Using MOLASSES, A Lava Flow Simulation Code, to Interpret the Morphology of Volcanoes: Example of Olympus Mons (Mars)

Authors

Charles Connor, University of South FloridaFollow
Laura Connor, University of South FloridaFollow
J A. Richardson, NASA Goddard Space Flight Center
Elisabeth Gallant, University of South FloridaFollow
Diana Miller, University of South FloridaFollow

Document Type

Poster Session

Publication Date

3-20-2018

Abstract

MOLASSES is a new lava flow simulator that helps infer eruptive processes from the topography of remotely observed volcano landforms, like Olympus Mons volcano.

Was this content written or created while at USF?

Yes

Citation / Publisher Attribution

Presented at the 49th Lunar and Planetary Science Conference on March 20, 2018 in The Woodlands, TX

Scholar Commons Citation

Connor, Charles; Connor, Laura; Richardson, J A.; Gallant, Elisabeth; and Miller, Diana, "Using MOLASSES, A Lava Flow Simulation Code, to Interpret the Morphology of Volcanoes: Example of Olympus Mons (Mars)" (2018). School of Geosciences Faculty and Staff Publications. 1100.
https://digitalcommons.usf.edu/geo_facpub/1100