Interplanetary stream magnetism: Kinematic effects

Details Interplanetary stream magnetism: Kinematic effects Interplanetary stream magnetism: Kinematic effects

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974stin...7519099b&link_type=abstract

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Physics

Interplanetary Magnetic Fields, Kinematics, Solar Magnetic Field, Solar Wind, Azimuth, Magnetic Flux, Maxwell Equation, Solar Wind Velocity, Velocity Distribution

Scientific paper

The particle density, and the magnetic field intensity and direction are calculated in corotating streams of the solar wind, assuming that the solar wind velocity is constant and radial and that its azimuthal variations are not two rapid. The effects of the radial velocity profile in corotating streams on the magnetic fields were examined using kinematic approximation and a variety of field configurations on the inner boundary. Kinematic and dynamic effects are discussed.

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