NASA NTRS · 20020046065
Modelling Mass Movements for Planetary Studies
Abstract
Use of an empirical model in conjunction with data from the Chaos Jumbles rock avalanches constrain to first order their flow behavior, and provide a method to interpret rock/debris avalanche emplacement on Mars. Additional information is contained in the original extended abstract.
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Bulmer, M. H., Glaze, L., Barnouin-Jha, O., Murphy, W., Neumann, G.. 2002-04-01. Modelling Mass Movements for Planetary Studies. https://ntrs.nasa.gov/citations/20020046065
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