hernan moreno - a vectorialmodel to compute terrain parameters and solar radiation on tin domains

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2015 CUAHSI Conference on Hydroinformatics

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  • A Vectorial Model to Compute Terrain Parameters and Solar Radiation

    on TIN Domains.Hernan A. Moreno

    Fred OgdenRobert C. Steinke

    Nels Frazier

    Department of Civil and Architectural EngineeringUniversity of Wyoming

    EPSCoREPS1135483

    3rd Conference on Hydroinformatics-2015

  • Outline

    Motivation Application Basin TIN Properties Solar Vector Computation Radiation on Inclined Surfaces Local and Remote Shading Next Steps

  • Motivation TINs provide economy and

    versatility. Tessellations improve

    representation of topography. Fewer data points allow storage

    and processing economy. Faster processing times than

    DEMs which scale well with parallel runs.

    Model large basins or small basins with very fine resolution.

  • Motivation Preserving high resolution at process-active areas is

    critical for accurate modeling.

    -Elevation - Slope- Aspect- Solar radiation- Evaporation- Transpiration

    - Runoff & surface flow- Erosion & transport- Infiltration- Subsurface flow- Channel formation- Energy balance

    - Surface-subsurface water interactions- Variable saturated areas- Solar energy potential- Snow accumulation and melt- Contaminant fate and transport- Soil moisture

  • Insolation modeling

    Measurement Pro ConInterpolation of point measurements

    Highly accurate source to interpolate.

    Expensive. Poorly performance in complex topography.

    Meteorologicgeostationary satellites

    Large areal coverage at relatively low cost.

    Low spatio-temporal resolution.Only work under clear sky conditions.

    Spatially-based solar radiation models

    Cost-efficient way with high spatio-temporalresolution

    So far they have only been tested in DEMs with time-expensive routines.

    We propose an efficient and novel methodology for rapid calculation of topographic parameters (slope and aspect) and to better estimate INSOLATION on TIN elements for hydrologic applications.

    INSOLATION=SWdir + SWremote + SWdiffuse

  • Study Basin

    Basin Area: 1220 km2

  • THANKS

    Green River, Wyoming

  • TIN properties

    DEM=158,325 cellsTIN=36,436 elements

    DEM

    TIN

  • P1

    P2

    P3

    n=(P3-P1)x(P2-P1)

    z

    x

    y

    Normal Unit Vector

    nx

    nz

    S

    S

    kn+jn+in=n uzuyuxu

    nn+jnn+inn=n zyxu 0> zzyx nk;n+jn+in=nSlope of plane from normal vector

    Slope of plane from eq. plane

    Equation of the plane

    ( )uzn=S arccos

    0=d+Zn+Yn+Xn zyx

    22

    yz+

    xz=S'

  • nux

    Mean Median St. Dev. Skewness

    -0.012 -0.0005 0.042 -0.003

  • nuy

    Mean Median St. Dev. Skewness

    -0.0024 -0.0037 0.0454 0.00026

  • nuz

    Mean Median St. Dev. Skewness

    0.9504 0.9879 0.9125 0.8811

  • Slope S

    ( )uzn=S arccos

  • Slope S'

    22

    yz+

    xz=S'

  • S'- S

  • S' Vs S

    SS'

    Slope 1st Quartile Mean Median 3rd Quartile Std. Dev. Skewness

    S 4.146 13.2406 8.9125 18.386 340.861 12757

    S' 4.153 14.5406 8.9851 19.044 463.487 22877

  • Slope Aspect

    | |

    nxny

    nxnx=A arctan

    2

  • Solar Vector

    Topocentric Spheric System

    At noon sun is at:

    ( )ozoyoxo S,S,S=S( ) ( )( ),So = cossin0,

    latitude Triangle=9090

    ndeclinatio Solar=

    23.4523.45

  • System RotationAs Earth rotates, So needs to be multiplied by three rotational matrices. Thus solar vector will be

    ( ) ( ) ( ) oxzx Srwrr=S ( )

    =rx

    cossin0

    sincos0

    001

    ( )

    100

    0

    0

    cossin

    sincos=wrz

    anglehour=

    +cosw

    sincos

    cossin=S

    sinsincoscos

    coscossin

  • Cosine lawLambert's cosine law determines the energy flux to each TIN element:

    ( )

    +cos

    sincos

    cossinn,n,n= uzuyuxs

    sinsincoscos

    coscossin

    cos

    nu

    Ss

    Direct Radiation(w/m2)

    Sn= us .cos

    When cos s

  • Incoming Solar Radiation

    Spring or fall Equinox

  • Incoming Solar Radiation

    Winter Solstice

  • Incoming Solar Radiation

    Summer Solstice

  • Remote ShelteringIn process of application. Groups of mesh elements are organized along the sun light path and their projections tested for remote shading.

    z

    x

    S

    TIN centroids

    T1 T2 T3 T4 T5 T6 T7

    Shaded elements

    SP

    d( )h+Rh=d 2

  • Next Steps Include a diffuse radiation model based on sky-view

    factors.

    Add a remote reflected radiation for short wave or high albedo areas.

    Include a module for canopy light reduction and below-canopy long wave radiation.

    Include an energy balance model. Couple a snow and evapotranspiration module. Couple modules to ADHydro infiltration and routing

    schemes.

  • THANKS

    Green River, Wyoming

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