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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Bibliographic Details
Main Authors: Viola, Donna, McEwen, Alfred S.
Format: Dataset
Language:unknown
Published: Zenodo 2018
Subjects:
Thermokarst
Online Access:https://dx.doi.org/10.5281/zenodo.1117102
https://zenodo.org/record/1117102
id ftdatacite:10.5281/zenodo.1117102
record_format openpolar
spelling ftdatacite:10.5281/zenodo.1117102 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.1117102 https://zenodo.org/record/1117102 unknown Zenodo https://dx.doi.org/10.5281/zenodo.1117101 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.1117102 https://doi.org/10.5281/zenodo.1117101 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)
institution 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.1117102
https://zenodo.org/record/1117102
genre Thermokarst
genre_facet Thermokarst
op_relation https://dx.doi.org/10.5281/zenodo.1117101
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.1117102
https://doi.org/10.5281/zenodo.1117101
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