IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC)
The surface of Mars has been an object of interest for planetary research since the launch of Mariner 4 in 1964. Since then different cameras such as the Viking Visual Imaging Subsystem (VIS), Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC), and Mars Reconnaissance Orbiter (MRO) Context Camera...
Published in: | The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences |
---|---|
Main Authors: | , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Copernicus Publications
2016
|
Subjects: | |
Online Access: | https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 https://noa.gwlb.de/receive/cop_mods_00012487 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00012443/isprs-archives-XLI-B4-463-2016.pdf https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLI-B4/463/2016/isprs-archives-XLI-B4-463-2016.pdf |
id |
ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00012487 |
---|---|
record_format |
openpolar |
spelling |
ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00012487 2023-05-15T18:23:22+02:00 IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) Putri, Alfiah Rizky Diana Sidiropoulos, Panagiotis Muller, Jan-Peter 2016-06 electronic https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 https://noa.gwlb.de/receive/cop_mods_00012487 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00012443/isprs-archives-XLI-B4-463-2016.pdf https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLI-B4/463/2016/isprs-archives-XLI-B4-463-2016.pdf eng eng Copernicus Publications ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences -- http://www.isprs.org/publications/archives.aspx -- 2194-9034 https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 https://noa.gwlb.de/receive/cop_mods_00012487 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00012443/isprs-archives-XLI-B4-463-2016.pdf https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLI-B4/463/2016/isprs-archives-XLI-B4-463-2016.pdf uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2016 ftnonlinearchiv https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 2022-02-08T22:56:05Z The surface of Mars has been an object of interest for planetary research since the launch of Mariner 4 in 1964. Since then different cameras such as the Viking Visual Imaging Subsystem (VIS), Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC), and Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and High Resolution Imaging Science Experiment (HiRISE) have been imaging its surface at ever higher resolution. The High Resolution Stereo Camera (HRSC) on board of the European Space Agency (ESA) Mars Express, has been imaging the Martian surface, since 25th December 2003 until the present-day. HRSC has covered 100 % of the surface of Mars, about 70 % of the surface with panchromatic images at 10-20 m/pixel, and about 98 % at better than 100 m/pixel (Neukum et. al., 2004), including the polar regions of Mars. The Mars polar regions have been studied intensively recently by analysing images taken by the Mars Express and MRO missions (Plaut et al., 2007). The South Polar Residual Cap (SPRC) does not change very much in volume overall but there are numerous examples of dynamic phenomena associated with seasonal changes in the atmosphere. In particular, we can examine the time variation of layers of solid carbon dioxide and water ice with dust deposition (Bibring, 2004), spider-like channels (Piqueux et al., 2003) and so-called Swiss Cheese Terrain (Titus et al., 2004). Because of seasonal changes each Martian year, due to the sublimation and deposition of water and CO2 ice on the Martian south polar region, clearly identifiable surface changes occur in otherwise permanently icy region. In this research, good quality HRSC images of the Mars South Polar region are processed based on previous identification as the optimal coverage of clear surfaces (Campbell et al., 2015). HRSC images of the Martian South Pole are categorized in terms of quality, time, and location to find overlapping areas, processed into high quality Digital Terrain Models (DTMs) and Orthorectified Images (ORIs) and projected into polar stereographic projection using DLR (Deutsches Zentrum für Luft- und Raumfahrt; German Aerospace Center)’s VICAR and GIS software with modifications developed by Kim & Muller (2009). Surface changes are identified in the Mars SPRC region and analysed based on their appearance in the HRSC images. Article in Journal/Newspaper South pole Niedersächsisches Online-Archiv NOA South Pole Titus ENVELOPE(169.033,169.033,-72.250,-72.250) The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLI-B4 463 469 |
institution |
Open Polar |
collection |
Niedersächsisches Online-Archiv NOA |
op_collection_id |
ftnonlinearchiv |
language |
English |
topic |
article Verlagsveröffentlichung |
spellingShingle |
article Verlagsveröffentlichung Putri, Alfiah Rizky Diana Sidiropoulos, Panagiotis Muller, Jan-Peter IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
topic_facet |
article Verlagsveröffentlichung |
description |
The surface of Mars has been an object of interest for planetary research since the launch of Mariner 4 in 1964. Since then different cameras such as the Viking Visual Imaging Subsystem (VIS), Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC), and Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and High Resolution Imaging Science Experiment (HiRISE) have been imaging its surface at ever higher resolution. The High Resolution Stereo Camera (HRSC) on board of the European Space Agency (ESA) Mars Express, has been imaging the Martian surface, since 25th December 2003 until the present-day. HRSC has covered 100 % of the surface of Mars, about 70 % of the surface with panchromatic images at 10-20 m/pixel, and about 98 % at better than 100 m/pixel (Neukum et. al., 2004), including the polar regions of Mars. The Mars polar regions have been studied intensively recently by analysing images taken by the Mars Express and MRO missions (Plaut et al., 2007). The South Polar Residual Cap (SPRC) does not change very much in volume overall but there are numerous examples of dynamic phenomena associated with seasonal changes in the atmosphere. In particular, we can examine the time variation of layers of solid carbon dioxide and water ice with dust deposition (Bibring, 2004), spider-like channels (Piqueux et al., 2003) and so-called Swiss Cheese Terrain (Titus et al., 2004). Because of seasonal changes each Martian year, due to the sublimation and deposition of water and CO2 ice on the Martian south polar region, clearly identifiable surface changes occur in otherwise permanently icy region. In this research, good quality HRSC images of the Mars South Polar region are processed based on previous identification as the optimal coverage of clear surfaces (Campbell et al., 2015). HRSC images of the Martian South Pole are categorized in terms of quality, time, and location to find overlapping areas, processed into high quality Digital Terrain Models (DTMs) and Orthorectified Images (ORIs) and projected into polar stereographic projection using DLR (Deutsches Zentrum für Luft- und Raumfahrt; German Aerospace Center)’s VICAR and GIS software with modifications developed by Kim & Muller (2009). Surface changes are identified in the Mars SPRC region and analysed based on their appearance in the HRSC images. |
format |
Article in Journal/Newspaper |
author |
Putri, Alfiah Rizky Diana Sidiropoulos, Panagiotis Muller, Jan-Peter |
author_facet |
Putri, Alfiah Rizky Diana Sidiropoulos, Panagiotis Muller, Jan-Peter |
author_sort |
Putri, Alfiah Rizky Diana |
title |
IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
title_short |
IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
title_full |
IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
title_fullStr |
IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
title_full_unstemmed |
IDENTIFYING SURFACE CHANGES ON HRSC IMAGES OF THE MARS SOUTH POLAR RESIDUAL CAP (SPRC) |
title_sort |
identifying surface changes on hrsc images of the mars south polar residual cap (sprc) |
publisher |
Copernicus Publications |
publishDate |
2016 |
url |
https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 https://noa.gwlb.de/receive/cop_mods_00012487 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00012443/isprs-archives-XLI-B4-463-2016.pdf https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLI-B4/463/2016/isprs-archives-XLI-B4-463-2016.pdf |
long_lat |
ENVELOPE(169.033,169.033,-72.250,-72.250) |
geographic |
South Pole Titus |
geographic_facet |
South Pole Titus |
genre |
South pole |
genre_facet |
South pole |
op_relation |
ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences -- http://www.isprs.org/publications/archives.aspx -- 2194-9034 https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 https://noa.gwlb.de/receive/cop_mods_00012487 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00012443/isprs-archives-XLI-B4-463-2016.pdf https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLI-B4/463/2016/isprs-archives-XLI-B4-463-2016.pdf |
op_rights |
uneingeschränkt info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.5194/isprs-archives-XLI-B4-463-2016 |
container_title |
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences |
container_volume |
XLI-B4 |
container_start_page |
463 |
op_container_end_page |
469 |
_version_ |
1766202947629219840 |