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...

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Detalles Bibliográficos
Main Authors: Cziczo, Daniel James, Garimella, Sarvesh, Raddatz, Michael, Hoehler, Kristina, Schnaiter, Martin, Saathoff, Harald, Moehler, Ottmar, Abbatt, Jonathan P. D., Ladino, Luis A.
Outros autores: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Formato: Artigo
Idioma:en_US
Publicado: American Geophysical Union 2014
Acceso en liña:http://hdl.handle.net/1721.1/87715
https://orcid.org/0000-0003-1851-8740
https://orcid.org/0000-0002-0828-8286