Ice nucleation by surrogates of Martian mineral dust: What can we learn about Mars without leaving Earth?
Water and carbon dioxide ice clouds have been observed in the Martian atmosphere where they are dynamic parts of that planet's water and carbon cycles. Many Martian atmospheric models struggle to correctly predict clouds and, with insufficient data, some use untested simplifications that cloud...
Main Authors: | , , , , , , , , |
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Outros autores: | |
Formato: | Artigo |
Idioma: | en_US |
Publicado: |
American Geophysical Union
2014
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Acceso en liña: | http://hdl.handle.net/1721.1/87715 https://orcid.org/0000-0003-1851-8740 https://orcid.org/0000-0002-0828-8286 |