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Volumn 318, Issue 5853, 2007, Pages 1125-1128

Radar sounding of the medusae fossae formation mars: Equatorial ice or dry, low-density deposits?

Author keywords

[No Author keywords available]

Indexed keywords

DENSITY; DUST; EOLIAN DEPOSIT; FORMATION MECHANISM; ICE; MARS; RADAR; VOLCANIC ASH;

EID: 36249023635     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1148112     Document Type: Article
Times cited : (146)

References (29)
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    • We are grateful to the other members of the MARSIS Science team and to the instrument operation staff. MARSIS is managed by the Agenzia Spaziale Italiana (ASI) and NASA. The Mars Express mission is managed and operated by the European Space Agency. The research activities of the MARSIS PI and Italian investigators are supported by grants under the Mars Express/ASI program. Work of the U.S. investigators is supported by grants under the Mars Express/NASA project
    • We are grateful to the other members of the MARSIS Science team and to the instrument operation staff. MARSIS is managed by the Agenzia Spaziale Italiana (ASI) and NASA. The Mars Express mission is managed and operated by the European Space Agency. The research activities of the MARSIS PI and Italian investigators are supported by grants under the Mars Express/ASI program. Work of the U.S. investigators is supported by grants under the Mars Express/NASA project.


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