Journal articles
Electron and Ion Dynamics of the Solar Wind Interaction with a Weakly Outgassing Comet
Abstract : Using a 3D fully kinetic approach, we disentangle and explain the ion and electron dynamics of the solar wind interaction with a weakly outgassing comet. We show that, to first order, the dynamical interaction is representative of a four-fluid coupled system. We self-consistently simulate and identify the origin of the warm and suprathermal electron distributions observed by ESA’s Rosetta mission to comet 67P/Churyumov-Gerasimenko and conclude that a detailed kinetic treatment of the electron dynamics is critical to fully capture the complex physics of mass-loading plasmas.
Cited literature [62 references]
https://hal-insu.archives-ouvertes.fr/insu-01541244
Contributor : Nathalie Rouchon <>
Submitted on : Thursday, December 20, 2018 - 3:53:22 PM
Last modification on : Tuesday, July 21, 2020 - 4:04:38 AM
Document(s) archivé(s) le : Friday, March 22, 2019 - 12:57:13 PM
Contributor : Nathalie Rouchon <>
Submitted on : Thursday, December 20, 2018 - 3:53:22 PM
Last modification on : Tuesday, July 21, 2020 - 4:04:38 AM
Document(s) archivé(s) le : Friday, March 22, 2019 - 12:57:13 PM
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Deca-2017.pdf
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