+ All Categories
Home > Documents > Simultaneous Nadir Overpass (SNO) Matchups GOSAT ......Intro The Greenhouse Gases Observing...

Simultaneous Nadir Overpass (SNO) Matchups GOSAT ......Intro The Greenhouse Gases Observing...

Date post: 10-Oct-2020
Category:
Upload: others
View: 6 times
Download: 0 times
Share this document with a friend
1
Results Simultaneous Nadir Overpass (SNO) Matchups GOSAT/TANSO - FTS and AQUA/AIRS: TIR Band April 2009 December 2015 Robert Knuteson 1 , G. Burgess 1 , K. Shiomi 2 , A. Kuze 2 , J. Yoshida 3 , F. Kataoka 4 , and H. Suto 2 1 Space, Science, and Engineering Center, University of Wisconsin – Madison, 2 Japan Aerospace Exploration Agency, Tsukuba-city, Ibaraki, Japan, 3 NEC Cooperation, Fuchu, Tokyo, Japan, 4 Remote Sensing Technology Center of Japan, Tsukuba-city, Ibaraki, Japan Intro The Greenhouse Gases Observing Satellite (GOSAT) was launched in January 2009, to monitor global atmospheric concentration and flux of CO2 and CH4 from space. The TANSO-FTS sensor is an interferometer spectrometer measuring shortwave reflected solar radiation with high spectral resolution in three spectral bands. A bore-sighted band 4 uses the same interferometer to measure thermal infrared radiation (TIR) at the top of the atmosphere. This paper is a comparison of the TANSO-FTS TIR band with coincident measurements of the NASA Atmospheric InfraRed Sounder (AIRS) grating spectrometer. The time and space coincident matchups are at the Simultaneous Nadir Overpass (SNO) locations of the orbits of GOSAT and the NASA AQUA satellite. GOSAT/AQUA SNOs occur at about 40N and 40S latitude. A continuous set of SNO matchups has been found from the start of valid radiance data collection in April 2009 through the end of 2015. UW-SSEC has obtained the time, latitude, and longitude of the SNO location using the ORBNAV software at http://sips.ssec.wisc.edu/orbnav. UW-SSEC obtained the matching AIRS v5 L1B radiances from the NASA archive. JAXA has reprocessed the entire TANSO-FTS TIR band using the previous v161.161 and a new calibration version which includes parameter optimizations. The TANSO-FTS has been reduced to the AIRS spectral channels using the AIRS spectral response functions (SRFs). This paper will show the time series of observed brightness temperatures from AIRS and GOSAT TANSO-FTS TIR observations from the SNO matchups. This poster illustrates the satellite inter-calibration data used to validate the improvements in the GOSAT ground calibration software by providing an independent reference to the AIRS on-orbit calibration accuracy. Improvements in the ground calibration software are expected to lead to improvements in the TIR band Level2 retrievals of CO2 profiles Co n tact: ro b ert.k n u teso n @ ssec.w isc.ed u UW-Madison SSEC References Kuze, A., Suto, H., Shi omi, K ., Urabe, T., Naka j ima , M., Yos h ida, J., .. &Buij s , H. (2 01 2). Le v e l 1 a lgo rith ms fo rT ANSO on GOSAT: proc e ssi n g a nd on-orb it calibrations. Atmo s .Me a s. Te c h , 5 (1 0 ), 2 44 7 - 2467. Kuze, A., SUto,H., Sh i omi , K., Na ka j ima , M., &Bu i j s,H. (20 1 3, Ju ne ). Ex peri en c e ga i n ed f rom GOSAT: FTSapp l i ca ti onfor wi despectra l ran ge observation. I n Fo u rie r Tra ns form Spec tros co py (pp. F W3 D-3). Optic a l Soc i ety o f Ame ri c a. Kuze, A., Suto, H., Shi omi, K ., & Nak a j i ma , M. (2 01 1, Ju l y). Le ss on s l ea rn ed from GOSAT an d impro ve me n ts fo r the ne xt mi ss io n . In F o uri er T ran sfo rm Spectroscopy (p. JMA3 ). Optic a l Soc i ety o f Ame ri ca . Kataoka, F., Knuteson, R. O., Kuze,A., Suto, H., Shi omi, K ., Ha ra da, M., .. & Rev erc omb, H. E. (2 01 4 ). T IRs pe c tra l ra dia n ce ca li brati on of the GOSAT s a te l l i te bo rne TANSO-F T S wi th the a i rc raft-bas ed S-HIS an d t he gro un d-ba se d S-AERI at t he Rail road Va lley desert play a. Geos c i e nc e a nd Re mo t e Se n s i n g, IEEE Tra n sa cti on s o n , 52(1 ), 8 9-1 0 5. Gero, P. J., Knuteson, R. O., Sh iomi,K., Kuz e, A., Kat aoka,F.,Revercomb, H. E., ... &Best, F. A. (2014, November). GOSAT TANSO FTS TIR band calibration: a fi ve ye ar re vi ew. In SPI E Asia Pac ifi c Remo te Se n si ng (pp. 92 6 31 6-9 2 63 16 ). In tern ati on a l Soc i ety forOptics and Photon i c s. A ckno w ledg ments This work was supported by JAXA through atask order with UW-SSEC. Summary The SNO method is used to make a direct assessment of the absolute calibration and stability of the GOSAT TIR spectra. The NASA AIRS sensor is used as a reference of comparison due to it’s well established calibration accuracy and stability. The GOSAT TIR radiance was reprocessed at the Aqua/GOSAT SNOs location for the time period April 2009 – December 2015 using JAXA ground processing version 161. The version 161 is seen to exhibit a calibration cold bias at several points in the infrared spectrum including the 15 micron CO2 band. A time series analysis shows that the bias is stable from April 2009 through May 2014 when it undergoes a step change to a colder bias. The root cause of this bias and the step changes have been addressed in JAXA ground processing version 200+. Future work includes validation of v200+ with AIRS & IASI SNOs. Method Data GOSAT TIR GOSAT radiances are from v161 provided by JAXA after consistent reprocessing. TIR radiances were provided only at SNO locations. AIRS Sounder The orbit of the Aqua satellite is polar sun-synchronous with a nominal altitude of 705 kilometers (438 miles) and an orbital period of 98.8 minutes, completing approximately 14.5 orbits per day. The satellite equatorial crossing local times are 1:30 a.m. in a descending orbit, and 1:30 p.m. in an ascending orbit. A grating spectrometer is used to produce about 2000 spectral channels with a resolving power of 1200. AIRS Level 1B version 5 (latest) http://disc.sci.gsfc.nasa.gov/AIRS/ Simultaneous Nadir Overpasses (SNOs) identify where satellite nadir ground tracks cross. The solid blue and red lines in the lower left figure show the nadir ground tracks. The blue circles show the swath of the AIRS sensor (90 FOVs per scan line) The red circles show the TANSO FTS fields of view (5 FOVs per scan line at that time) The black circle includes the TANSO FTS and AIRS footprints near the SNO point. A single GOSAT TIR radiance is used along with the four closest AIRS FOVs. The time difference between the GOSAT and AIRS is limited to < 1 hour. The mean and standard deviation of the AIRS FOVs is computed for each AIRS spectral channel. The standard deviation is used as a test for scene uniformity The GOSAT TIR spectrum is convolved with the AIRS spectral response functions (SRFs) to match the spectral resolution of the AIRS sensor. A quality check is made on the imaginary part of the GOSAT TIR spectrum to confirm the GOSAT calibration has removed the complex phase properly. Observed Brightness Temperature (K) A mean of all SNO cases from April 2009 through May 2014 was used to calculate a mean brightness temperature comparison and a spectral bias of the mean difference. The primary problems appear to be a cold bias in the 15 micron and 7 micron regions in JAXA version 161. This bias is expected to be significantly reduced in JAXA version 200+. Radiometric cold bias is apparent in 15 micron band CO2 and in 7 micron CH4 bands. GOSAT/AQUA SNOs Location (+- 40 deg Latitude) A time series analysis of the GOSAT/AIRS SNOs shows a highly stable biasfrom April 2009 through May 2014. This indicates very good stability for the TANSO FTS instrument. The step changes in bias in June 2014 andin 2015are due to loss of satellite solar power causing the TANSO FTS to undergo a cold soaking. After returning to service the TIR detectors were found to have a change in responsivity. This anomaly hasbeen corrected in JAXA ground processing version 200+. Jan2009 Jan2010 Jan2011 Jan2012 Jan2013 Jan2014 Jan2015 GOSAT - AIRS BT (K) -2 -1 0 1 2 Five Year Timeseries of GOSAT - AIRS at Four Levels 689cm-1 smoothed 689cm-1 Jan2010 Jan2011 Jan2012 Jan2013 Jan2014 GOSAT - AIRS BT (K) -2 -1 0 1 2 735cm-1 smoothed 735cm-1 Jan2010 Jan2011 Jan2012 Jan2013 Jan2014 GOSAT - AIRS BT (K) -8 -6 -4 -2 0 2 4 6 8 880cm-1 smoothed 880cm-1 Jan2010 Jan2011 Jan2012 Jan2013 Jan2014 GOSAT - AIRS BT (K) -8 -6 -4 -2 0 2 4 6 8 1150cm-1 smoothed 1150cm-1 Longitude (deg) -100 -95 -90 -85 -80 -75 Latitude (deg) 30 35 40 45 50 55 GOSAT_AIRS_SNO_20090406T190613 600 700 800 900 1000 1100 1200 1300 1400 1500 1600 Radiance (RU) 0 50 100 150 GOSAT_AIRS_SNO_20090406T190613 GOSAT (Real) GOSAT (Imag) AIRS Mean Wavenumber (cm -1 ) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600 Radiance (RU) 0 5 10 15 20 25 30 AIRS Std Dev (4 FOVs) Time series show very stable bias from April 2009 through May 2014 (Five Years) Time Series of SNO bias at 14.5 microns 600 700 800 900 1000 1100 1200 1300 1400 1500 1600 B.T. (K) 200 250 300 Mean GOSAT Mean AIRS Wavenumber (cm -1 ) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600 B.T. (K) -2 -1 0 1 2 Mean GOSAT-AIRS Bias (863 cases) Wavenumber (cm -1 ) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600 B.T. (K) 0 1 2 3 Std. Dev. GOSAT-AIRS (863 cases) CO 2 Band
Transcript
Page 1: Simultaneous Nadir Overpass (SNO) Matchups GOSAT ......Intro The Greenhouse Gases Observing Satellite (GOSAT) was launched in January 2009, to monitor global atmospheric concentration

Results

Simultaneous Nadir Overpass (SNO) Matchups GOSAT/TANSO-FTS and AQUA/AIRS: TIR Band April 2009 – December 2015

Robert Knuteson1, G. Burgess1, K. Shiomi2, A. Kuze2, J. Yoshida3, F. Kataoka 4, and H. Suto 2

1Space, Science, and Engineering Center, University of Wisconsin – Madison, 2Japan Aerospace Exploration Agency, Tsukuba-city, Ibaraki, Japan,3NEC Cooperation, Fuchu, Tokyo, Japan, 4Remote Sensing Technology Center of Japan, Tsukuba-city, Ibaraki, Japan

IntroThe Greenhouse Gases Observing Satellite (GOSAT) was launched in January 2009, to monitor global atmospheric concentration and flux of CO2 and CH4 from space. The TANSO-FTS sensor is an interferometer spectrometer measuring shortwave reflected solar radiation with high spectral resolution in three spectral bands. A bore-sighted band 4 uses the same interferometer to measure thermal infrared radiation (TIR) at the top of the atmosphere. This paper is a comparison of the TANSO-FTS TIR band with coincident measurements of the NASA Atmospheric InfraRed Sounder (AIRS) grating spectrometer. The time and space coincident matchups are at the Simultaneous Nadir Overpass (SNO) locations of the orbits of GOSAT and the NASA AQUA satellite. GOSAT/AQUA SNOs occur at about 40N and 40S latitude. A continuous set of SNO matchups has been found from the start of valid radiance data collection in April 2009 through the end of 2015. UW-SSEC has obtained the time, latitude, and longitude of the SNO location using the ORBNAV software at http://sips.ssec.wisc.edu/orbnav. UW-SSEC obtained the matching AIRS v5 L1B radiances from the NASA archive. JAXA has reprocessed the entire TANSO-FTS TIR band using the previous v161.161 and a new calibration version which includes parameter optimizations. The TANSO-FTS has been reduced to the AIRS spectral channels using the AIRS spectral response functions (SRFs). This paper will show the time series of observed brightnesstemperatures from AIRS and GOSAT TANSO-FTS TIR observations from the SNO matchups. This poster illustrates the satellite inter-calibration data used to validate the improvements in the GOSAT ground calibration software by providing an independent reference to the AIRS on-orbit calibration accuracy. Improvements in the ground calibration software are expected to lead to improvements in the TIR band Level2 retrievals of CO2 profiles

Contact: [email protected] UW-Madison SSEC

References• Kuz e, A., Suto, H., Sh iomi , K., Urabe, T ., Nak aj ima, M., Yos hida, J., ... & Bui js , H. (2012). Lev el 1 a lgorithms for TANSO on GOSAT: processing and on-orbi t

ca l ibrations . Atmos . Meas. Tech, 5(10), 2447-2467.• Kuz e, A., SUto, H., Shiomi , K., Nakaj ima, M., & Bui js , H. (2013, June). Ex perience gained from GOSAT: FTS appl ication for wide s pectral range

obs erv ation. In Fourier Trans form Spectros copy (pp. FW3D-3). Optica l Society o f America.• Kuz e, A., Suto, H., Sh iomi , K., & Nak aj ima, M. (2011, Ju ly). Less ons learned from GOSAT and improvements for the next miss ion. In Fourier Transform

Spectros copy (p. JMA3). Optica l Society o f America.• Kataok a, F ., Knuteson, R. O., Kuze, A., Suto, H., Sh iomi , K., Harada, M., ... & Rev ercomb, H. E. (2014). T IR s pectra l radiance calibration of the GOSAT

s ate l l i te borne TANSO-FTS wi th the ai rcraft-bas ed S-HIS and the ground-based S-AERI at the Rai lroad Val ley desert play a. Geos cience and Remote Sens ing, IEEE Transactions on, 52 (1), 89-105.

• Gero, P. J ., Knuteson, R. O., Shiomi , K., Kuz e, A., Kataoka, F ., Revercomb, H. E., ... & Best, F. A. (2014, November). GOSAT TANSO FTS TIR band cal ibration: a five year review. In SPIE Asia Paci fic Remote Sensing (pp. 926316-926316). In ternational Society for Optics and Photonics.

Acknowledgments This work was supported by JAXA through a task order with UW-SSEC.

Summary• The SNO method is used to make a direct assessment of the absolute

calibration and stability of the GOSAT TIR spectra.• The NASA AIRS sensor is used as a reference of comparison due to

it’s well established calibration accuracy and stability.• The GOSAT TIR radiance was reprocessed at the Aqua/GOSAT SNOs

location for the time period April 2009 – December 2015 using JAXA ground processing version 161.

• The version 161 is seen to exhibit a calibration cold bias at several points in the infrared spectrum including the 15 micron CO2 band.

• A time series analysis shows that the bias is stable from April 2009 through May 2014 when it undergoes a step change to a colder bias.

• The root cause of this bias and the step changes have been addressed in JAXA ground processing version 200+.

• Future work includes validation of v200+ with AIRS & IASI SNOs.

Method DataGOSAT TIRGOSAT radiances are from v161 provided by JAXA after consistent reprocessing. TIR radiances were provided only at SNO locations.AIRS SounderThe orbit of the Aqua satellite is polar sun-synchronous with a nominal altitude of 705 kilometers (438 miles) and an orbital period of 98.8 minutes, completing approximately 14.5 orbits per day. The satellite equatorial crossing local times are 1:30 a.m. in a descending orbit, and 1:30 p.m. in an ascending orbit. A grating spectrometer is used to produce about 2000 spectral channels with a resolving power of 1200.AIRS Level 1B version 5 (latest) http://disc.sci.gsfc.nasa.gov/AIRS/

• Simultaneous Nadir Overpasses (SNOs) identify where satellite nadir ground tracks cross. The solid blue and red lines in the lower left figure show the nadir ground tracks. The blue circles show the swath of the AIRS sensor (90 FOVs per scan line) The red circles show the TANSO FTS fields of view (5 FOVs per scan line at that time) The black circle includes the TANSO FTS and AIRS footprints near the SNO point. A single GOSAT TIR radiance is used along with the four closest AIRS FOVs. The time difference between the GOSAT and AIRS is limited to < 1 hour.

• The mean and standard deviation of the AIRS FOVs is computed for each AIRS spectral channel. The standard deviation is used as a test for scene uniformity

• The GOSAT TIR spectrum is convolved with the AIRS spectral response functions (SRFs) to match the spectral resolution of the AIRS sensor. A quality check is made on the imaginary part of the GOSAT TIR spectrum to confirm the GOSAT calibration has removed the complex phase properly.

Obs

erve

d Br

ightn

ess

Tem

pera

ture

(K)A mean of all SNO cases

from April 2009 through May2014 was used to calculate amean brightness temperaturecomparison and a spectralbias of the mean difference.The primary problems appearto be a cold bias in the 15micron and 7 micron regionsin JAXA version 161. Thisbias is expected to besignificantly reduced inJAXA version 200+.

Radiometric cold bias is apparent in 15 micron band CO2 and in 7 micron CH4 bands.

GOSAT/AQUA SNOs Location (+- 40 degLatitude)

A time series analysis of theGOSAT/AIRS SNOs shows a highlystable bias from April 2009 throughMay 2014. This indicates very goodstability for the TANSO FTSinstrument. The step changes in biasin June 2014 and in 2015 are due toloss of satellite solar power causingthe TANSO FTS to undergo a coldsoaking. After returning to servicethe TIR detectors were found to havea change in responsivity. Thisanomaly hasbeen corrected in JAXAground processing version 200+.

Jan2009 Jan2010 Jan2011 Jan2012 Jan2013 Jan2014 Jan2015

GO

SAT

- AIR

S BT

(K)

-2

-1

0

1

2 Five Year Timeseries of GOSAT - AIRS at Four Levels

689cm-1smoothed 689cm-1

Jan2010 Jan2011 Jan2012 Jan2013 Jan2014

GO

SAT

- AIR

S BT

(K)

-2

-1

0

1

2735cm-1smoothed 735cm-1

Jan2010 Jan2011 Jan2012 Jan2013 Jan2014

GO

SAT

- AIR

S BT

(K)

-8-6-4-202468

880cm-1smoothed 880cm-1

Jan2010 Jan2011 Jan2012 Jan2013 Jan2014G

OSA

T - A

IRS

BT (K

)-8-6-4-202468

1150cm-1smoothed 1150cm-1

Longitude (deg) -100 -95 -90 -85 -80 -75

Latit

ude

(deg

)

30

35

40

45

50

55GOSAT_AIRS_SNO_20090406T190613

600 700 800 900 1000 1100 1200 1300 1400 1500 1600

Radi

ance

(RU)

0

50

100

150GOSAT_AIRS_SNO_20090406T190613

GOSAT (Real)GOSAT (Imag)AIRS Mean

Wavenumber (cm-1) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600

Radi

ance

(RU)

0

5

10

15

20

25

30AIRS Std Dev (4 FOVs)

Time series show very stable bias from April 2009 through May 2014 (Five Years)

Time Series of SNO bias at 14.5 microns

600 700 800 900 1000 1100 1200 1300 1400 1500 1600

B.T.

(K)

200

250

300Mean GOSATMean AIRS

Wavenumber (cm-1) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600

B.T.

(K)

-2

-1

0

1

2Mean GOSAT-AIRS Bias (863 cases)

Wavenumber (cm-1) 600 700 800 900 1000 1100 1200 1300 1400 1500 1600

B.T.

(K)

0

1

2

3Std. Dev. GOSAT-AIRS (863 cases)

CO2 Band

Recommended