We are currently working in adapting a microphysical model previously developed for the water ice clouds formation on Mars ([14], based on that of [17]) with the aim at coupling it to a mesoscale and a general circulation model We will describe the model used and present the modifications we initiated.
from HAL : Dernières publications http://ift.tt/1pxeyHF
from HAL : Dernières publications http://ift.tt/1pxeyHF

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