Comparison of Effusive Volcanism at Olympus, Arsia, Pavonis, and Ascraeus Montes, Mars from Lava Flow Mapping Using Mars Express HRSC Data

Details Comparison of Effusive Volcanism at Olympus, Arsia, Pavonis, and Ascraeus Montes, Mars from Lava Flow Mapping Using Mars Express HRSC Data Comparison of Effusive Volcanism at Olympus, Arsia, Pavonis, and Ascraeus Montes, Mars from Lava Flow Mapping Using Mars Express HRSC Data

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1182b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1182

Physics

2

Scientific paper

HRSC data enable lava flow mapping at high resolution with regional
context. Results show a flank transition to channel-forming eruptions,
followed by rift apron development where each volcano displays different
morphologies and flow relationships.

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