Global Surface Winds and Aeolian Sediment Pathways on Mars from the Morphology of Barchan Dunes
In the absence of consistent meteorological data on Mars, the morphology of dunes can be employed to study its atmosphere. Specifically, barchan dunes, which form under approximately unimodal winds, are reliable proxies for the dominant wind direction. Here, we characterize near-surface winds on Mar...
Main Authors: | , , , , , , |
---|---|
Format: | Other/Unknown Material |
Language: | unknown |
Published: |
Authorea, Inc.
2022
|
Subjects: | |
Online Access: | http://dx.doi.org/10.22541/essoar.167169649.93488411/v1 |