Global tectonic patterns of the Moon
Data analyzed in this study were a re-analysis of existing data, which are openly available at locations cited in the reference section of "Global tectonic patterns of the Moon". The data are the spherical harmonic expansion coefficients of South-Pole Aitken (SPA) and Lunar Mare models. Fo...
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| Format: | Dataset |
| Language: | unknown |
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University of Arizona Research Data Repository
2020
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| Online Access: | https://dx.doi.org/10.25422/azu.data.12935162.v1 https://arizona.figshare.com/articles/dataset/Global_tectonic_patterns_of_the_Moon/12935162/1 |
| Summary: | Data analyzed in this study were a re-analysis of existing data, which are openly available at locations cited in the reference section of "Global tectonic patterns of the Moon". The data are the spherical harmonic expansion coefficients of South-Pole Aitken (SPA) and Lunar Mare models. Format for the spherical harmonics is the usual SHTOOLS format: l, m, Clm, Slm. The SPA crustal thickness data (SHTOOLS_SH_correctedcrustalthickness_v2_180919_0000_to_0310.txt) is a table of the normalized spherical harmonic expansion coefficients from l=0 to l=310.The Lunar Mare data (SHTOOLS_SH_lunarmare_0000_to_0179.txt) is a table of the normalized spherical harmonic expansion coefficients from l=0 to l=179 For inquiries regarding the contents of this dataset, please contact the Corresponding Author listed in the README.txt file. Administrative inquiries (e.g., removal requests, trouble downloading, etc.) can be directed to data-management@arizona.edu |
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