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 …

Although not the prime focus of the InSight mission, the near-surface geology and physical
properties investigations provide critical information for both placing the instruments …

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 …

Nine simulations are used to predict the meteorology and aeolian activity of the Mars 2020
landing site region. Predicted seasonal variations of pressure and surface and atmospheric …

In November 2018, for the first time a dedicated geophysical station, the InSight lander, will
be deployed on the surface of Mars. Along with the two main geophysical packages, the …

The movement of active dunes is tightly linked to climatic conditions (eg, wind regime,
temperature and precipitation) as well as human influence (eg, grazing, dune fixation and …

The characteristics of the wind regime and the development of dune morphology in the
Taklamakan Desert have been the focus of scholars. In this study, we used ERA5 reanalysis …

Dunes are among the most abundant aeolian landforms found on Earth and other planets.
The automatic mapping of dunes over large-scale areas is crucial for predicting, monitoring …

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 …

Although dunes are very common bedforms in terrestrial sand seas, the description of linear
dune growth, either by extension or lateral accretion, is still hindered by our limited …