Idealized Jovian magnetosphere shape and field

Physics

Scientific paper

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Jupiter Atmosphere, Magnetic Field Configurations, Pioneer 10 Space Probe, Planetary Magnetic Fields, Planetary Magnetospheres, Atmospheric Models, Current Sheets, Geomagnetic Tail, Magnetic Dipoles, Magnetopause, Periodic Variations, Jupiter, Magnetosphere, Shape, Magnetic Fields, Models, Pioneer 11, Magnetopause, Current Sheets, Procedure, Pressure, Magnetotail, Thermal Effects, Data, Equatorial Regions, Dipole, Solar Wind, Mathematical Models, Spherical Harmonic Analysis, Boundary Layers

Scientific paper

An equatorial sheet current deduced from Pioneer 10 magnetic field observations has been added to a planetary dipole field to construct a model of magnetic field due to sources inside the magnetopause. This internal field has then been used to calculate the magnetopause surface in a cyclic process to a fifth order, in cycles, at which the calculation converges. The resulting magnetopause is considerably flatter in shape than one resulting from a primarily dipole internal field source. The field internal and external to the magnetopause surface due to the currents on the surface has been computed by integrating over the entire magnetopause. A model for the total magnetospheric field of the inflated magnetosphere has been constructed by adding this latter contribution to the internal source fields to obtain a global model of an inflated Jovian-like magnetospheric field.

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