Thickness of the seasonal deposits by examining the shadow variations of the fallen ice blocks at Martian North Pole
Published: 9 January 2024| Version 1 | DOI: 10.17632/5yy475dbry.1
Contributors:
Haifeng Xiao, , , Frédéric Schmidt, , Description
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.
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Institutions
Instituto de Astrofisica de Andalucia
Categories
Snow, Mars