Thickness of the seasonal deposits by examining the shadow variations of the fallen ice blocks at Martian North Pole
HiRISE_1m_DEM is the generated 1/pixel DEM at the Martian scarp centered at (85.0°N, 151.5°E);Snofall_thickness_in_MY31.py can be used to reproduce Figure 9 in Xiao et al. (2024);Interannual_snowfall_variations_in_early_spring.py can be used to reproduce Figure 11 in Xiao et al. (2024);Crown_depth_e...
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Language: | unknown |
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2024
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Online Access: | http://nbn-resolving.org/urn:nbn:nl:ui:13-ut-qtct https://easy.dans.knaw.nl/ui/datasets/id/easy-dataset:331402 |
Summary: | HiRISE_1m_DEM is the generated 1/pixel DEM at the Martian scarp centered at (85.0°N, 151.5°E);Snofall_thickness_in_MY31.py can be used to reproduce Figure 9 in Xiao et al. (2024);Interannual_snowfall_variations_in_early_spring.py can be used to reproduce Figure 11 in Xiao et al. (2024);Crown_depth_estimation.py can be used to reproduce Figure 13 in Xiao et al. (2024);Total_thickness_of_snowfall_and_frost.py can be used to reproduce Figure 14 in Xiao et al. (2024).Xiao, H., Xiao, Y., Su, S., Schmidt, F., Lara, L. M., & Gutiérrez, P. J. (2024). Thickness of the seasonal deposits by examining the shadow variations of the fallen ice blocks at Martian North Pole. Journal of Geophysical Research: Planets. In Revision. THIS DATASET IS ARCHIVED AT DANS/EASY, BUT NOT ACCESSIBLE HERE. TO VIEW A LIST OF FILES AND ACCESS THE FILES IN THIS DATASET CLICK ON THE DOI-LINK ABOVE |
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