On the problem of rotation of the ocean and icy crust of Jovian moon Europa

Details On the problem of rotation of the ocean and icy crust of Jovian moon Europa On the problem of rotation of the ocean and icy crust of Jovian moon Europa

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cosre..47..287r&link_type=abstract

Cosmic Research, Volume 47, Issue 4, pp.287-298

Mathematics

95.30.Ld

Scientific paper

A mathematical model of the non-steady-state magnetosphere of the ocean of Jupiter’s moon Europa is described. This magnetosphere is induced by the magnetic field of Jupiter, and its interaction with the Europa ocean is considered. Rotation of the ocean and its icy crust with respect to the hard core is described by a system of integro-differential equations with singular kernels, the values of the Reynolds number and magnetic Reynolds number being large for the system. The solution to these equations obtained by the methods of operational calculus is analyzed quantitatively and compared with a model experiment.

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