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  • EP31D: Aeolian Processes and Liquid Flows Shaping Landscapes of the Solar System I Poster
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Primary Convener:
Carlos Gary Bicas, Louisiana State University

Convener:
Colin Marvin, Stanford University
Indujaa Ganesh, University of Arizona
Mathieu Lapotre, Stanford University
Gaia Stucky de Quay, Harvard University
Madeline Kelley, USGS, Southwest Biological Science Center, Grand Canyon Monitoring and Research Center
Suniti Karunatillake, Louisiana State University

Early Career Convener:
Colin Marvin, Stanford University

Chair:
Colin Marvin, Stanford University
Suniti Karunatillake, Louisiana State University
Mathieu Lapotre, Stanford University

The signatures of aeolian processes and liquid flows record interactions across planetary interiors, surfaces, and atmospheres on a variety of planetary bodies. Accordingly, we consolidate two proposed sessions centered on aeolian processes and liquid flows in the Solar System, while maintaining their original foci. A portion of the contributions focuses on windblown landscapes, including (but not limited to) sediment transport, bedform and aeolian morphodynamics, the aeolian rock record, dust, and coastal aeolian environments across planets. The rest examines landscape evolution from liquid flows at the critical zone, where exchanges between planetary crusts and atmospheres take place. Examples include water-driven paleochannels, cryospheric processes, global hydrology, and lava flows. Studies of aeolian-fluvial interactions, approaches to instrumentation, theory, Earth-analogs, experimental work, and data analyses bridge the scopes of both proposed topical sessions.

Index Terms
0343 Planetary atmospheres
1862 Sediment transport
5419 Hydrology and fluvial processes
5470 Surface materials and properties

Cross-Listed:
P - Planetary Sciences

Co-Sponsored Sessions:
CGS: Chinese Geophysical Society
AAS: American Astronomical Society
JpGU: Japan Geoscience Union
EGU: European Geosciences Union

Neighborhoods:
3. Earth Covering

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