Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...

The seasonal deposition and sublimation of CO2 constitute a major element in Martian volatile cycles. We reprocess the Mars Orbiter Laser Altimeter (MOLA) data and apply co-registration procedures to obtain spatio-temporal variations in levels of the Seasonal North Polar Cap (SNPC). The maximum leve...

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Main Authors: Xiao, Haifeng, Stark, Alexander, Schmidt, Frédéric, Hao, Jingyan, Steinbrügge, Gregor, Wagner, Nicholas L., Su, Shu, Cheng, Yuan, Oberst, Jürgen
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union (AGU) 2022
Subjects:
Online Access:https://dx.doi.org/10.14279/depositonce-21071
https://depositonce.tu-berlin.de/handle/11303/22270
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author Xiao, Haifeng
Stark, Alexander
Schmidt, Frédéric
Hao, Jingyan
Steinbrügge, Gregor
Wagner, Nicholas L.
Su, Shu
Cheng, Yuan
Oberst, Jürgen
author_facet Xiao, Haifeng
Stark, Alexander
Schmidt, Frédéric
Hao, Jingyan
Steinbrügge, Gregor
Wagner, Nicholas L.
Su, Shu
Cheng, Yuan
Oberst, Jürgen
author_sort Xiao, Haifeng
collection DataCite
description The seasonal deposition and sublimation of CO2 constitute a major element in Martian volatile cycles. We reprocess the Mars Orbiter Laser Altimeter (MOLA) data and apply co-registration procedures to obtain spatio-temporal variations in levels of the Seasonal North Polar Cap (SNPC). The maximum level over the Residual North Polar Cap (RNPC) is 1.3 m, approximately half of that at the south pole (2.5 m). However, the maximum level in the dune fields at Olympia Undae can be up to 3.8 m. Furthermore, off-season decreases up to 3 m during the northern winter at Olympia Undae are observed. These are likely due to metamorphism effects accentuated by the reduced snowfall at this period. Meanwhile, off-season increases of up to 2 m during the northern spring are noted, the cause of which remains to be explored. The volume of the SNPC peaks at the end of northern winter and is estimated to be approximately 9.6 × 1012 m3, which is 2% more than that of the Seasonal South Polar Cap. The bulk density of the SNPC can go ...
format Article in Journal/Newspaper
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op_doi https://doi.org/10.14279/depositonce-21071
op_rights Creative Commons Attribution 4.0 International
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spelling ftdatacite:10.14279/depositonce-21071 2025-01-17T00:52:21+00:00 Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ... Xiao, Haifeng Stark, Alexander Schmidt, Frédéric Hao, Jingyan Steinbrügge, Gregor Wagner, Nicholas L. Su, Shu Cheng, Yuan Oberst, Jürgen 2022 https://dx.doi.org/10.14279/depositonce-21071 https://depositonce.tu-berlin.de/handle/11303/22270 en eng American Geophysical Union (AGU) Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften Mars seasonal polar cap CO2 ice MOLA level variation pseudo cross-over JournalArticle Article ScholarlyArticle article-journal 2022 ftdatacite https://doi.org/10.14279/depositonce-21071 2024-09-02T08:02:13Z The seasonal deposition and sublimation of CO2 constitute a major element in Martian volatile cycles. We reprocess the Mars Orbiter Laser Altimeter (MOLA) data and apply co-registration procedures to obtain spatio-temporal variations in levels of the Seasonal North Polar Cap (SNPC). The maximum level over the Residual North Polar Cap (RNPC) is 1.3 m, approximately half of that at the south pole (2.5 m). However, the maximum level in the dune fields at Olympia Undae can be up to 3.8 m. Furthermore, off-season decreases up to 3 m during the northern winter at Olympia Undae are observed. These are likely due to metamorphism effects accentuated by the reduced snowfall at this period. Meanwhile, off-season increases of up to 2 m during the northern spring are noted, the cause of which remains to be explored. The volume of the SNPC peaks at the end of northern winter and is estimated to be approximately 9.6 × 1012 m3, which is 2% more than that of the Seasonal South Polar Cap. The bulk density of the SNPC can go ... Article in Journal/Newspaper South pole DataCite South Pole
spellingShingle 500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
Mars
seasonal polar cap
CO2 ice
MOLA
level variation
pseudo cross-over
Xiao, Haifeng
Stark, Alexander
Schmidt, Frédéric
Hao, Jingyan
Steinbrügge, Gregor
Wagner, Nicholas L.
Su, Shu
Cheng, Yuan
Oberst, Jürgen
Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title_full Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title_fullStr Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title_full_unstemmed Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title_short Spatio‐Temporal Level Variations of the Martian Seasonal North Polar Cap From Co‐Registration of MOLA Profiles ...
title_sort spatio‐temporal level variations of the martian seasonal north polar cap from co‐registration of mola profiles ...
topic 500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
Mars
seasonal polar cap
CO2 ice
MOLA
level variation
pseudo cross-over
topic_facet 500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
Mars
seasonal polar cap
CO2 ice
MOLA
level variation
pseudo cross-over
url https://dx.doi.org/10.14279/depositonce-21071
https://depositonce.tu-berlin.de/handle/11303/22270