Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95499/1/grl22882.pd
International audienceWe present initial results from the first community-wide effort to compare glo...
International audienceDuring the last decade, MAVEN space mission have emphasized a widespread spati...
[1] Our newly developed 3‐D, multifluid MHD model is used to study the interaction of the solar wind...
A detailed model‐model comparison between the results provided by a multispecies and a multifluid ma...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95232/1/jgra17355.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95291/1/jgra16521.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95318/1/jgra21138.pd
We refine a recently presented method to estimate ion escape from non-magnetized planets and apply i...
Present-day Mars is a cold and dry planet with a thin CO2-dominated atmosphere comprising only a few...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/106987/1/grl51608.pd
Global models of the interaction of the solar wind with the Martian upper atmosphere have proved to ...
Because Mars has a weak magnetic field in comparison with Earth, the solar wind can directly interac...
International audienceIn November 2014 the MAVEN (Mars Atmosphere and Volatile EvolutioN) spacecraft...
A comprehensive study of the solar wind interaction with the Martian upper atmosphere is presented. ...
Using Mars Express data from 2007 until 2020 we show how ion outflow from Mars varied over more than...
International audienceWe present initial results from the first community-wide effort to compare glo...
International audienceDuring the last decade, MAVEN space mission have emphasized a widespread spati...
[1] Our newly developed 3‐D, multifluid MHD model is used to study the interaction of the solar wind...
A detailed model‐model comparison between the results provided by a multispecies and a multifluid ma...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95232/1/jgra17355.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95291/1/jgra16521.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95318/1/jgra21138.pd
We refine a recently presented method to estimate ion escape from non-magnetized planets and apply i...
Present-day Mars is a cold and dry planet with a thin CO2-dominated atmosphere comprising only a few...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/106987/1/grl51608.pd
Global models of the interaction of the solar wind with the Martian upper atmosphere have proved to ...
Because Mars has a weak magnetic field in comparison with Earth, the solar wind can directly interac...
International audienceIn November 2014 the MAVEN (Mars Atmosphere and Volatile EvolutioN) spacecraft...
A comprehensive study of the solar wind interaction with the Martian upper atmosphere is presented. ...
Using Mars Express data from 2007 until 2020 we show how ion outflow from Mars varied over more than...
International audienceWe present initial results from the first community-wide effort to compare glo...
International audienceDuring the last decade, MAVEN space mission have emphasized a widespread spati...
[1] Our newly developed 3‐D, multifluid MHD model is used to study the interaction of the solar wind...
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