Analytical two-dimensional model for a pole-on magnetosphere

Details Analytical two-dimensional model for a pole-on magnetosphere Analytical two-dimensional model for a pole-on magnetosphere

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29.1101b&link_type=abstract

Planetary and Space Science, vol. 29, Oct. 1981, p. 1101-1107.

Astronomy and Astrophysics

Astronomy

6

Conformal Mapping, Magnetic Field Configurations, Magnetopause, Planetary Magnetic Fields, Solar Activity Effects, Solar Wind, Two Dimensional Models, Uranus Atmosphere, Astronomical Models, Boundary Value Problems, Magnetic Dipoles, Magnetohydrodynamic Flow, Plasma Interactions, Space Plasmas

Scientific paper

Magnetospheres, which result from a solar wind flow parallel to the magnetic dipole, are expected for Uranus at its solstitial points and perhaps for the paleo-earth during the times of field reversal. A two-dimensional analytical model is presented for a pole-on magnetopause and the magnetospheric magnetic field line configuration, which employs a conformal mapping method.

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