Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm23b1608r&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SM23B-1608
Physics
[5405] Planetary Sciences: Solid Surface Planets / Atmospheres, [5421] Planetary Sciences: Solid Surface Planets / Interactions With Particles And Fields, [5443] Planetary Sciences: Solid Surface Planets / Magnetospheres, [6221] Planetary Sciences: Solar System Objects / Europa
Scientific paper
Jupiter’s moon Europa has a thin gravitationally bound neutral atmosphere which is mostly created through sputtering of high energy ions impacting on its icy surface. In a first step we will simulate the interaction of Europa with the Jovian magnetosphere by using the magnetohydrodynamics (MHD) model BATSRUS. Starting from the model used by Kabin et al. [JGR, Vol. 104, No. A9, (1999)] which accounts for the exospheric mass loading, ion-neutral charge exchange, and recombination we will further use the resistive MHD equations addressing the finite electron diffusivity. These results, including the magnetic field topology, are then used to calculate the Lorentz forces for our test particle Monte Carlo model. We use this model to simulate Europa’s plasma and neutral environment by tracking particles created on the moon’s surface by sputtering or sublimation, through dissociation and/or ionization in the atmosphere, or entering the system from Jupiter’s magnetosphere as high energy ions. Neutral particle trajectories are followed by solving the equation of motion in Europa’s gravity field whereas the ion population is additionally subject to the Lorentz force. We will show preliminary results of this work with application to the missions to the Jupiter system currently under consideration by NASA (JEO) and ESA (JGO).
Combi Michael R.
Gombosi Tamas I.
Hansen Kenneth Calvin
Jia Xun
Rubin Mathieu
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