The transport of sand and dust by wind is a potent erosional force, creates sand dunes and
ripples, and loads the atmosphere with suspended dust aerosols. This paper presents an …

The planet Mars hosts an atmosphere that is perhaps the closest in terms of its meteorology
and climate to that of the Earth. But Mars differs from Earth in its greater distance from the …

We identify temporal variations in surface albedo at Jezero crater using first‐of‐their‐kind
high‐cadence in‐situ measurements of reflected shortwave radiation during the first 350 …

Sublimation-thermokarst landforms result from collapse of the surface when ice is lost from
the subsurface. On Mars, scalloped landforms with scales of decameters to kilometers are …

The vertical distribution of dust in Mars' atmosphere is a critical unknown in the simulation of
its general circulation and a source of insight into the lifting and transport of dust. Zonal …

Spirit began operations in Gusev Crater in January 2004 and has returned data on three
seasons of dust devil (DD) activity. Total DDs observed were 533 in season one, 101 in …

Abstract The Mars Environmental Dynamics Analyzer, onboard the Perseverance rover, is a
meteorological station that is operating on Mars and includes, among other sensors, the …

We report the aeolian changes observed in situ by NASA's InSight lander during the first 400
sols of operations: Granule creep, saltation, dust removal, and the formation of dark surface …

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 …

Two hundred fifty‐two transient drops in atmospheric pressure, likely caused by passing
convective vortices, were detected by the Rover Environmental Monitoring Station …