 158 734 460 479 100 36 79 661 7 2,714

3 602 450 5,146 2,130 387 113 190 1,070 21 10,108

4 2,246 244 1,417 15,728 1,813 208 573 3,880 79 26,189

5 1,135 114 523 3,779 7,697 232 387 2,913 189 16,969

6 25 6 32 100 47 668 503 523 15 1,919

7 256 40 219 976 285 1,046 5,392 2,591 82 10,886

8 2,201 768 1,331 6,513 2,597 1,887 3,590 26,711 305 45,903

9 145 7 37 261 300 72 156 432 418 1,830

Total 7,597 2,393 9,276 30,792 13,439 4,289 10,911 39,126 1,140 118,964

Table G2 Final Morning Peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 1,117 63 158 1,480 601 47 115 576 83 4,241

2 197 381 743 200 60 36 67 518 3 2,206

3 858 424 5,177 1,978 278 164 281 1,399 19 10,579

4 2,474 208 1,289 15,795 2,020 181 639 3,941 100 26,646

5 1,163 52 493 4,217 8,334 142 291 3,062 221 17,976

6 17 12 23 95 35 881 477 511 18 2,068

7 212 85 254 1,134 254 1,068 5,767 2,569 160 11,503

8 2,044 571 1,685 5,833 2,703 2,358 3,180 26,280 308 44,962

9 140 1 26 320 328 67 217 483 434 2,016

Total 8,222 1,797 9,848 31,052 14,613 4,945 11,035 39,338 1,346 122,196

Page 146: Appendix B3 – Saturn Model Development Report

Table G3 Absolute Difference – Morning Peak

1 2 3 4 5 6 7 8 9 Total

1 288 33 47 655 390 20 74 230 59 1,796

2 40 -353 283 -280 -40 0 -12 -142 -4 -508

3 256 -26 31 -152 -109 52 91 330 -2 470

4 227 -36 -128 67 206 -27 66 61 20 457

5 28 -61 -30 438 637 -91 -95 149 33 1,007

6 -8 6 -9 -5 -12 213 -27 -12 3 149

7 -44 45 35 158 -31 22 376 -21 79 617

8 -157 -196 355 -680 106 471 -410 -432 3 -942

9 -5 -6 -11 59 27 -5 61 50 16 186

Total 625 -596 572 260 1,174 656 124 212 206 3,232

Table G4 Percentage Difference – Morning Peak

1 2 3 4 5 6 7 8 9 Total

1 35% 108% 42% 79% 185% 75% 178% 66% 245% 73%

2 25% -48% 62% -58% -40% 0% -15% -22% -55% -19%

3 43% -6% 1% -7% -28% 46% 48% 31% -8% 5%

4 10% -15% -9% 0% 11% -13% 12% 2% 26% 2%

5 2% -54% -6% 12% 8% -39% -25% 5% 17% 6%

6 -32% 99% -28% -5% -26% 32% -5% -2% 22% 8%

7 -17% 111% 16% 16% -11% 2% 7% -1% 96% 6%

8 -7% -26% 27% -10% 4% 25% -11% -2% 1% -2%

9 -3% -84% -29% 22% 9% -7% 39% 12% 4% 10%

Total 8% -25% 6% 1% 9% 15% 1% 1% 18% 3%

Page 147: Appendix B3 – Saturn Model Development Report

Table G5 GEH Difference – Morning Peak

1 2 3 4 5 6 7 8 9 Total

1 9.2 4.8 4.0 19.3 19.4 3.3 8.3 10.7 8.1 31.1

2 3.0 15.0 11.5 15.2 4.4 0.0 1.3 5.9 1.7 10.2

3 9.5 1.3 0.4 3.4 6.0 4.4 5.9 9.4 0.4 4.6

4 4.7 2.4 3.5 0.5 4.7 1.9 2.7 1.0 2.1 2.8

5 0.8 6.7 1.3 6.9 7.1 6.6 5.2 2.7 2.3 7.6

6 1.7 2.0 1.7 0.5 1.9 7.7 1.2 0.5 0.8 3.3

7 2.9 5.6 2.3 4.9 1.9 0.7 5.0 0.4 7.1 5.8

8 3.4 7.6 9.1 8.7 2.1 10.2 7.1 2.7 0.1 4.4

9 0.4 3.0 1.9 3.4 1.5 0.6 4.4 2.4 0.8 4.2

Total 7.0 13.0 5.9 1.5 9.9 9.6 1.2 1.1 5.8 9.3

Page 148: Appendix B3 – Saturn Model Development Report

Table G6 Initial Inter-peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 1,275 53 270 1,745 489 30 85 814 47 4,808

2 48 376 490 254 106 17 67 552 4 1,914

3 231 428 3,315 1,845 352 48 142 828 16 7,205

4 1,744 262 1,858 13,339 2,460 128 796 4,194 117 24,898

5 411 91 353 2,390 5,726 88 285 2,243 306 11,894

6 37 16 54 144 95 451 1,083 1,014 36 2,930

7 78 69 148 783 288 1,227 3,573 2,862 98 9,127

8 669 496 847 4,135 2,197 962 2,676 20,195 284 32,462

9 26 2 18 113 312 36 103 278 245 1,132

Total 4,519 1,793 7,353 24,748 12,024 2,986 8,811 32,978 1,156 96,368

Table G7 Final Inter-peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 1,776 46 263 1,915 748 28 115 986 73 5,951

2 43 165 710 177 50 9 43 478 1 1,676

3 319 660 3,757 2,021 143 51 182 942 7 8,082

4 2,048 165 1,993 15,161 2,641 121 833 4,307 112 27,382

5 387 54 218 2,432 6,379 48 253 2,151 429 12,351

6 25 27 62 124 63 868 1,144 1,112 55 3,480

7 82 90 156 786 235 1,218 4,575 3,023 176 10,342

8 807 364 829 4,929 2,329 1,011 2,618 19,434 288 32,608

9 32 1 11 110 393 34 128 310 260 1,279

Total 5,520 1,572 7,999 27,656 12,980 3,386 9,891 32,744 1,402 103,151

Page 149: Appendix B3 – Saturn Model Development Report

Table G8 Absolute Difference – Inter-peak

1 2 3 4 5 6 7 8 9 Total

1 501 -8 -7 170 259 -2 30 173 26 1,143

2 -5 -211 220 -77 -56 -8 -25 -74 -3 -238

3 88 233 442 177 -209 2 40 114 -9 877

4 304 -97 136 1,822 180 -7 37 114 -5 2,485

5 -24 -37 -135 41 653 -40 -32 -92 123 458

6 -12 11 8 -19 -32 416 61 99 18 550

7 4 21 8 4 -53 -9 1,002 161 78 1,215

8 138 -132 -19 794 133 49 -59 -762 4 147

9 6 -1 -8 -2 81 -2 25 32 15 148

Total 1,001 -221 646 2,909 956 400 1,080 -234 246 6,783

Table G9 Percentage Difference – Inter-peak

1 2 3 4 5 6 7 8 9 Total

1 39% -15% -2% 10% 53% -7% 36% 21% 54% 24%

2 -10% -56% 45% -30% -53% -47% -37% -13% -72% -12%

3 38% 54% 13% 10% -59% 5% 28% 14% -57% 12%

4 17% -37% 7% 14% 7% -5% 5% 3% -4% 10%

5 -6% -41% -38% 2% 11% -46% -11% -4% 40% 4%

6 -32% 70% 15% -13% -34% 92% 6% 10% 51% 19%

7 5% 30% 5% 0% -18% -1% 28% 6% 79% 13%

8 21% -27% -2% 19% 6% 5% -2% -4% 1% 0%

9 25% -48% -42% -2% 26% -5% 25% 12% 6% 13%

Total 22% -12% 9% 12% 8% 13% 12% -1% 21% 7%

Page 150: Appendix B3 – Saturn Model Development Report

Table G10 GEH Difference – Inter-peak

1 2 3 4 5 6 7 8 9 Total

1 12.8 1.1 0.4 4.0 10.4 0.4 3.0 5.8 3.3 15.6

2 0.7 12.8 9.0 5.3 6.3 2.2 3.3 3.2 1.8 5.6

3 5.3 10.0 7.4 4.0 13.3 0.3 3.1 3.8 2.7 10.0

4 7.0 6.6 3.1 15.3 3.6 0.6 1.3 1.7 0.5 15.4

5 1.2 4.4 8.0 0.8 8.4 4.9 1.9 2.0 6.4 4.2

6 2.2 2.4 1.1 1.7 3.6 16.2 1.8 3.0 2.7 9.7

7 0.4 2.3 0.6 0.1 3.3 0.3 15.7 3.0 6.6 12.3

8 5.1 6.4 0.6 11.8 2.8 1.6 1.1 5.4 0.2 0.8

9 1.2 0.7 2.0 0.2 4.3 0.3 2.4 1.9 0.9 4.3

Total 14.1 5.4 7.4 18.0 8.6 7.1 11.2 1.3 6.9 21.5

Page 151: Appendix B3 – Saturn Model Development Report

Table G11 Initial Evening peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 732 108 487 2,214 898 24 212 1,820 116 6,612

2 44 855 641 343 118 10 83 775 4 2,873

3 243 521 5,507 1,963 514 22 202 1,174 35 10,181

4 1,142 446 2,450 15,951 3,434 108 1,018 6,247 241 31,036

5 261 99 430 2,411 8,849 46 309 2,658 349 15,412

6 13 34 94 200 205 533 1,208 1,565 68 3,919

7 39 93 220 928 413 652 5,385 3,722 171 11,623

8 451 711 1,119 4,611 3,156 605 2,923 27,182 473 41,231

9 26 8 17 103 220 16 94 342 430 1,257

Total 2,951 2,875 10,965 28,723 17,807 2,017 11,435 45,484 1,887 124,143

Table G12 Final Evening Peak Matrix

1 2 3 4 5 6 7 8 9 Total

1 1,109 100 569 2,325 1,061 28 243 1,678 171 7,285

2 65 434 731 255 47 5 39 738 0 2,314

3 369 1,013 5,608 2,129 264 38 210 1,554 13 11,199

4 1,441 248 2,378 16,147 3,385 106 1,243 6,797 282 32,029

5 283 35 352 2,469 9,200 35 296 2,414 475 15,559

6 8 28 96 136 186 824 1,224 1,851 78 4,431

7 29 56 286 870 387 704 6,152 3,623 291 12,397

8 481 603 1,298 4,499 3,588 707 2,901 27,399 540 42,016

9 26 3 18 131 300 37 178 338 469 1,500

Total 3,811 2,520 11,335 28,962 18,417 2,484 12,486 46,392 2,320 128,730

Page 152: Appendix B3 – Saturn Model Development Report

Table G13 Absolute Difference – Evening Peak

1 2 3 4 5 6 7 8 9 Total

1 376 -8 82 111 164 4 31 -142 56 673

2 21 -421 90 -88 -71 -5 -44 -37 -3 -559

3 126 492 100 165 -250 16 9 380 -21 1,018

4 299 -198 -72 197 -48 -1 225 551 41 993

5 22 -63 -78 58 350 -11 -13 -244 126 148

6 -5 -5 2 -63 -19 291 15 286 10 512

7 -9 -37 65 -58 -27 51 767 -99 120 774

8 30 -108 179 -112 432 102 -22 217 67 785

9 0 -5 1 28 80 22 83 -4 38 243

Total 861 -355 370 239 611 468 1,051 908 434 4,587

Table G14 Percentage Difference – Evening Peak

1 2 3 4 5 6 7 8 9 Total

1 51% -8% 17% 5% 18% 15% 15% -8% 48% 10%

2 48% -49% 14% -26% -60% -54% -53% -5% -88% -19%

3 52% 95% 2% 8% -49% 72% 4% 32% -62% 10%

4 26% -44% -3% 1% -1% -1% 22% 9% 17% 3%

5 9% -64% -18% 2% 4% -23% -4% -9% 36% 1%

6 -36% -16% 2% -32% -9% 55% 1% 18% 14% 13%

7 -24% -40% 30% -6% -6% 8% 14% -3% 70% 7%

8 7% -15% 16% -2% 14% 17% -1% 1% 14% 2%

9 1% -67% 5% 27% 36% 138% 88% -1% 9% 19%

Total 29% -12% 3% 1% 3% 23% 9% 2% 23% 4%

Page 153: Appendix B3 – Saturn Model Development Report

Table G15 GEH Difference – Evening Peak

1 2 3 4 5 6 7 8 9 Total

1 12.4 0.8 3.6 2.3 5.2 0.7 2.0 3.4 4.6 8.1

2 2.8 16.6 3.4 5.1 7.8 2.0 5.7 1.3 2.3 11.0

3 7.2 17.8 1.3 3.7 12.7 2.9 0.6 10.3 4.4 9.8

4 8.3 10.6 1.5 1.6 0.8 0.1 6.7 6.8 2.6 5.6

5 1.4 7.7 3.9 1.2 3.7 1.7 0.7 4.9 6.2 1.2

6 1.4 1.0 0.2 4.9 1.4 11.2 0.4 6.9 1.1 7.9

7 1.6 4.3 4.1 1.9 1.3 2.0 10.1 1.6 7.9 7.1

8 1.4 4.2 5.2 1.7 7.4 4.0 0.4 1.3 3.0 3.8

9 0.0 2.4 0.2 2.6 5.0 4.2 7.1 0.2 1.8 6.5

Total 14.8 6.8 3.5 1.4 4.5 9.9 9.6 4.2 9.5 12.9

Page 154: Appendix B3 – Saturn Model Development Report

Appendix H – Trip Length Distributions

1 Key

1.1 The trips length distribution plots show variations in trip length distribution for Car, LGV and

OGV between the prior matrices and post matrix estimation matrices.

1.2 This analysis is presented looking at the 3 user class matrices that were run through matrix

estimation.

Page 155: Appendix B3 – Saturn Model Development Report

Morning Peak Car Trip Length Distribution

0

2

4

6

8

10

12

14

16

18

20

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H1 Morning Peak Trip Length Distribution for Cars

Page 156: Appendix B3 – Saturn Model Development Report

Morning Peak LGV Trip Length Distribution

0

5

10

15

20

25

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H2 Morning Peak Trip Length Distribution for Light Goods Vehicles

Page 157: Appendix B3 – Saturn Model Development Report

Morning Peak OGV Trip Length Distribution

0

10

20

30

40

50

60

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H3 Morning Peak Trip Length Distribution for Other Goods Vehicles

Page 158: Appendix B3 – Saturn Model Development Report

Inter Peak Car Trip Length Distribution

0

5

10

15

20

25

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H4 Inter-peak Trip Length Distribution for Cars

Page 159: Appendix B3 – Saturn Model Development Report

Inter Peak LGV Trip Length Distribution

0

5

10

15

20

25

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H5 Inter-peak Trip Length Distribution for Light Goods Vehicles

Page 160: Appendix B3 – Saturn Model Development Report

Inter Peak OGV Trip Length Distribution

0

5

10

15

20

25

30

35

40

45

50

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H6 Inter-peak Trip Length Distribution for Other Goods Vehicles

Page 161: Appendix B3 – Saturn Model Development Report

Evening Peak Car Trip Length Distribution

0

2

4

6

8

10

12

14

16

18

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H7 Evening Peak Trip Length Distribution for Cars

Page 162: Appendix B3 – Saturn Model Development Report

Evening Peak LGV Trip Length Distribution

0

5

10

15

20

25

30

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H8 Evening Peak Trip Length Distribution for Light Goods Vehicles

Page 163: Appendix B3 – Saturn Model Development Report

Evening Peak OGV Trip Length Distribution

0

10

20

30

40

50

60

70

80

0 to 2 2 to 4 4 to 6 6 to 8 8 to 10 10 to 12 12 to 14 14 to 16 16 to 18 18 to 20 20 to 22 22 to 24 24 to 26 26 to 28 28 to 30 Above30

Trip Length (km)

Perc

enta

ge o

f Tot

al T

rips

(%)

Before Matrix Estimation After Matrix Estimation

Figure H9 Evening Peak Trip Length Distribution for Other Goods Vehicles

Page 164: Appendix B3 – Saturn Model Development Report

Appendix I – Index of Important Files

1 Networks

Morning Peak sr07a447_6uc.dat

Inter Peak sr07i447_6uc.dat

Evening Peak sr07p447_6uc.dat

2 Matrices

Morning Peak sr07a447_6uc.ufm

Inter Peak sr07i447_6uc.ufm

Evening Peak sr07p447_6uc.ufm

3 Assigned Networks

Morning Peak sr07a447_6uc.ufs

Inter Peak sr07i447_6uc.ufs

Evening Peak sr07p447_6uc.ufs

4 Calibration Counts Files

All Counts Counts{A,I,P}027All.dat

Sheffield and Rotherham District Counts

Counts{A,I,P}027SheffandRoth.dat

5 Pelican Data

sr08pel08.dat

6 Coordinates File

Sr08a128.xy

7 Bus Route Files

Morning Peak sr08abus001.dat

Inter-peak sr08ibus001.dat

Evening Peak sr08pbus001.dat

Page 165: Appendix B3 – Saturn Model Development Report

8 Journey Time Files

Morning Peak 2007 routes - sr06aJTSh101a.dat

2006 routes - sr06aJTSh101b.dat

Inter-peak 2007 routes - sr06iJTSh101a.dat

2006 routes - sr06iJTSh101b.dat

Evening Peak 2007 routes - sr06pJTSh101a.dat

2006 routes - sr06pJTSh101b.dat

9 KR Files for Matrix Estimation

All Counts

Fully Observed Trips Frozen sr06{a,i,p}kr{c,l,o}001.dat

Sheffield and Rotherham Counts

Fully Observed Trips Frozen sr06{a,i,p}kr{c,l,o}002.dat

Sheffield and Rotherham Counts sr06{a,i,p}kr{c,l,o}003.dat

All Counts sr06{a,i,p}kr{c,l,o}004.dat

Page 166: Appendix B3 – Saturn Model Development Report

Appendix J – Method for Controlling Matrices to Tempro

Technical Note

Project Title: SRHM3

MVA Project Number: C37272

Subject: Method for Controlling Matrices to TEMPRO

Note Number: 02 Version: 1

Author(s): John Allan

Reviewer(s): Alice Woolley, Peter Kidd, James Blythe, Nick Benbow

Date: 10 March 2009

Introduction

To build the SATURN model matrices for the SRHM3 highway model, we carried out matrix

estimation on the SRHM2 matrices using new counts gathered since the Northern Inner Relief

Road was built. The matrix estimation was carried out with all car based journey purposes

gathered together into a single user class – because the traffic counts do distinguish between

journey purposes.

The SRDM3 model requires matrices at a very detailed level of journey purpose segmentations. To

build matrices for SRDM3 we had to transfer the impact of matrix estimation from the all-car

matrices to the individual journey purpose matrices built for SRHM2.

In building matrices for SRDM3, we have discovered a mismatch between the journey purpose

proportions in the model and those in TEMPRO. The model matrices have more employer’s

business trips and more non-home based trips than TEMPRO. However, we cannot match the

trip-ends exactly because for one journey purpose the fully observed trip ends exceed the

TEMPRO total by a large margin. We have investigated the processing of the roadside interview

data and concluded that the mismatch is carried through from the raw data.

The mismatch between the RIS data and TEMPRO probably reflects the differing biases inherent in

the two different survey approaches. In RIS, we may expect long distance trips to be over-

Page 167: Appendix B3 – Saturn Model Development Report

represented and short-distance trips to be under represented, this means that RIS may contain

a high proportion of employer’s business trips and a low proportion of eductation trips. OIn the

other hdand, household surveys, such as the one on which TEMPRO is based, tend to under

represent trips in the middle of trip chains so they will under represent non-home based trips

including non-home based employers business The true proportions are probably somewhere

between those estimated in the two different surveys.

We considered three possible approaches for controlling the SATURN trip-ends to match TEMPRO.

We have decided to use an approach that uses trip rates calculated from TEMPRO with

population data at zonal level.

Outline of the Approach

The broad approach is as follows:

Task 1 - Calculate 12-hour tour trip-rates from TEMPRO using the trip ends and

population data for the combined Sheffield and Rotherham districts, for the purposes HW,

HEB, HED ..

Task 2 - Calculate 12-hour to modelled-hour factors by purpose separately for from-home

and to-home matrices

Task 3 - Multiply the 12 hour trip rates by the 12-hour to modelled hour factors to

produce hourly trip rates

Task 4 - Apply the modelled hour trip rates to the zonal population data to produce hourly

trip ends - note that the zonal population will need to be controlled to the latest mid-year

population estimates because the population in Census seems very different from the

population in TEMPRO.

Task 5 - Use the hourly trip ends in MVGRAM to produce synthetic matrices (with intra-

zonals estimated using an estimated cost of half the cost to the nearest zone)

Task 6 - Calculate K-factors at sector level to ensure that the gravity model matches the

observed data and that the in-fill data sums to the target trip-end less the observed data

Task 7 - Re-run MVGRAM to produce revised matrices

Task 8 - Over write the fully observed cells with the fully observed data

Problem with NHBEB and an Adjustment

This approach will work for all the journey purposes except NHBEB for which the fully

observed demand exceeds the total forecast by TEMPRO. For NHBEB, we will build synthetic

matrices using trip ends calculated from the TEMPRO trip rates and we will overwrite the fully

observed cells with fully observed demand. We will not adjust the total to match TEMPRO.

The approach we have adopted for NHBEB will yield matrices that do not match the journey

purpose proportions in TEMPRO for either EB of NHB trips. In fact the matrices will end up

with EB and NHB proportions that lie somewhere in between the proportions in TEMPRO and

those in the original roadside interview surveys.

Page 168: Appendix B3 – Saturn Model Development Report

From what we know about the types of survey from which the two alternatives were

estimated, it seems reasonable to suppose that the true proportions lie somewhere between

the two. We expect that the roadside interview surveys have a bias towards boosting the

proportion of observed trips on longer journey purposes (such as employer’s business ) and

reducing the proportion of trips on shorter journey purposes (such as education trips). We

also expect that a household interview survey (such as NTS on which the TEMPRO trip ends

were based) is likely to yield underestimates of non-compulsory trips, employer’s business

trips and non-home based trips.

Task 1 Daily Trip Rates from TEMPRO

Task 1

Task 1 Calculate daily trip rates from TEMPRO

Objective To generate trip rates for each TEMPRO journey purpose – for car an public

transport

Inputs TEMPRO PA trips

TEMPRO variables

Census Variables

Processes Find a set of variables that are common to Census and TEMPRO so we can

calculate trip rates

Find variables that can take some account of

Outputs 14 trip rates – one 12-hour trip rate for car trips for each of the 7 journey

purposes and one rate for PT trips

We plan to use trip rates and population data to estimate production trip ends for the zones

in the study area. For the attractions, we plan to use attraction weights – which MVGRAM

will factor so that the trip productions are preserved.

We need to calculate rates in TEMPRO that can be applied at zonal level so we need

segmentation variables are available in both TEMPRO and our zonal data.

Trip rates could be calculated using the following TEMPRO variables

Households

Workers

Jobs

Population

Households by car ownership 0, 1 , 2, 3+

Total number of cars

Page 169: Appendix B3 – Saturn Model Development Report

Zone level Census data is available at for the trip end calculations for the following variables:

Residential population

Daytime population

Households

Households with a car

Households without a car

Jobs

Jobs reached by car

Jobs reached by PT

Jobs reached by other mode

Workers

Resident workers who normally drive

Resident workers who normally use PT

Resident workers who normally use another mode

Number of non-car owning households

We could try to take some account of car ownership levels by building car ownership data

into the trip rates. To achieve this, we need to use variables that are common to the two

data sets. The only possibility is to use the ratio of car owning households to total

households.

We assume that workers who want to buy a car will buy one so the car ownership level

within a zone will already be reflected in the numbers of workers within the zone. We

therefore have not applied the car ownership adjustment to commute trips or employers

business trips.

To produce trip rates for each purpose we have divided numbers of productions-attractions in

TEMPRO by the denominators in Table 1.

Trip Rate Denominators

Purpose Trip Rate Denominator

HBW Workers

HBEB Workers

HBED Population * households with car / Total

households

Page 170: Appendix B3 – Saturn Model Development Report

HBShop Population * households with car / Total

households

HBOther Population * households with car / Total

households

NHBEB Jobs

NHBO Population

Note that the productions-attractions in TEMPRO are outbound and return legs – to convert

home-based productions-attractions to the number of journeys you must multiply by 2. The

non-home based productions-attractions journeys in TEMPRO do not need to be multiplied by

two – they are already origin-destination journeys.

Having chosen the TEMPRO variables for the denominators for trip rates, we must identify

the corresponding variables in the Census data. These variables are set out in Table 2. Note

that the some of the fields in this table are not directly available from the census data rather

they have been calculated from other census variables. Examples include the number of

workers who travel to work by each mode, which we have summed over the modes provided

in the census data.

The calculation of trip demand for home based purposes will be constrained by the

production totals so we don’t need to produce attraction trip-rates. Instead we can use

attraction weights. The benefits of using attraction weights rather than trip rates is that the

variables used for the weights need not be common to both data sets, they can exist just in

the zonal data. That gives us a little more information that we can use to distribute the

commute trips according the car commute usage within the attraction zone.

Production Variables and Attraction Weights

Purpose Production Variable Attraction Weight

HBW Workers Daytime TTW by Car

HBEB Workers r Daytime TTW by Car plus PT

HBED resident population * Population

* households with car / Total

households

Resident population

HBShop resident population * Population

* households with car / Total

households

Daytime population

Page 171: Appendix B3 – Saturn Model Development Report

HBOther resident population * Population

* households with car / Total

households

Daytime population

NHBEB Jobs Daytime TTW by Car plus PT

NHBO Daytime population Daytime population

The output of this step will be a set of 14 trip rates: 7 journey

Page 172: Appendix B3 – Saturn Model Development Report

12-Hour to Modelled-hour Factors

Task 2

Task 2 Calculate hourly trip rates

Objective Generate factors to convert 12-hour trip rates into modelled hour trip rates

Inputs Observed RIS journey purpose proportions by modelled hour for the 12

hour day

Processes Separately for from-home and to-home trips, calculate the proportion of the

12-hour total that occur in the three modelled hours in the highway model –

0800 to 0900, average of 1000 to 1600 , and 1700 to 1800.

Multiply the 12-hour trip rates by the hour factors

Outputs 84 trip rates – one trip rate for for each combination of the 2 directions, 3

periods, 7 journey purposes, and 2 modes (car and PT)

Page 173: Appendix B3 – Saturn Model Development Report

Hourly Trip Ends

Task 3

Task 3 Calculate hourly trip-ends

Objective Create production trip-ends and attraction weights for the gravity model

Inputs Hourly trip-rates

Census data by zone – including attraction end data in the external zones

Observed productions from the external area to the internal area only (ie

exclude external to external trips)

Processes For internal area production trip-ends, multiplying the hourly trip rates by

the census data

For external area productions, use the observed trips to attractions within

the study area

Generate attraction weights by extracting the relevant census data by zone,

then factor the attraction weights to match the total productions – last step

may not be needed as MVGRAM may take care of it. We need attraction

data in the external area because some trips will be attracted from the study

area. Although the gravity model will only deal with internal area

productions we can use the full attraction data because the gravity model

will be set up so that it does not produce any external-to-external trips.

Outputs 84 sets of production trip ends and attraction weights – one for each

combination of the 2 directions, 3 periods, 7 journey purposes, and 2

modes (car and PT)

Page 174: Appendix B3 – Saturn Model Development Report

Task 4 - Initial MVGRAM

Task 4

Task 4 Calculate hourly trip rates

Objective Generate initial synthetic matrices for each purpose and time period

combination

Inputs Trip-ends from the previous process

X1 and X2 factors for the gravity models calibrated from the fully observed

RIS data

Distance skim matrices

Processes Zeroise the external-to-external cells in the skim matrices

Transpose the skim matrices for use with transposed the to-home

productions and attractions to make productions into rows in the matrices

Run gravity models separately for each journey purpose – separately for

home to work and work to home.

Run the models so productions are rows and attractions are columns – use

the normal skim for from-home and the transposed skim for to-home.

Outputs 84 trip matrices– one for each combination of the 2 directions, 3 periods, 7

journey purposes, and 2 modes (car and PT)

Page 175: Appendix B3 – Saturn Model Development Report

Task 5 Calculate K-factors

Task 5

Task 5 Generate K-Factors

Objective Generate a set of K-factors that can be used in a second run of the gravity

model to ensure it matches all the fully observed sector-to-sector and the

sector productions, so that we can be sure that the intra sector movements

have the correct totals

Inputs Observed RIS data

Mask to identify fully observed data and not fully observed data

Synthetic matrices from MVGRAM

Processes Identify the fully observed RIS

SQEX both fully observed RIS and synthetic matrices to the RIS sector

system

Divide SQEXed synthetic by RIS – to produce K-factors at sector level – note

the leading diagonal should be set to 1.0 as an experiment. We may need

to return to this step to set the leading diagonal factor so that the

productions in each sector match the synthetic totals. Check whether this

second step is necessary using one or two examples

Unsqex the factors to zone level.

Outputs 84 matrices of k-factors – one for each combination of the 2 directions, 3

periods, 7 journey purposes, and 2 modes (car and PT)

Page 176: Appendix B3 – Saturn Model Development Report

Task 6 Re-run MVGRAM

Task 6

Task 6 Generate K-Factors

Objective Rerun MVGRAM to produce synthetic matrices that both match both the

trip-end targets from TEMPRO and the fully observed movements at sector-

to-sector level

Inputs Trip-ends

X1 and X3 from the calibration

K-factors

Processes Run MVGRAM

Transpose the to-home matrices

Sum the from-home and to-home matrices

Outputs 84 synthetic matrices of hourly trips in PA format – one for each

combination of the 2 directions, 3 periods, 7 journey purposes, and 2

modes (car and PT)

Page 177: Appendix B3 – Saturn Model Development Report

Task 7 - Over write the fully observed cells with the fully observed data

Task 7

Task 7 Overwrite the fully observed cells

Objective Re-insert the fully observed RIS data into the trip matrices

Inputs Synthetic trips

Observed data from RIS

Mask matrices

Processes Mask the observed RIS to retain just the fully observed data

Mask the synthetic data to retain everything except the fully observed cells

Sum the masked matrices

Outputs 84 synthetic matrices of hourly trips in OD format – one for each

combination of the 2 directions, 3 periods, 7 journey purposes, and 2

modes (car and PT)

Page 178: Appendix B3 – Saturn Model Development Report

Task 8 - Over write the through trips

Task 8

Task 8 Overwrite the through trips

Objective Re-insert the through trips

Inputs Assignment matrices from the previous version of the model

Observed journey purpose proportions from RIS

Mask matrices

Matrices of trips from Task 8 (combined observed and synthetic for all the

trips with at least on trip-end inside the study area)

Processes Mask the old assignment matrices to produce just the external to external

trips

Apply JP splitting factors from RIS to get 5 user class assignment matrices

to our 14 user-class matrices

Add the masked matrices to the matrices of Task 8

Outputs 84 synthetic matrices of hourly trips in PA format – one for each

combination of the 2 directions, 3 periods, 7 journey purposes, and 2

modes (car and PT)

John Allan

Managing Consultant

Page 179: Appendix B3 – Saturn Model Development Report

Sheffield and Rotherham District SATURN Model 2008 4

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