We will present results obtained with the 1D- simulations of mesospheric CO2 ice clouds within cold pockets created by gravity waves, and compare them to observations. Simple dust scenarios are pre- scribed to account for condensation nuclei, necessary to explain measured opacities
International audienceSince the first probable observation of a CO2 mesospheric cloud on Mars [1] th...
International audienceSince the first claimed detection of CO2 ice clouds by the Mariner campaign (H...
International audienceWe have implemented full CO 2 ice cloud microphysics into the LMD Mars Global ...
We will present results obtained with the 1D- simulations of mesospheric CO2 ice clouds within cold ...
International audienceMesospheric CO2 ice clouds on Mars are simulated with a 1D microphysical model...
International audienceSince the first probable observation of a CO2 mesospheric cloud on Mars [1] th...
International audienceSince the first claimed detection of CO2 ice clouds by the Mariner campaign (H...
International audienceWe have implemented full CO 2 ice cloud microphysics into the LMD Mars Global ...
We will present results obtained with the 1D- simulations of mesospheric CO2 ice clouds within cold ...
International audienceMesospheric CO2 ice clouds on Mars are simulated with a 1D microphysical model...
International audienceSince the first probable observation of a CO2 mesospheric cloud on Mars [1] th...
International audienceSince the first claimed detection of CO2 ice clouds by the Mariner campaign (H...
International audienceWe have implemented full CO 2 ice cloud microphysics into the LMD Mars Global ...