Extensive evidence of landform-scale martian geomorphic changes has been acquired in
the last decade, and the number and range of examples of surface activity have increased …

It has been over a decade since COSI-Corr, the Co-Registration of Optically Sensed Images
and Correlation, was first used to produce a raster map of sand dune movement, however …

Untitled Page 1 Page 2 GEOMORPHOLOGY OF DESERT DUNES Sand dunes cover up to a
quarter of many desert regions. Determining the factors that determine their shape, size and …

Strong and sustained winds on Mars have been considered rare, on the basis of surface
meteorology measurements and global circulation models,, raising the question of whether …

The ripple field known as “El Dorado” was a unique stop on Spirit's traverse where dust‐
raising, active mafic sand ripples and larger inactive coarse‐grained ripples interact …

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 …

The structure of the barchan field located between Tarfaya and Laayoune (Atlantic Sahara,
Morocco) is quantitatively investigated and compared to that in La Pampa de la Joya …

Wind has been an enduring geologic agent throughout the history of Mars, but it is often
unclear where and why sediment is mobile in the current epoch. We investigated whether …

Quantifying sand flux with field measurements is an expensive and time‐consuming
process. We here present an alternative approach using the COSI‐Corr software package …

Sand dune movement causes severe damage to infrastructure and rural settlements in Iran
every year. Identifying active dunes and monitoring areas with migrating sand are important …