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AGU 2002 Fall Meeting NASA Langley Research Center / Atmospheric Sciences QuickTim GIF deco are needed Validation of GOES-8 Derived Cloud Properties Over the Southeastern Pacific J. K. Ayers 1 , P. Minnis 2 , R. Wood 3 , P.W. Heck 1 , D. F. Young 2 , W. L. Smith, Jr. 2 , C. W. Fairall 4 , T. Uttal 4 1 Analytical Services and Materials, Inc, Hampton, VA 2 NASA Langley Research Center, Atmospheric Sciences, Hampton, VA 3 Atmospheric Sciences, University of Washington, Seattle, WA 4 NOAA ETL, Boulder, CO

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AGU 2002 Fall Meeting

NASA Langley Research Center / Atmospheric SciencesQuickTime™ and aGIF decompressorare needed to see this picture.

Validation of GOES-8 Derived Cloud Properties Over the Southeastern Pacific

J. K. Ayers1, P. Minnis2, R. Wood3, P.W. Heck1,

D. F. Young2, W. L. Smith, Jr.2,

C. W. Fairall4, T. Uttal4

1 Analytical Services and Materials, Inc, Hampton, VA

2 NASA Langley Research Center, Atmospheric Sciences, Hampton, VA

3 Atmospheric Sciences, University of Washington, Seattle, WA

4 NOAA ETL, Boulder, CO

AGU 2002 Fall Meeting

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Outline

• Introduction

• Cloud Property Retrieval – VISST/SIST Methodology

– Required Inputs

• Sample Cloud Properties– Hourly

• Pixel Level, Gridded

– Monthly• Gridded

• Validation– Tc, Zc, , re, LWP

• Conclusions

• Future Work

AGU 2002 Fall Meeting

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Introduction

• Why do we need satellite cloud products?– Very important climatic region

• ITCZ

• Stratocumulus region

• Southern hemispheric storm track

– Region is vast and in-situ measurements are limited

– Satellite cloud products are the only way to get near continuous coverage of the entire region

• Why do we need validation?– Without validation satellite products are suspect

– Provides means for correcting and proving algorithms

AGU 2002 Fall Meeting

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Methodology

• Visible Infrared Solar-Infrared Split Window Technique (VISST)– Daytime

– 0.65, 3.9, 10.8, 12.0 µm channels

– Utilizes parameterization of theoretical radiance calculations for 7 water and 9 ice crystal size distributions

– Retrieves cloud optical properties by matching calculations to observations

• Solar-Infrared Infrared Split Window Technique (SIST)– Night

– 3.9, 10.8, 12.0 µm channels

– Minimum error, iterative regression method

– Retrieves cloud optical properties by matching calculations to observations

AGU 2002 Fall Meeting

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Required Inputs

• Soundings from model runs or in-situ measurements

• Surface characterization from IGBP 10 minute map

• Uses CERES cloud mask algorithm

• Clear sky reflectances from CERES & GOES-based ocean model

• Narrowband to Broadband flux conversion functions from GOES-ERBE

• Satellite data (GOES-8, GOES-10) 4-km pixel resolution

AGU 2002 Fall Meeting

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Sample Products - Hourly Pixel Level (11/01/99 , 14:45 UTC)

Liquid Water Path

Cloud Height

Effective DropletRadius

Cloud MaskIce

Water

SLW

No Ret

Clear

AGU 2002 Fall Meeting

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Monthly Gridded Cloud Fractions (1°)April

Oct

Jan

July

AGU 2002 Fall Meeting

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Validation

• VISST/SIST– Analysis for a 1° box centered on the ship

– Solar zenith angle restricted to 82° or less

– Cloud limited to a single phase in most cases

– Appropriate properties adjusted by cloud fraction

• Fall 2000– 20 minute average centered on satellite image time

• Fall 2001– 60 minute average centered on image time

– 20 minute average centered on satellite image time (Cloud Height)

AGU 2002 Fall Meeting

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Fall 2000

AGU 2002 Fall Meeting

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Comparison of Satellite and Ceilometer Cloud Fraction(Fall 2000 Cruise)

VISSTCeilometer 0-20 20-40 40-60 60-80 80-100

0-20 20 5 3 0 020-40 1 1 2 2 040-60 2 3 3 1 360-80 0 1 1 2 3

80-100 2 3 2 2 47

Cmean = 64.3%, Vmean = 60.4%, StDev = 24%

AGU 2002 Fall Meeting

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Comparison of Radar and VISST Derived Cloud Heights ( Fall 2000 )

0

2

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0 2 4 6 8 10 12 14 16

Radar Cloud Height (km)

VISST Cloud Height (km)

High CloudMean Radar = 13.0 kmRMS = 0.99%RMS = 7.7Bias = 1.6N=11

Low CloudMean Radar = 1.92 kmRMS = 0.97%RMS = 50.0Bias = 0.14N = 29

AGU 2002 Fall Meeting

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Fall 2001

AGU 2002 Fall Meeting

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0

0.5

1

1.5

2

0 0.5 1 1.5 2

Radar Cloud height (km)

VISST Cloud Height (km)

Cloud Height Comparison

Mean Radar = 1.2 kmRMS = 0.27%RMS = 22.5Bias = 0.17N=54

AGU 2002 Fall Meeting

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Cloud Fraction Comparison

VISSTCeilometer 0-20 20-40 40-60 60-80 80-100

0-20 1 0 0 0 020-40 0 0 0 0 040-60 0 2 2 0 060-80 0 0 2 2 2

80-100 0 0 3 3 60

Cmean = 92.6%, Vmean = 84.3%, StDev =12%

AGU 2002 Fall Meeting

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278 280 282 284 286 288 290

Radiosonde Cloud Temperature (K)

Cloud Temperature Comparison

Mean Rad. = 281.8RMS = 0.85%RMS = 0.3Bias = -0.2N=56

AGU 2002 Fall Meeting

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45

0 5 10 15 20 25 30 35 40 45

MW+ST Optical Depth

Optical Depth Comparison

Mean MW+ST = 14.8RMS = 7.9%RMS = 54.2Bias = -0.66N=17

AGU 2002 Fall Meeting

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Liquid Water Path Comparison

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0 50 100 150 200 250 300 350

MW + ST LWP (gm-2)

Mean MW= 85.3RMS = 71.3%RMS = 83.6Bias = -51.7N=29

AGU 2002 Fall Meeting

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Effective Radius Timeline

AGU 2002 Fall Meeting

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0 5 10 15 20 25 30

MW+ST Effective Radius (µm)

Effective Droplet Radius Comparison

Mean MW+ST = 10.7RMS = 6.9%RMS = 65.4Bias = -6.3N=17

AGU 2002 Fall Meeting

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Conclusions

• Cloud amounts in good agreement, need to explore cases of poor agreement

• Cloud heights are as good as we can expect, some issues with overlap

• Diurnal cycles for all parameters show good agreement

• Magnitude of re differences in question

AGU 2002 Fall Meeting

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Future Work

• Explore cases of bad agreement for cloud amount

• Compare nocturnal cloud amount and heights

• Examine re differences more closely

• Evaluate microwave LWP using different techniques and compare with SSMI and TMI (on TRMM)

• Compare TOA albedos from VISST and surface with CERES instrument on TERRA

• Compute average lapse rate for each cruise to determine if a change in cloud height determination method is needed

• Continue producing products for the domain, implement improvements from comparisons