Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes
This data supplements the results presented in Viola & McEwen (2018), Journal of Geophysical Research: Planets, doi:10.1002/2017JE005366. The GIS databases presented here describe the presence of thermokarstic features (expanded craters and scalloped depressions) and pedestal craters found in im...
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ftdatacite:10.5281/zenodo.1117101 2023-05-15T18:32:57+02:00 Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes Viola, Donna McEwen, Alfred S. 2018 https://dx.doi.org/10.5281/zenodo.1117101 https://zenodo.org/record/1117101 unknown Zenodo https://dx.doi.org/10.5281/zenodo.1117102 Open Access Creative Commons Attribution 4.0 https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess CC-BY dataset Dataset 2018 ftdatacite https://doi.org/10.5281/zenodo.1117101 https://doi.org/10.5281/zenodo.1117102 2021-11-05T12:55:41Z This data supplements the results presented in Viola & McEwen (2018), Journal of Geophysical Research: Planets, doi:10.1002/2017JE005366. The GIS databases presented here describe the presence of thermokarstic features (expanded craters and scalloped depressions) and pedestal craters found in images from the High Resolution Imaging Science Experiment (HiRISE) on the Mars Reconnaissance Orbiter (MRO) within two study regions: southern Arcadia Planitia (25–40°N, 180–240°E) and the southern mid-latitude band (30–60°S). These features suggest the presence of near-surface excess ice on Mars. Dataset Thermokarst DataCite Metadata Store (German National Library of Science and Technology) |
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Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
description |
This data supplements the results presented in Viola & McEwen (2018), Journal of Geophysical Research: Planets, doi:10.1002/2017JE005366. The GIS databases presented here describe the presence of thermokarstic features (expanded craters and scalloped depressions) and pedestal craters found in images from the High Resolution Imaging Science Experiment (HiRISE) on the Mars Reconnaissance Orbiter (MRO) within two study regions: southern Arcadia Planitia (25–40°N, 180–240°E) and the southern mid-latitude band (30–60°S). These features suggest the presence of near-surface excess ice on Mars. |
format |
Dataset |
author |
Viola, Donna McEwen, Alfred S. |
spellingShingle |
Viola, Donna McEwen, Alfred S. Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
author_facet |
Viola, Donna McEwen, Alfred S. |
author_sort |
Viola, Donna |
title |
Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
title_short |
Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
title_full |
Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
title_fullStr |
Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
title_full_unstemmed |
Martian Thermokarst: South Arcadia Planitia And The Southern Mid-Latitudes |
title_sort |
martian thermokarst: south arcadia planitia and the southern mid-latitudes |
publisher |
Zenodo |
publishDate |
2018 |
url |
https://dx.doi.org/10.5281/zenodo.1117101 https://zenodo.org/record/1117101 |
genre |
Thermokarst |
genre_facet |
Thermokarst |
op_relation |
https://dx.doi.org/10.5281/zenodo.1117102 |
op_rights |
Open Access Creative Commons Attribution 4.0 https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.1117101 https://doi.org/10.5281/zenodo.1117102 |
_version_ |
1766217170876891136 |