Mars exhibits diverse surface changes at all latitudes and all seasons. Active processes
include impact cratering, aeolian sand and dust transport, a variety of slope processes …

The first in situ investigation of an active dune field on another planetary surface occurred in
2015–2016 when the Mars Science Laboratory Curiosity rover investigated the Bagnold …

We provide a critical review of research paradigms for classifying intermediate‐scale
aeolian bedforms on Mars and the new terminology that has emerged. The systematic …

Rover data can provide important constraints on the possible origin of wind‐related martian
features that have been termed “Transverse Aeolian Ridges”(TARs). The large aeolian …

Abstract Aeolian features at Oxia Planum—the 2023 landing site for the ExoMars Rosalind
Franklin Rover (ERFR)—are important for Mars exploration because they record information …

Aeolian processes have likely been the predominant geomorphic agent for most of Mars'
history and have the potential to produce relatively young exposure ages for geologic units …

A new terrestrial analog site for transverse aeolian ridges (TARs) is described in this study.
The Lut desert of Iran hosts large ripple-like aeolian bedforms, with the same horizontal …

Change detection analyses of aeolian bedforms (dunes and ripples), using multitemporal
images acquired by the Mars Reconnaissance Orbiter High Resolution Imaging Science …

Aeolian sediment transport, deposition, and erosion have been ongoing throughout Mars's
history. This record of widespread aeolian processes is preserved in landforms and geologic …

Abstract Transverse Aeolian Ridges (TARs) are curious aeolian megaripples on Mars, but
there are few sites identified thus far to study as terrestrial analogs. A new terrestrial analog …