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机译:Interannual perturbations of the Martian surface heat flow by atmospheric dust opacity variations
German Aerospace Center (DLR), Berlin, Germany;
Department of Atmospheric Sciences, Texas A&M University, College Station, Texas, USA;
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USAPlanetary Science Institute, Tucson, Arizona, USA;
We use a 5 Mars years time series of the Martian atmospheric; dust opacity data to quantify the magnitude of the heat flow perturbations; Numerical simulations show minor and moderate pertubation; of the heat flow caused by local and global dust storm; respectively; The heat pulse introduced by global dust storms travels; up to a depth of 3 m and can only be observed in the Mars year following the storm;