Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia

We compare AIRS, IASI-A and CrIS under the cold conditions encountered in the daily overpasses of Dome Concordia, which is located on a high plateau in Antarctica, between May 2012 and March 2016. The brightness temperatures at DomeC for the 900 cm-1 atmospheric window channel is 218K on average, bu...

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Main Authors: Aumann, H.H., Elliott, Denis
Format: Conference Object
Language:English
Published: Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2016 2019
Subjects:
Online Access:http://hdl.handle.net/2014/45986
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spelling ftnasajpl:oai:trs.jpl.nasa.gov:2014/45986 2023-05-15T13:46:47+02:00 Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia Aumann, H.H. Elliott, Denis 2019-03-29T17:38:01Z application/pdf http://hdl.handle.net/2014/45986 en_US eng Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2016 SPIE Optics and Photonics, San Diego, California, August 28 - September 1, 2016 16-3055 http://hdl.handle.net/2014/45986 Presentation 2019 ftnasajpl 2021-12-23T13:15:26Z We compare AIRS, IASI-A and CrIS under the cold conditions encountered in the daily overpasses of Dome Concordia, which is located on a high plateau in Antarctica, between May 2012 and March 2016. The brightness temperatures at DomeC for the 900 cm-1 atmospheric window channel is 218K on average, but varies seasonally from 185K to 255K. Averaged over all simultaneous overpass data AIRS is 26±13 mK warmer than IASI-A, AIRS is 116±7 mK colder than CrIS. However, we find that differences for both AIRS/IASI-A and AIRS/CrIS are temperature dependent, with AIRS being 250mK colder than IASI-A at 200K. These effects have been independently verified by other investigators. AIRS and CrIS bt900 results for simultaneous overpasses and daily mean values agree within 100 mK. AIRS and IASI simultaneous overpasses agree within 100 mK, but AIRS is 2K warmer than IASI for daily mean values. We attribute this effect to an overactive IASI QC which is sensitive to scene temperature above about 240K. The DomeC data do not reveal if this QC effect is present at temperatures warmer than 255K. These effects need to be taken into account when comparing results from AIRS, IASI and CrIS, and even more so when analyzing data from vintage instruments with respect to climate change. NASA/JPL Conference Object Antarc* Antarctica Cris JPL Technical Report Server
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language English
description We compare AIRS, IASI-A and CrIS under the cold conditions encountered in the daily overpasses of Dome Concordia, which is located on a high plateau in Antarctica, between May 2012 and March 2016. The brightness temperatures at DomeC for the 900 cm-1 atmospheric window channel is 218K on average, but varies seasonally from 185K to 255K. Averaged over all simultaneous overpass data AIRS is 26±13 mK warmer than IASI-A, AIRS is 116±7 mK colder than CrIS. However, we find that differences for both AIRS/IASI-A and AIRS/CrIS are temperature dependent, with AIRS being 250mK colder than IASI-A at 200K. These effects have been independently verified by other investigators. AIRS and CrIS bt900 results for simultaneous overpasses and daily mean values agree within 100 mK. AIRS and IASI simultaneous overpasses agree within 100 mK, but AIRS is 2K warmer than IASI for daily mean values. We attribute this effect to an overactive IASI QC which is sensitive to scene temperature above about 240K. The DomeC data do not reveal if this QC effect is present at temperatures warmer than 255K. These effects need to be taken into account when comparing results from AIRS, IASI and CrIS, and even more so when analyzing data from vintage instruments with respect to climate change. NASA/JPL
format Conference Object
author Aumann, H.H.
Elliott, Denis
spellingShingle Aumann, H.H.
Elliott, Denis
Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
author_facet Aumann, H.H.
Elliott, Denis
author_sort Aumann, H.H.
title Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
title_short Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
title_full Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
title_fullStr Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
title_full_unstemmed Comparison of the AIRS, IASI, and CrIS 900 cm-1 channel for Dome Concordia
title_sort comparison of the airs, iasi, and cris 900 cm-1 channel for dome concordia
publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2016
publishDate 2019
url http://hdl.handle.net/2014/45986
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Antarctica
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op_relation SPIE Optics and Photonics, San Diego, California, August 28 - September 1, 2016
16-3055
http://hdl.handle.net/2014/45986
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