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Stability of water ice beneath porous dust layers of the Martian south polar terrain

MPS-Authors
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Keller,  H. U.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Skorov,  Y. V.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Markiewicz,  W. J.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Keller, H. U., Skorov, Y. V., Markiewicz, W. J., & Basilevsky, A. T. (2000). Stability of water ice beneath porous dust layers of the Martian south polar terrain. In H. Björnsson, S. Clifford, D. Paige, & T. Thornsteinsson (Eds.), The Second International Conference on Mars Polar Science and Exploration. Houston, Texas/USA: Lunar and Planetary Institute.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-E188-4
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