The quasi-stationary electromagnetic field in the solar wind

Details The quasi-stationary electromagnetic field in the solar wind The quasi-stationary electromagnetic field in the solar wind

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22....5a&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Jan.-Feb. 1982, p. 5-9. In Russian.

Computer Science

Interplanetary Magnetic Fields, Lines Of Force, Solar Wind, Electrodynamics, Kinematic Equations, Maxwell Equation

Scientific paper

Parker's (1958, 1963) kinematic model of the interplanetary field with ideal conductivity is examined. It is shown that Parker's assumption of the absence of the meridional component (Btheta = 0) is not a necessary one. Instead, in the general case the interplanetary magnetic field can have three components (Br, Btheta, and B sub phi).

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