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Titel Four Fluid Plasma-Neutral Simulations of the Plasma Environment of 67P/C-G
VerfasserIn Zhenguang Huang, Tamas Gombosi, Gabor Toth, Xianzhe Jia, André Bieler, Kenneth Hansen, Yinsi Shou, Kathrin Altwegg Link zu Wikipedia, Martin Rubin
Konferenz EGU General Assembly 2015
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 17 (2015)
Datensatznummer 250103601
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2015-3015.pdf
 
Zusammenfassung
A 3D four fluid (solar wind ions, cometary ions, electrons and cometary neutrals) simulation capability has been developed for the support of the Rosetta mission. Our model is based on our multi-physics code, BATS-R-US, within the SWMF (Space Weather Modeling Framework) that solves the governing equations of multi fluid HD/MHD. The model includes various mass-loading processes, including ionization, charge exchange, dissociative ion-electron recombination, as well as collisional interactions between different fluids. Simulation results are presented for various heliocentric distances and compared to Rosetta neutral and ion observations.