Add to ORKGsurface temperature is a central element in the descrip-tion of martian climate. Surface thermal inertia and albedo are critical boundary inputs for simulating sur-face temperature in Mars general circulation model
ose mesoscale-to-microscale meteorological events remains of key interest to betteThe thin veil of s...
International audienceWe have used two different General Circulation Models to study the thermal and...
The most widely used thermal inertia data for Mars assumes the atmospheric contribution is constant ...
The daily and seasonal variation of surface temperature is a central element in the description of m...
Introduction and general discussion Regional, diurnal and seasonal variations of surface temperature...
A general circulation model is used to evaluate changes to the circulation and dust transport in the...
International audienceRadiative control of surface temperature is a key characteristic of the martia...
Atmospheric dust on Mars is of fundamental importance to the overall climate system, as it can alter...
Airborne dust is the main driver of Martian atmospheric temperature, and accurately accounting for i...
The objective of this thesis is to present a configuration of the UM simulating the Martian climate ...
We study the interannual variability of dust storms on Mars in an assimilation of thermal profiles a...
Using a ground-to-exosphere general circulation model for Mars we have simulated the variability of ...
Calculations of the daily solar radiation incident at the tops of the atmospheres of Mars and the ou...
The influence of atmospheric dust on the dynamics and stability of the martian polar vortices is exa...
The planet Mars hosts an atmosphere that is perhaps the closest in terms of its meteorology and clim...
ose mesoscale-to-microscale meteorological events remains of key interest to betteThe thin veil of s...
International audienceWe have used two different General Circulation Models to study the thermal and...
The most widely used thermal inertia data for Mars assumes the atmospheric contribution is constant ...
The daily and seasonal variation of surface temperature is a central element in the description of m...
Introduction and general discussion Regional, diurnal and seasonal variations of surface temperature...
A general circulation model is used to evaluate changes to the circulation and dust transport in the...
International audienceRadiative control of surface temperature is a key characteristic of the martia...
Atmospheric dust on Mars is of fundamental importance to the overall climate system, as it can alter...
Airborne dust is the main driver of Martian atmospheric temperature, and accurately accounting for i...
The objective of this thesis is to present a configuration of the UM simulating the Martian climate ...
We study the interannual variability of dust storms on Mars in an assimilation of thermal profiles a...
Using a ground-to-exosphere general circulation model for Mars we have simulated the variability of ...
Calculations of the daily solar radiation incident at the tops of the atmospheres of Mars and the ou...
The influence of atmospheric dust on the dynamics and stability of the martian polar vortices is exa...
The planet Mars hosts an atmosphere that is perhaps the closest in terms of its meteorology and clim...
ose mesoscale-to-microscale meteorological events remains of key interest to betteThe thin veil of s...
International audienceWe have used two different General Circulation Models to study the thermal and...
The most widely used thermal inertia data for Mars assumes the atmospheric contribution is constant ...