ceres fm1‐fm4 edion3 radiometric calibraon · 2009. 11. 18. · calibraon. susan thomas kory...

27
CERES FM1‐FM4 Edi-on3 Radiometric Calibra-on Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith, Norman Loeb CERES Science Team Meeting Fort Collins, Colorado November 3, 2009

Upload: others

Post on 24-Mar-2021

3 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERESFM1‐FM4Edi-on3RadiometricCalibra-on

Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar

Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith, Norman Loeb

CERES Science Team Meeting Fort Collins, Colorado

November 3, 2009

Page 2: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

Edi-on3Studies1. Gain Adjustments

Incorporate all known changes in gain and other calibration coefficients for each instrument based on the on-board calibration results.

2. Beginning of Mission Spectral Response Functions

Reassess the ground calibration data and determine the spectral response function for the Shortwave and the Total sensors.

3. Set the CERES instruments on the same radiometric scale at mission start

Develop the methodology to place all CERES instruments on the same rad. scale.

4. Determine optimal Spectral Response Function to correct for the on-orbit degradation in Shortwave region

Direct comparison approach is used to correct the change in the SW sensors.

Regression on the Day-Night differences of Longwave and Window measurements on each instrument is used to correct for the degradation in the shortwave region of total sensor.

Page 3: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

GainAdjustments

Thein‐flightgainchangesweredeterminedusingtheon‐boardBlackbodysourcesandtheSWICS.

Themonthlyvaria-oninthetotalandwindowsensorgainswerereducedwithafivemonthrunningmeanapproach.

TheBlackbodyandSWICScalibra-ondatacollectedduringgroundtes-ngwerereevaluatedandincorporatedforthegroundtoflightchangesinthesensorgains.

Page 4: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERESFM1GAINCORRECTIONS

In-Flight Gain Adjustment

0.997

0.998

0.999

1.000

1.001

1.002

1.003

1.004

1.005

1.006

1.007

3/00 3/01 3/02 3/03 3/04 3/05 3/06 3/07 3/08 3/09 3/10

Sen

sor

Res

po

nse

Ch

ang

e

TOTAL WN SW

GroundtoFlightSensorResponsechange:

Total Window Shortwave

0.989 1.004 0.995

‐1.1% +0.4% ‐0.5%

Page 5: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERESFM2GAINCORRECTIONSGroundtoFlightSensorResponseChange:

Total Window Shortwave

0.9888 1.0161 0.9999

‐1.12% +1.61% ‐0.01%

In-Flight Gain Adjustment

0.997

0.998

0.999

1.000

1.001

1.002

1.003

1.004

1.005

1.006

1.007

1.008

3/00 3/01 3/02 3/03 3/04 3/05 3/06 3/07 3/08 3/09 3/10

Sen

sor

Res

po

nse

Ch

ang

e

TOTAL WN SW

Page 6: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

AQUA:CERESFM3&FM4GAINCHANGESCERES FM3 In-Flight Gain Corrections

0.990

0.992

0.994

0.996

0.998

1.000

1.002

1.004

1.006

1.008

1.010

7/02 12/02 7/03 12/03 6/04 12/04 6/05 12/05 7/06 12/06 7/07 12/07 6/08 12/08 6/09 12/09

Sen

sor

Res

pons

e C

hang

e

TOTAL WN SW

CERES FM4 In-Flight Gain Corrections

0.990

0.992

0.994

0.996

0.998

1.000

1.002

1.004

1.006

1.008

1.010

7/02 12/02 7/03 12/03 6/04 12/04 6/05 12/05 7/06 12/06 7/07 12/07 6/08 12/08 6/09 12/09

Sen

sor

Res

pons

e C

hang

e

TOTAL WN SW

Page 7: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

Edi-on3Studies1. Gain Adjustments

Incorporate all known changes in gain and other calibration coefficients for each instrument based on the on-board calibration results.

2. Beginning of Mission Spectral Response Functions

Reassess the ground calibration data and determine the spectral response function for the Shortwave and the Total sensors.

3. Set the CERES instruments on the same radiometric scale at mission start

Develop the methodology to place all CERES instruments on the same rad. scale.

4. Determine optimal Spectral Response Function to correct for the on-orbit degradation in Shortwave region

Direct comparison approach is used to correct the change in the SW sensors.

Regression on the Day-Night differences of Longwave and Window measurements on each instrument is used to correct for the degradation in the shortwave region of total sensor.

Page 8: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERESSpectralResponseFunc-onFM1Edi-on2‐StartofMission

-0.2

0

0.2

0.4

0.6

0.8

1

0.1 1 10 100

Sen

so

r R

esp

on

se

Wavelength (microns)

TOTAL SW WINDOW

Page 9: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

SpectralResponseFunc-onEvalua-on

Measurementsfromthepre‐launchtestdatawerere‐analyzedtodeterminetheop-malSpectralResponseFunc-on(SRF)forCERESsensors.

SHORTWAVEREGION:Componentmeasurementsre‐evalua-on:Silverdatafromdifferentcoa-ngruns.

Impactofshortwavereferencesource(SWRS)spectralthroughputonband‐passfiltersusedinthedetermina-onofGain/SRF.

LONGWAVEREGION:

TheFourierTransformSpectrometer(FTS)measurementanalysistodeterminetheSRFintheLongwaveregion.

MohanShankar’spresenta-oninADMWGwillgivedetaileddescrip-onofSpectralResponseFunc-ondetermina-on.

Page 10: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERES FM1 SW Spectral Response Function

0.72

0.74

0.76

0.78

0.80

0.82

0.00 0.50 1.00 1.50 2.00 2.50 3.00 3.50 4.00

Wavelength, microns

Sen

sor

Resp

on

se

Edition3 Edition2

CERES FM2 SW Spectral Response Function

0.72

0.74

0.76

0.78

0.80

0.82

0.00 0.50 1.00 1.50 2.00 2.50 3.00 3.50 4.00

Wavelength, microns

Sen

sor

Resp

on

se

Edition3 Edition2

Page 11: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERES FM1 & FM2 Total Sensor Spectral Response Functions

-0.2

0

0.2

0.4

0.6

0.8

1

0.1 1 10 100 1000

Wavelength (microns)

Resp

on

se

FM1- Edition 3 FM2- Edition 3 FM1_Ed1CV FM2_Ed1CV

Page 12: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

TERRARadianceComparisonEdi-on2andEdi-on3SpectralResponseFunc-on

ALLSKYGlobalFluxResultsforMarch2000basedonERBE‐LikeES‐8product

NADIRdata

FM1 FM2

Edi-on3Wm‐2

Edi-on2Wm‐2

Ed3‐Ed2 Edi-on2Wm‐2

Edi-on3Wm‐2

Ed3–Ed2

LWday 231.77 230 0.77% 231.84 230.95 0.38%

LWnite 224.61 225.28 ‐0.3% 223.63 224.89 ‐0.56%

SW 256.20 253.59 1.03% 255.52 253.48 0.8%

Page 13: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERES FM3 SW Spectral Response Function

0.50

0.55

0.60

0.65

0.70

0.75

0.80

0 1 2 3 4 5

Wavelength, microns

Sen

sor

Resp

on

se

Edition3_Test Edition2

CERES FM4 SW Spectral Response Function

0.50

0.55

0.60

0.65

0.70

0.75

0.80

0 1 2 3 4 5

Wavelength, microns

Sen

sor

Resp

on

se

Edition3_Test Edition2

Page 14: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

AQUA: CERES FM3 & FM4 Total Sensor Spectral Response Functions

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0.10 1.00 10.00 100.00 1000.00

Wavelength (microns)

Sen

so

r R

esp

on

se

FM3-Ed3Test FM4-Ed3Test FM3-Ed2 FM4-Ed2

Page 15: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

Edi-on3Studies1. Gain Adjustments

Incorporate all known changes in gain and other calibration coefficients for each instrument based on the on-board calibration results.

2. Beginning of Mission Spectral Response Functions

Reassess the ground calibration data and determine the spectral response function for the Shortwave and the Total sensors.

3. Set the CERES instruments on the same radiometric scale at mission start

Develop the methodology to place all CERES instruments on the same rad. scale.

4. Determine optimal Spectral Response Function to correct for the on-orbit degradation in Shortwave region

Direct comparison approach is used to correct the change in the SW sensors.

Regression on the Day-Night differences of Longwave and Window measurements on each instrument is used to correct for the degradation in the shortwave region of total sensor.

Page 16: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

PlacementofCERESmeasurementsonsameRadiometricScale

•  CERESmeasurementsfrom5differentinstrumentsspan12years(1998‐2009).

TRMM‐PFM:January–August1998,March2000Terra–FM1&FM2:March2000–PresentAqua–FM3&FM4:July2002‐Present

•  ThesameradiometricscaleattheBeginningofMissionMarch2000forTerraandJuly2002forAqua

•  FM1isselectedtobetheclimateinstrument:–  Producesthelongest,con-nuousdataset–  Longestincross‐trackmodeofopera-on–  Showsthesmallestspectralchangesforthemission–  Showsthebestconsistencyforthe3‐channelcomparison–  HasbeenusedtocomparewithAQUAsince2002

Page 17: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

TesttosetCERESFM1asreference

•  DirectcompareofCERESFM1andFM2basedonERBE‐LikeES‐8product–  ProposedEdi-on3dataforMarch2000–  Comparisonattheunfilteredradiancelevel

•  matchedgeometryofmeasurementsforVZA<60°–  1500comparisonregionsfordayornightinonemonth

–  Averagingover1°×1°grid–  Forallthreechannelsandallscenetypes

Page 18: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

ComplementaryTests•  DirectcompareofFM1orFM2andPFM:–  ThesameapproachasforTerra

•  Edi-on2,March2000PFMdata•  PFMgeometrymatchedbyFM1orFM2(PAPSmode)

•  DeepConvec-veCloud(DCC)SWalbedo–  SSFdatawasusedtodefinedeepconvec-veclouds

•  DirectcompareofFM1andFM2basedonSSF–  ClearOcean(CLRO)andDCCsubsets–  Nearnadirmeasurements–  Imagerinforma-oninselec-ngmatchedfootprints

•  DirectcompareofTerrafootprintsatnadir(ES8)

Page 19: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

RequiredshiqsfortheTerraInstrumentsatBeginningofMission

•  Directcompareandothertestsshowsa-sfactoryconsistency,andsta-s-callysignificantdifferences(@2sigmalevel)inthe3channels:

•  AdjustmentstotheCERESFM2Measurements–  Shortwave(SW)shouldberaisedby0.22%–  LW_dayshouldbedecreasedby0.05%–  LW_nightshouldberaisedby0.4%– Window(WN)shouldberaisedby0.45%

Z.PeterSzewczykpresenta-onintheADMWGwillcovertheintercomparisonstudyindetail.

Page 20: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

Edi-on3Calibra-onSummary1. Gain Adjustments

ThegainchangesforTerraInstrumentsfromMarch2000–Dec2004weredeliveredforproduc-on.ThegainsfromJan2005–Mar2009arebeingvalidated.TheradiometricgainchangesfortheAquaInstrumentswerederived.

2. Beginning of Mission Spectral Response Functions

Theevalua-onofSpectralResponseFunc-onsforTerraInstrumentswerecompletedanddelivered.TheBOMSpectralResponseFunc-onsforAquaInstrumentsarecurrentlyundertes-ng.

3. Set the CERES instruments on the same radiometric scale at mission start

CERESFM1instrumentisselectedasthestandardinstrument.ThecomparisonstudiesbetweenFM1andFM2instrumentswerecompleted.Thecorrec-onvaluestobringTerrainstrumentsonthesameradiometricscalewerederived.

Page 21: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

Edi-on3Studies1. Gain Adjustments

Incorporate all known changes in gain and other calibration coefficients for each instrument based on the on-board calibration results.

2. Beginning of Mission Spectral Response Functions

Reassess the ground calibration data and determine the spectral response function for the Shortwave and the Total sensors.

3. Set the CERES instruments on the same radiometric scale at mission start

Develop the methodology to place all CERES instruments on the same rad. scale.

4. Determine optimal Spectral Response Function to correct for the on-orbit degradation in Shortwave region

Direct comparison approach is used to correct the change in the SW sensors.

Regression on the Day-Night differences of Longwave and Window measurements on each instrument is used to correct for the degradation in the shortwave region of total sensor.

Page 22: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

BACKUPSLIDES

Page 23: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERES FM2 In-Flight Gain Adjustment

0.997

0.998

0.999

1.000

1.001

1.002

1.003

1.004

1.005

1.006

1.007

1.008

3/00 3/01 3/02 3/03 3/04 3/05 3/06 3/07 3/08 3/09 3/10

Se

ns

or

Re

sp

on

se

Ch

an

ge

TOTAL WN SW Total -Ed2

Page 24: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

CERESFM1&FM2ComparisonsResultsbasedonAll‐sky(ES‐8product)

FM2Radiance(Wm‐2)

RadianceDifference(FM2‐FM1)

Difference%change

73.73 0.04 0.05

70.24 ‐0.23 ‐0.4

72.72 ‐0.16 ‐0.22

5.14 ‐0.02 ‐0.47

4.81 ‐0.02 ‐0.47

Page 25: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

TRMM–TERRAComparisonsFM1‐PFMResultsforAll‐Skyscene

Unfiltered Radiance

µ FM1

Δµ Δµ %µ

LW_day 85.69 -0.08 -0.10

LW_night 80.98 -0.46 -0.56

SW 73.63 0.20 0.28

FM2‐PFMResultsforAll‐Skyscene

Unfiltered Radiance

µ FM2

Δµ Δµ %µ

LW_day 85.59 -0.04 -0.05

LW_night 80.57 -0.78 -0.97

SW 70.93 -0.24 -0.34

Page 26: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

SSFDCCbasedSWAlbedo

TERRAFM1‐FM2Comparison:FM1andFM2albedoresultsfrommatchedfootprintsare0.721and0.720respec-vely.

TRMM–TERRAComparison:PFM,FM1andFM2albedoresultsare0.709,0.705and0.7respec-vely.

Page 27: CERES FM1‐FM4 Edion3 Radiometric Calibraon · 2009. 11. 18. · Calibraon. Susan Thomas Kory Priestley, Phillip Hess, Mohan Shankar Z. Peter Szewczyk, Dale Walikainen Navtidad M-Smith,

FM1ThreeChannelComparison

Day@meNadirslope(fSWvs.DeltaLW)

Edi-on1‐CV ‐0.0208

Edi-on‐3 ‐0.0036