New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars

Details New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3397m&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3397

Physics

Scientific paper

We suggest that the tectonic and topographic structure of Olympus Mons
is controlled by spatially varying frictional conditions at the base of
the edifice, which in turn are established by variations in ancient
sediment deposits imposed by regional topography and basement roughness.

Affiliated with

Also associated with

No associations

Rating

New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Models of Volcanic Spreading and Implications for Azimuthal Variations in the Structure of Olympus Mons, Mars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-786112