Diurnal changes in solar radiation on Mars set up a cycle of cooling and heating of the planetary boundary layer, this effect strongly influences the wind field. The stratification of the air layer is stable in early morning since the ground is cooler than the air above it. When the ground is heated and becomes warmer than the air its heat is transferred to the air above it. The heated parcels of air near the surface will, in effect, increase the near surface wind speed or increase the aeolian surface stress the wind has upon the surface when compared to an unheated or cooled surface. This means that for the same wind speed at a fixed height above the surface, ground-level shear stress will be greater for the heated surface than an unheated...
The Mars moon Phobos passed in front of the Sun from the perspective of the InSight lander on severa...
Radiative-conductive heat transfer has been investigated for the ground-atmosphere system of the pla...
Numerical simulations of the Martian near-surface wind regime using a mesoscale atmospheric model ha...
International audienceRadiative control of surface temperature is a key characteristic of the martia...
Regional, diurnal and seasonal variations of surface temperature are particularly large on Mars. Th...
Aeolian activity was predicted for Mars from earth based observations of changing surface patterns t...
Surface wind stresses and dust lifting in the south polar region of Mars are examined with a three-d...
The impact of Mars’ 2018 Global Dust Storm (GDS) on surface and near‐surface air temperatures was in...
A number of different dust lifting parameterizations have been used to model the injection of dust f...
Background: Mars si both a windy and dusty environment. Ariborne dust is a crucial climate component...
Aeolian processes are important in modifying the surface of Mars at present, and appear to have been...
Studies concerning mesoscale topographical effects on Martian flows examined low-level jets in the n...
abstract: The temperature of a planet's surface depends on numerous physical factors, including ther...
The physics and geological relationships of particles driven by the wind under near Martian conditio...
An apparatus has been fabricated to simulate terrestrial and Martian dust devils. Comparisons of sur...
The Mars moon Phobos passed in front of the Sun from the perspective of the InSight lander on severa...
Radiative-conductive heat transfer has been investigated for the ground-atmosphere system of the pla...
Numerical simulations of the Martian near-surface wind regime using a mesoscale atmospheric model ha...
International audienceRadiative control of surface temperature is a key characteristic of the martia...
Regional, diurnal and seasonal variations of surface temperature are particularly large on Mars. Th...
Aeolian activity was predicted for Mars from earth based observations of changing surface patterns t...
Surface wind stresses and dust lifting in the south polar region of Mars are examined with a three-d...
The impact of Mars’ 2018 Global Dust Storm (GDS) on surface and near‐surface air temperatures was in...
A number of different dust lifting parameterizations have been used to model the injection of dust f...
Background: Mars si both a windy and dusty environment. Ariborne dust is a crucial climate component...
Aeolian processes are important in modifying the surface of Mars at present, and appear to have been...
Studies concerning mesoscale topographical effects on Martian flows examined low-level jets in the n...
abstract: The temperature of a planet's surface depends on numerous physical factors, including ther...
The physics and geological relationships of particles driven by the wind under near Martian conditio...
An apparatus has been fabricated to simulate terrestrial and Martian dust devils. Comparisons of sur...
The Mars moon Phobos passed in front of the Sun from the perspective of the InSight lander on severa...
Radiative-conductive heat transfer has been investigated for the ground-atmosphere system of the pla...
Numerical simulations of the Martian near-surface wind regime using a mesoscale atmospheric model ha...