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Interaction of the Solar Wind with Weak Obstacles: Hybrid Simulations for Weakly Active Comets and for Mars
DOI: 10.1007/s11214-006-6218-2 Bibcode: 2006SSRv..122..197M

Kührt, E.; Motschmann, U.

Obstacles in the solar wind are weak when their extension is small or comparable to the characteristic ion gyroradii. In this case interactions involve kinetic features, and hybrid models are an adequate description. A hybrid code operating on a curvilinear 3D grid and its application to solar wind interaction with weak obstacles is discussed. The…

2006 Space Science Reviews
Rosetta 24