This repository contains: 1. Calculated spectra of snow-dust mixtures from Khuller and Christensen (2020) 2. Measured spectra of ice and soil from Blaney et al. (2009) 3. Refractive indices of martian dust from Wolff et al. (2009) 4. Effective thermal conductivities of martian snow and ice, based on Clow (1987). 5. Image details of HiRISE, CTX and THEMIS images analyzed in this work. References: Blaney, D. L., Archer, D., Arvidson, R., Cull, S., Ellehøj, M., Fisher, D., ... & Pike, T. (2009). Multi-spectral imaging of the Phoenix landing site: Characteristics of surface and subsurface ice, rocks, and soils. LPI, 2047. Clow, G. D. (1987). Generation of liquid water on Mars through the melting of a dusty snowpack. Icarus, 72(1), 95-12...
The distribution and nature of water ice on Mars has important implications for understanding the Ma...
The aim of this project is to model the Martian water cycle, including radiatively active water ice ...
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we d...
This repository contains: 1. Calculated spectra of snow-dust mixtures from Khuller and Christensen ...
Thesis (Ph.D.)--University of Washington, 2018The water cycle of Mars has been intensely studied tha...
NASA\u27s Phoenix Lander uncovered two types of ice at its 2008 landing site on the northern plains ...
This repository contains: 1. Snow/Ice Albedos from Khuller, Christensen & Warren (2021) a) Clean Sn...
These files were produced as part of the study entitled “Thermal infrared spectral characteristics o...
Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction...
The Mars Subsurface Water Ice Mapping (SWIM) Project is a NASA-funded effort using orbital remote-se...
A thermal model is developed to find the distribution of stable near-surface ground ice on Mars that...
International audienceThe properties of Martian aerosols are an integral part of the planetary clima...
International audienceExtensive evidence of landform-scale martian geomorphic changes has been acqui...
The penetration depth of broad spectrum solar radiation (300 nm – 1100 nm) in ices relevant to Mars ...
One of the many questions of Martian exploration is to uncover the history of Mars, through analysis...
The distribution and nature of water ice on Mars has important implications for understanding the Ma...
The aim of this project is to model the Martian water cycle, including radiatively active water ice ...
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we d...
This repository contains: 1. Calculated spectra of snow-dust mixtures from Khuller and Christensen ...
Thesis (Ph.D.)--University of Washington, 2018The water cycle of Mars has been intensely studied tha...
NASA\u27s Phoenix Lander uncovered two types of ice at its 2008 landing site on the northern plains ...
This repository contains: 1. Snow/Ice Albedos from Khuller, Christensen & Warren (2021) a) Clean Sn...
These files were produced as part of the study entitled “Thermal infrared spectral characteristics o...
Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction...
The Mars Subsurface Water Ice Mapping (SWIM) Project is a NASA-funded effort using orbital remote-se...
A thermal model is developed to find the distribution of stable near-surface ground ice on Mars that...
International audienceThe properties of Martian aerosols are an integral part of the planetary clima...
International audienceExtensive evidence of landform-scale martian geomorphic changes has been acqui...
The penetration depth of broad spectrum solar radiation (300 nm – 1100 nm) in ices relevant to Mars ...
One of the many questions of Martian exploration is to uncover the history of Mars, through analysis...
The distribution and nature of water ice on Mars has important implications for understanding the Ma...
The aim of this project is to model the Martian water cycle, including radiatively active water ice ...
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we d...