Premium
Callisto plasma interactions: Hybrid modeling including induction by a subsurface ocean
Author(s) -
Lindkvist Jesper,
Holmström Mats,
Khurana Krishan K.,
Fatemi Shahab,
Barabash Stas
Publication year - 2015
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2015ja021212
Subject(s) - magnetosphere , jupiter (rocket family) , plasma , physics , astrobiology , geophysics , solar wind , dipole , computational physics , spacecraft , astronomy , quantum mechanics
By using a hybrid plasma solver (ions as particles and electrons as a fluid), we have modeled the interaction between Callisto and Jupiter's magnetosphere for variable ambient plasma parameters. We compared the results with the magnetometer data from flybys (C3, C9, and C10) by the Galileo spacecraft. Modeling the interaction between Callisto and Jupiter's magnetosphere is important to establish the origin of the magnetic field perturbations observed by Galileo and thought to be related to a subsurface ocean. Using typical upstream magnetospheric plasma parameters and a magnetic dipole corresponding to the inductive response inside the moon, we show that the model results agree well with observations for the C3 and C9 flybys, but agrees poorly with the C10 flyby close to Callisto. The study does support the existence of a subsurface ocean at Callisto.