Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars

Overview Multispectral mapping data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) provide a unique opportunity to characterize south polar ice deposits at higher spectral sampling, spatial resolution, or spatiotemporal coverage than previous work. This new perspective can hel...

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Main Author: Cartwright, S. F. A.
Format: Other/Unknown Material
Language:English
Published: Zenodo 2023
Subjects:
ice
Online Access:https://doi.org/10.5281/zenodo.8201616
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spelling ftzenodo:oai:zenodo.org:8201616 2024-09-15T18:36:55+00:00 Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars Cartwright, S. F. A. 2023-08-01 https://doi.org/10.5281/zenodo.8201616 eng eng Zenodo https://doi.org/10.5281/zenodo.6960943 https://doi.org/10.1029/2022JE007372 https://doi.org/10.5281/zenodo.8201615 https://doi.org/10.5281/zenodo.8201616 oai:zenodo.org:8201616 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode Mars polar ice spectroscopy machine learning info:eu-repo/semantics/other 2023 ftzenodo https://doi.org/10.5281/zenodo.820161610.5281/zenodo.696094310.1029/2022JE00737210.5281/zenodo.8201615 2024-07-26T22:27:49Z Overview Multispectral mapping data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) provide a unique opportunity to characterize south polar ice deposits at higher spectral sampling, spatial resolution, or spatiotemporal coverage than previous work. This new perspective can help to constrain the nature and distribution of different mixtures of CO 2 ice, H 2 O ice, and dust that influence the formation, evolution, and preservation of Mars climate records. We processed 1103 CRISM observations spanning southern summer of six Mars Years through a combination of k -means clustering and random forest classification. Using a set of 12 spectral endmembers directly tied to previous work with high-resolution CRISM targeted data, we made a series of temporally restricted mosaics showing surface spectral variation over time.The endmember set and classified mosaics produced in this work can provide critical context for future studies of the dynamic processes that shape south polar ice deposits. This is follow-on work to a previous study that produced a series of classified maps and a spectral library from CRISM targeted data. That work can be accessed with the following links: Publication: https://doi.org/10.1029/2022JE007372 Repository: https://doi.org/10.5281/zenodo.6960943 Contents The repository contains two .zip files, which can be expanded to access the files described below: classified_mosaics.zip lookup_files SP_CRISM_RF_ColorMap.clr : An ESRI-formatted color map file that can be used to apply the endmember color schemeto random forest-classified maps in ArcGIS (see Symbology settings). Note that for continuity with Cartwright (2022), there are 21 colors in this file, though only endmembers associated with 12 of those colors are present in the classified mosaics. SP_CRISM_RF_ColorMap.txt : A text file that can be loaded into Python as a numpy array and used to generate a matplotlib color ramp. Row indices correspond to endmember numbers (see below) and columns are red, green, and blue values ... Other/Unknown Material South pole Zenodo
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language English
topic Mars
polar
ice
spectroscopy
machine learning
spellingShingle Mars
polar
ice
spectroscopy
machine learning
Cartwright, S. F. A.
Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
topic_facet Mars
polar
ice
spectroscopy
machine learning
description Overview Multispectral mapping data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) provide a unique opportunity to characterize south polar ice deposits at higher spectral sampling, spatial resolution, or spatiotemporal coverage than previous work. This new perspective can help to constrain the nature and distribution of different mixtures of CO 2 ice, H 2 O ice, and dust that influence the formation, evolution, and preservation of Mars climate records. We processed 1103 CRISM observations spanning southern summer of six Mars Years through a combination of k -means clustering and random forest classification. Using a set of 12 spectral endmembers directly tied to previous work with high-resolution CRISM targeted data, we made a series of temporally restricted mosaics showing surface spectral variation over time.The endmember set and classified mosaics produced in this work can provide critical context for future studies of the dynamic processes that shape south polar ice deposits. This is follow-on work to a previous study that produced a series of classified maps and a spectral library from CRISM targeted data. That work can be accessed with the following links: Publication: https://doi.org/10.1029/2022JE007372 Repository: https://doi.org/10.5281/zenodo.6960943 Contents The repository contains two .zip files, which can be expanded to access the files described below: classified_mosaics.zip lookup_files SP_CRISM_RF_ColorMap.clr : An ESRI-formatted color map file that can be used to apply the endmember color schemeto random forest-classified maps in ArcGIS (see Symbology settings). Note that for continuity with Cartwright (2022), there are 21 colors in this file, though only endmembers associated with 12 of those colors are present in the classified mosaics. SP_CRISM_RF_ColorMap.txt : A text file that can be loaded into Python as a numpy array and used to generate a matplotlib color ramp. Row indices correspond to endmember numbers (see below) and columns are red, green, and blue values ...
format Other/Unknown Material
author Cartwright, S. F. A.
author_facet Cartwright, S. F. A.
author_sort Cartwright, S. F. A.
title Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
title_short Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
title_full Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
title_fullStr Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
title_full_unstemmed Endmember spectra and classified mosaics derived from CRISM mapping data at the south pole of Mars
title_sort endmember spectra and classified mosaics derived from crism mapping data at the south pole of mars
publisher Zenodo
publishDate 2023
url https://doi.org/10.5281/zenodo.8201616
genre South pole
genre_facet South pole
op_relation https://doi.org/10.5281/zenodo.6960943
https://doi.org/10.1029/2022JE007372
https://doi.org/10.5281/zenodo.8201615
https://doi.org/10.5281/zenodo.8201616
oai:zenodo.org:8201616
op_rights info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
op_doi https://doi.org/10.5281/zenodo.820161610.5281/zenodo.696094310.1029/2022JE00737210.5281/zenodo.8201615
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