CryoSat Ice Baseline-D validation and evolutions

The ESA Earth Explorer CryoSat-2 was launched on 8 April 2010 to monitor the precise changes in the thickness of terrestrial ice sheets and marine floating ice. To do that, CryoSat orbits the planet at an altitude of around 720 km with a retrograde orbit inclination of 92 ∘ and a quasi repeat cycle...

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Published in:The Cryosphere
Main Authors: Meloni, Marco, Bouffard, Jerome, Parrinello, Tommaso, Dawson, Geoffrey, Garnier, Florent, Helm, Veit, Bella, Alessandro, Hendricks, Stefan, Ricker, Robert, Webb, Erica, Wright, Ben, Nielsen, Karina, Lee, Sanggyun, Passaro, Marcello, Scagliola, Michele, Simonsen, Sebastian Bjerregaard, Sandberg Sørensen, Louise, Brockley, David, Baker, Steven, Fleury, Sara, Bamber, Jonathan, Maestri, Luca, Skourup, Henriette, Forsberg, René, Mizzi, Loretta
Format: Text
Language:English
Published: 2020
Subjects:
Online Access:https://doi.org/10.5194/tc-14-1889-2020
https://tc.copernicus.org/articles/14/1889/2020/
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spelling ftcopernicus:oai:publications.copernicus.org:tc81227 2023-05-15T15:33:56+02:00 CryoSat Ice Baseline-D validation and evolutions Meloni, Marco Bouffard, Jerome Parrinello, Tommaso Dawson, Geoffrey Garnier, Florent Helm, Veit Bella, Alessandro Hendricks, Stefan Ricker, Robert Webb, Erica Wright, Ben Nielsen, Karina Lee, Sanggyun Passaro, Marcello Scagliola, Michele Simonsen, Sebastian Bjerregaard Sandberg Sørensen, Louise Brockley, David Baker, Steven Fleury, Sara Bamber, Jonathan Maestri, Luca Skourup, Henriette Forsberg, René Mizzi, Loretta 2020-06-12 application/pdf https://doi.org/10.5194/tc-14-1889-2020 https://tc.copernicus.org/articles/14/1889/2020/ eng eng doi:10.5194/tc-14-1889-2020 https://tc.copernicus.org/articles/14/1889/2020/ eISSN: 1994-0424 Text 2020 ftcopernicus https://doi.org/10.5194/tc-14-1889-2020 2020-07-20T16:22:06Z The ESA Earth Explorer CryoSat-2 was launched on 8 April 2010 to monitor the precise changes in the thickness of terrestrial ice sheets and marine floating ice. To do that, CryoSat orbits the planet at an altitude of around 720 km with a retrograde orbit inclination of 92 ∘ and a quasi repeat cycle of 369 d (30 d subcycle). To reach the mission goals, the CryoSat products have to meet the highest quality standards to date, achieved through continual improvements of the operational processing chains. The new CryoSat Ice Baseline-D, in operation since 27 May 2019, represents a major processor upgrade with respect to the previous Ice Baseline-C. Over land ice the new Baseline-D provides better results with respect to the previous baseline when comparing the data to a reference elevation model over the Austfonna ice cap region, improving the ascending and descending crossover statistics from 1.9 to 0.1 m. The improved processing of the star tracker measurements implemented in Baseline-D has led to a reduction in the standard deviation of the point-to-point comparison with the previous star tracker processing method implemented in Baseline-C from 3.8 to 3.7 m. Over sea ice, Baseline-D improves the quality of the retrieved heights inside and at the boundaries of the synthetic aperture radar interferometric (SARIn or SIN) acquisition mask, removing the negative freeboard pattern which is beneficial not only for freeboard retrieval but also for any application that exploits the phase information from SARIn Level 1B (L1B) products. In addition, scatter comparisons with the Beaufort Gyre Exploration Project (BGEP; https://www.whoi.edu/beaufortgyre , last access: October 2019) and Operation IceBridge (OIB; Kurtz et al., 2013) in situ measurements confirm the improvements in the Baseline-D freeboard product quality. Relative to OIB, the Baseline-D freeboard mean bias is reduced by about 8 cm, which roughly corresponds to a 60 % decrease with respect to Baseline-C. The BGEP data indicate a similar tendency with a mean draft bias lowered from 0.85 to − 0.14 m. For the two in situ datasets, the root mean square deviation (RMSD) is also well reduced from 14 to 11 cm for OIB and by a factor of 2 for the BGEP. Observations over inland waters show a slight increase in the percentage of good observations in Baseline-D, generally around 5 %–10 % for most lakes. This paper provides an overview of the new Level 1 and Level 2 (L2) CryoSat Ice Baseline-D evolutions and related data quality assessment, based on results obtained from analyzing the 6-month Baseline-D test dataset released to CryoSat expert users prior to the final transfer to operations. Text Austfonna Ice cap Sea ice Copernicus Publications: E-Journals Austfonna ENVELOPE(24.559,24.559,79.835,79.835) The Cryosphere 14 6 1889 1907
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The ESA Earth Explorer CryoSat-2 was launched on 8 April 2010 to monitor the precise changes in the thickness of terrestrial ice sheets and marine floating ice. To do that, CryoSat orbits the planet at an altitude of around 720 km with a retrograde orbit inclination of 92 ∘ and a quasi repeat cycle of 369 d (30 d subcycle). To reach the mission goals, the CryoSat products have to meet the highest quality standards to date, achieved through continual improvements of the operational processing chains. The new CryoSat Ice Baseline-D, in operation since 27 May 2019, represents a major processor upgrade with respect to the previous Ice Baseline-C. Over land ice the new Baseline-D provides better results with respect to the previous baseline when comparing the data to a reference elevation model over the Austfonna ice cap region, improving the ascending and descending crossover statistics from 1.9 to 0.1 m. The improved processing of the star tracker measurements implemented in Baseline-D has led to a reduction in the standard deviation of the point-to-point comparison with the previous star tracker processing method implemented in Baseline-C from 3.8 to 3.7 m. Over sea ice, Baseline-D improves the quality of the retrieved heights inside and at the boundaries of the synthetic aperture radar interferometric (SARIn or SIN) acquisition mask, removing the negative freeboard pattern which is beneficial not only for freeboard retrieval but also for any application that exploits the phase information from SARIn Level 1B (L1B) products. In addition, scatter comparisons with the Beaufort Gyre Exploration Project (BGEP; https://www.whoi.edu/beaufortgyre , last access: October 2019) and Operation IceBridge (OIB; Kurtz et al., 2013) in situ measurements confirm the improvements in the Baseline-D freeboard product quality. Relative to OIB, the Baseline-D freeboard mean bias is reduced by about 8 cm, which roughly corresponds to a 60 % decrease with respect to Baseline-C. The BGEP data indicate a similar tendency with a mean draft bias lowered from 0.85 to − 0.14 m. For the two in situ datasets, the root mean square deviation (RMSD) is also well reduced from 14 to 11 cm for OIB and by a factor of 2 for the BGEP. Observations over inland waters show a slight increase in the percentage of good observations in Baseline-D, generally around 5 %–10 % for most lakes. This paper provides an overview of the new Level 1 and Level 2 (L2) CryoSat Ice Baseline-D evolutions and related data quality assessment, based on results obtained from analyzing the 6-month Baseline-D test dataset released to CryoSat expert users prior to the final transfer to operations.
format Text
author Meloni, Marco
Bouffard, Jerome
Parrinello, Tommaso
Dawson, Geoffrey
Garnier, Florent
Helm, Veit
Bella, Alessandro
Hendricks, Stefan
Ricker, Robert
Webb, Erica
Wright, Ben
Nielsen, Karina
Lee, Sanggyun
Passaro, Marcello
Scagliola, Michele
Simonsen, Sebastian Bjerregaard
Sandberg Sørensen, Louise
Brockley, David
Baker, Steven
Fleury, Sara
Bamber, Jonathan
Maestri, Luca
Skourup, Henriette
Forsberg, René
Mizzi, Loretta
spellingShingle Meloni, Marco
Bouffard, Jerome
Parrinello, Tommaso
Dawson, Geoffrey
Garnier, Florent
Helm, Veit
Bella, Alessandro
Hendricks, Stefan
Ricker, Robert
Webb, Erica
Wright, Ben
Nielsen, Karina
Lee, Sanggyun
Passaro, Marcello
Scagliola, Michele
Simonsen, Sebastian Bjerregaard
Sandberg Sørensen, Louise
Brockley, David
Baker, Steven
Fleury, Sara
Bamber, Jonathan
Maestri, Luca
Skourup, Henriette
Forsberg, René
Mizzi, Loretta
CryoSat Ice Baseline-D validation and evolutions
author_facet Meloni, Marco
Bouffard, Jerome
Parrinello, Tommaso
Dawson, Geoffrey
Garnier, Florent
Helm, Veit
Bella, Alessandro
Hendricks, Stefan
Ricker, Robert
Webb, Erica
Wright, Ben
Nielsen, Karina
Lee, Sanggyun
Passaro, Marcello
Scagliola, Michele
Simonsen, Sebastian Bjerregaard
Sandberg Sørensen, Louise
Brockley, David
Baker, Steven
Fleury, Sara
Bamber, Jonathan
Maestri, Luca
Skourup, Henriette
Forsberg, René
Mizzi, Loretta
author_sort Meloni, Marco
title CryoSat Ice Baseline-D validation and evolutions
title_short CryoSat Ice Baseline-D validation and evolutions
title_full CryoSat Ice Baseline-D validation and evolutions
title_fullStr CryoSat Ice Baseline-D validation and evolutions
title_full_unstemmed CryoSat Ice Baseline-D validation and evolutions
title_sort cryosat ice baseline-d validation and evolutions
publishDate 2020
url https://doi.org/10.5194/tc-14-1889-2020
https://tc.copernicus.org/articles/14/1889/2020/
long_lat ENVELOPE(24.559,24.559,79.835,79.835)
geographic Austfonna
geographic_facet Austfonna
genre Austfonna
Ice cap
Sea ice
genre_facet Austfonna
Ice cap
Sea ice
op_source eISSN: 1994-0424
op_relation doi:10.5194/tc-14-1889-2020
https://tc.copernicus.org/articles/14/1889/2020/
op_doi https://doi.org/10.5194/tc-14-1889-2020
container_title The Cryosphere
container_volume 14
container_issue 6
container_start_page 1889
op_container_end_page 1907
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