Magnetic field configuration of the heliosphere and spiral galaxies

Details Magnetic field configuration of the heliosphere and spiral galaxies Magnetic field configuration of the heliosphere and spiral galaxies

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253..552a&link_type=abstract

Astrophysical Journal, Part 1, vol. 253, Feb. 15, 1982, p. 552-555.

Astronomy and Astrophysics

Astrophysics

4

Galactic Structure, Heliosphere, Magnetic Field Configurations, Solar Magnetic Field, Spiral Galaxies, Magnetohydrodynamics, Solar Activity Effects, Solar Wind

Scientific paper

The magnetic field configuration of the heliosphere and spiral galaxies is investigated. Magnetic field lines emanating from a colatitude circle of theta equals 10 deg and 20 deg are presented, showing the lines wound up on a cone-shaped surface. The possibility that the solar current disk is considerably warped is discussed. The density and magnetic field intensity are higher along the spiral structure of the heliosphere, and it is speculated that the magnetic field configuration of a spiral galaxy has some similarity with that of the heliosphere.

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