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The Florida State University 1 [email protected] 1 st Joint GOSUD/SAMOS Workshop Sensitivity of Surface Turbulent Fluxes to Observational Errors or Where We Could Go Seriously Wrong Mark A. Bourassa and Paul J. Hughes Center for Ocean-Atmospheric Prediction Studies & Department of Meteorology, The Florida State University

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Page 1: Bourassa@met.fsu.edu 1 st Joint GOSUD/SAMOS Workshop The Florida State University 1 Sensitivity of Surface Turbulent Fluxes to Observational Errors  or

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Sensitivity of Surface Turbulent Fluxes to Observational Errors

or Where We Could Go Seriously Wrong

Mark A. Bourassa and Paul J. HughesCenter for Ocean-Atmospheric Prediction Studies &

Department of Meteorology,The Florida State University

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The Relevant Types of Errors Depend on the Application

Estimating a climatological heat flux Biases and sampling error (sampling vs. natural variability) are

important Satellite calibration

In many cases there are insufficient co-located observations to ignore random error.

Biases and random error are important Input for numerical weather prediction (NWP)

Biases and random error are important Approximately 95% of marine surface observations are rejected in

NOAA’s data assimilation. NWP is not an ideal application.

Climate comparisons If done correctly, dependent largely on errors in the mean (biases). Random error is small if there are enough observations.

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Suggested Measurement AccuracyFrom the Handbook

I will assume that a 5Wm-2 is the limit for biases in radiative fluxes.

Then 5Wm-2 is the limit for biases in surface turbulent heat fluxes.

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Historical and Modern Goals

During TOGA-COARE it was determined that a goal in surface turbulent flux observations was a bias of no more than 5Wm-2.

This same goal is currently being stated in comments on decadal satellite survey.

There have been several estimates on the observational accuracies required to achieve this goal.

HOWEVER these accuracies were determined for the environments being observed during TOGA-COARE (the tropical Pacific Ocean). The conditions in the tropical Pacific Ocean are somewhat

different from other parts of the globe. How much do the necessary observational accuracies change for

different environments? Are they applicable to each application?

I will describe how to determine these requirements, and discuss how to trade off strengths and weaknesses to minimize errors in fluxes. Good things to know when designing an observation system!

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Observational Errors

We are primarily interested in how biases in observations of wind speed (w), sea surface temperature (SST), near surface air temperature (Tair), and near surface humidity (qair) translate to biases in calculated fluxes. Sensible heat (H), latent heat (E), and stress ().

In general, the bias in one of these observations can be related to the bias in a flux through a Sensitivity (S).

Errors can be described as composed of A bias (this bias could be a function of environmental conditions), And a random uncertainty. The same tables can be used to determine the influence of the bias

and the uncertainty.

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Biases

To first order, the the biases can be calculated for each input variable, and then summed.

The maximum allowable bias in an observation (e.g., |w|) can be estimated from the maximum specified error in the calculated variable (e.g., |E|max), and the sensitivity (e.g., SE,w)

|w|max = |E|max / |SE,w|

The bias in a calculated variable (a flux) is equal to the sum of ‘sensitivity (S) times the bias in a input observation).

Example: How much does a bias in speed (w) contribute to a bias in the latent heat flux (E)?

E = SE,w w

If SE,w is very large, then even a small bias in w can result in a large bias in E.

If the sensitivity is very small, then the calculated variable is insensitive to errors in the observation.

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How is the Sensitivity Determined?

The sensitivity is the partial derivative of the output quantity (e.g., the flux) with respect to the input observation (e.g., wind speed).

SE,w = E/w

The sensitivity can be determined by solving the bulk formula, and using finite differences to determine the partial derivative of the drag coefficients.

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Example: Sensitivity of Sensible Heat Flux to Errors in Temperature (H/T)

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Example: Sensitivity of Sensible Heat Flux to Errors in 10m Wind Speed (H/w)

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Example: Sensitivity of Latent Heat Flux to Errors in Wind Speed: (E/q)/w

Air/sea humidity differences are also important.

A third dimension is awkward to work with. Therefore Sensitivity, per kg/kg is given.

Humidity differences are typically on the order of 1g/kg.

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Random Errors

If the random errors have a Gaussian distribution, which might be expected from the central limit theorem, then random errors are described by a standard deviation (, which is used a measure of spread).

If the latent heat flux (E) is written as a function of the input variables:

E = f(x1, x2, x3, x4),

Then the uncertainty in E () for a single observation can be written as

2

2

2 22 22 2 2 2 2

i

air air

E xi i

E w T SST qair air

f

x

E E E E

w T SST q

s s

s s s s s

æ ö¶ ÷ç ÷= ç ÷ç ÷÷ç¶è ø

æ ö æ öæ ö æ ö¶ ¶ ¶ ¶÷ ÷ç ç÷ ÷ç ç÷ ÷= + + +ç ç÷ ÷ç ç÷ ÷÷ ÷ç ç÷ ÷ç ç÷ ÷÷ ÷ç çè ø è ø¶ ¶ ¶ ¶è ø è ø

å

An uncertainty in the mean is equal to E divided by the squareroot of the number of independent observations.

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Error Limits for Observation Errors

For this talk, we will ignore random errors, assuming that they will be small given enough samples. This is a common assumption, but will not be true for all

applications! The maximum allowable bias in an observation (e.g., |w|) can be

estimated from the maximum specified error in the calculated variable (e.g., |E|), and the sensitivity (e.g., SE,w)

|w|max = |E|max / |SE,w|

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Example: How Much Bias in Wind Speed Can We Tolerate in Calculated SHF

We must be relatively accurate.

We can be relatively sloppy.

Assume a bias in SHF of <1.25 Wm-2 is OK.

Clim

ate

Acc

urac

y 0.

2 m

/s

Clim

ate

Acc

urac

y 0.

2 m

/s

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Example: How Much Bias in SST Can We Tolerate in Calculated SHF

Assume a bias in SHF of <1.25 Wm-2 is OK.

We can be extremely sloppy.

Can Gary Wick give us good satellite SST fields in a warm core seclusion?

Climate accuracy 0.1C

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Example: How Much Bias in Wind Speed Can We Tolerate in Calculated LHF

Fortunately, high winds are usually associated with unstable stratification (SST –Tair > 0).

In strong storms, we will not meet our accuracy requirement.

0.2 m/s (climate)

0.4 m/s (satellite)

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How Much Bias in Air Temperature Can We Tolerate in Calculated LHF

Not a problem!

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Saturation Vapor Pressure

‘Surface’ humidity is considered to be 98% or 100% of the saturation value, which is a strong function of temperature.

The Clausius-Clapeyron equation describes how the saturation vapor pressure changes with temperature.

where eo = 0.611 kPa, To = 273K, and Rv = 461 JK-1kg-1 is the gas constant for water vapor.

L is either the latent heat of vaporization (Lv = 2.5x106 Jkg-1), or the latent heat of deposition (Ld = 2.83x106 Jkg-1), depending on whether or not we are describing equilibrium with a flat surface of water or ice.

1 1exps o

v o

Le e

R T T

é ùæ ö÷çê ú÷= -ç ÷ê úç ÷çè øê úë û

Figure from Meteorology by Danielson, Levin and Abrams

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How Much Bias in SST Can We Tolerate in Calculated LHF?

For low temperature regions, we might what tighter accuracies than have been specified.

In areas with large q, there could be issues for very high winds and unstable stratification. Particularly so for

point comparisons

Recall that these numbers should be divided by q (in g/kg).

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Maximize Benefits of Improvements in Observations

How do we decide which instruments to improve? A ratio of sensitivities provides some indication of where

improvements to accuracy will have the greatest influence. That is, which type of observation is the best to improve. Technically this should be weighted by the cost and time involved

in the improvement. However, if you can estimate that it will take $x to make a certain

amount of improvement, you can determine where the money is best spent.

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When Will Improved Accuracy in Air Temperature and Speed Help The Most?

Examine the relative sensitivity of SHF to errors in Tair and wind speed:H/w / HTair

A ratio of 1 indicates an improvement of x m/s will equal the improvement of x C

Improving Tair has a greater impact

Improving w has a greater impact

Improving w has a greater impact

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Take Home Messages

The type(s) of error (bias, random, sampling) that are relevant depend on the application.

Errors (or uncertainties) in observed variables can be used to determine the biases (and uncertainties) in calculated variables.

The same sensitivity tables can used to determine both random errors and biases.

The current suggestions for accuracies are for the most part good enough for many applications; however, there are conditions for which they are insufficient.

Ratios of these sensitivities provides some insight into which instruments to improve to improve fluxes.

Suggested changes to accuracies: Tighter requirements for mean wind speed? Tighter mean SST accuracy would be nice, but can we do it? Tighter requirements preferred for satellite calibration.

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Suggested Measurement AccuracyFrom the Handbook

Wave data