The microstructural evolution of water ice in the solar system through sintering.

Molaro, J L; Choukroun, M; Phillips, C B; Phelps, E S; Hodyss, R; Mitchell, K L; Lora, J M; Meirion-Griffith, G

Molaro, J L; Choukroun, M; Phillips, C B; Phelps, E S; Hodyss, R; Mitchell, K L; Lora, J M; Meirion-Griffith, G.

Afiliação

Molaro JL; Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719, USA.
Choukroun M; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Phillips CB; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Phelps ES; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Hodyss R; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Mitchell KL; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Lora JM; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
Meirion-Griffith G; University of California, Los Angeles, 595 Charles Young Drive East, Los Angeles, CA 90095, USA.

J Geophys Res Planets ; 124(2): 243-277, 2019 Feb.

Article em En | MEDLINE | ID: mdl-32874819

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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2019 Tipo de documento: Article

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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2019 Tipo de documento: Article