Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style
Author:
Funder
Arizona State University
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference59 articles.
1. Amazonian-aged fluvial system and associated ice-related features in Terra Cimmeria, Mars;Adeli;Icarus,2016
2. Thermophysical properties and surface heterogeneity of landing sites on Mars from overlapping Thermal Emission Imaging System (THEMIS) observations;Ahern;J. Geophys. Res. Planets,2021
3. Anatomy of a White Mountains debris-flow – the making of an alluvial fan;Beaty,1990
4. Surface clay formation during short-term warmer and wetter conditions on a largely cold ancient Mars;Bishop;Nat. Astron.,2018
5. Cause of dominance by sheetflood vs. debris flow processes on two adjoning alluvial fans, Death Valley, California;Blair;Sedimentology,1999
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