Journal articles
The induced magnetosphere of Mars. Asymmetrical topology of the magnetic field lines
Abstract : An asymmetrical pileup of the interplanetary magnetic field (IMF) leads to an additional draping of the field lines in the opposite direction to the motional electric field. Such a draping and the associated magnetic field forces push the ionosphere plasma in the transverse direction opening a passage for an ion trail which contains dense and slowly moving plasma. We found that wrapping of the field lines around Mars starts in the hemisphere pointing in the direction of the motional electric field and propagates to the opposite hemisphere where the cross‐flow component of the draped IMF changes sign in a broad area accompanied by the formation of loops of closed field lines. Reconnection near Mars accompanied by the generation of plasma vortices imposes serious constraints on the ion dynamics and their escape through the tail. The existence of all these features is confirmed by hybrid simulations.
Cited literature [30 references]
https://hal-insu.archives-ouvertes.fr/insu-02339781
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Tuesday, September 8, 2020 - 2:15:24 PM
Last modification on : Friday, December 3, 2021 - 11:42:53 AM
Long-term archiving on: : Friday, December 4, 2020 - 6:45:42 PM
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Tuesday, September 8, 2020 - 2:15:24 PM
Last modification on : Friday, December 3, 2021 - 11:42:53 AM
Long-term archiving on: : Friday, December 4, 2020 - 6:45:42 PM
File
2019GL084387.pdf
Publisher files allowed on an open archive