Volatile Losses from Lava Flows Revisited: Implications for Large Sheet Flows on Mars

Details Volatile Losses from Lava Flows Revisited: Implications for Large Sheet Flows on Mars Volatile Losses from Lava Flows Revisited: Implications for Large Sheet Flows on Mars

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1961b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1961

Physics

Scientific paper

Degassing may be an important process for explaining why long lava flows
on Mars show modest increases in thickness with distance. A new
formulation for the rate of degassing sets the stage for deriving
exsolution velocities and extending the model to include bubble growth
during emplacement.

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