A Broad Continuum of Aeolian Impact Ripple Morphologies on Mars is Enabled by Low Wind Dynamic Pressures-Reference-Cited by-同舟云学术

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A Broad Continuum of Aeolian Impact Ripple Morphologies on Mars is Enabled by Low Wind Dynamic Pressures

Published:2020-10 Issue:10 Volume:125 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Sullivan R.¹^ORCID,Kok J. F.²^ORCID,Katra I.³,Yizhaq H.⁴^ORCID

Affiliation:

1. Cornell Center for Astrophysics and Planetary Sciences Cornell University Ithaca NY USA

2. Department of Atmospheric and Oceanic Sciences University of California, Los Angeles Los Angeles CA USA

3. Department of Geography and Environmental Development Ben‐Gurion University of the Negev Beer Sheva Israel

4. Department of Solar Energy and Environmental Physics BIDR, Ben‐Gurion University of the Negev Beer Sheva Israel

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JE006485

Reference135 articles.

1. Assessing the Martian surface distribution of aeolian sand using a Mars general circulation model

2. A theoretical model for aeolian impact ripples

3. Eolian ripples as examples of self-organization in geomorphological systems

4. Geomorphology

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4. Multiple Evolution Modes of Megaripples in the Qaidam Basin and Implications for Ripple‐Like Aeolian Landforms on Mars;Journal of Geophysical Research: Earth Surface;2024-03

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