Comparison of the meridional components of the solar and interplanetary magnetic fields

Details Comparison of the meridional components of the solar and interplanetary magnetic fields Comparison of the meridional components of the solar and interplanetary magnetic fields

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..123d&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 20, Jan.-Feb. 1980, p. 123-126.) Geomagnetism and Aeronomy, vol. 20, Aug. 1980, p. 77-79. Tran

Computer Science

Interplanetary Magnetic Fields, Solar Corona, Solar Magnetic Field, Solar Wind, Earth Orbits, Interplanetary Medium, Magnetic Induction, Magnetic Storms

Scientific paper

The present analysis deals with some experimental data on the solar magnetic fields at the level of the photosphere and in interplanetary space. A distinct difference is found between the behavior of the Bz-component of the IMF at the earth's orbit and the meridional component of the coronal magnetic field during the period from September through December 1965. Characteristic of the Bz-component are sudden frequent variations which differ drastically from the behavior of the coronal field. Bz tends to attain large values in the region of solar wind compression; however, the mechanism of this behavior is not clear.

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