Physics
Scientific paper
Mar 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1170g&link_type=abstract
42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1170
Physics
Scientific paper
Resolving a common flaw in numerical models of ring fault (hence
caldera) formation (1) leads to a new understanding of where/why ring
faults can form, and (2) reconciles long-standing differences between
analogue and numerical model results.
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