Variability of the magnetic field in high-velocity streams of the solar wind

Details Variability of the magnetic field in high-velocity streams of the solar wind Variability of the magnetic field in high-velocity streams of the solar wind

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..477d&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, May-June 1983, p. 477-479. In Russian.

Computer Science

5

Interplanetary Magnetic Fields, Solar Wind Velocity, Solar Activity Effects, Solar Magnetic Field

Scientific paper

The degree of regularity of the magnetic field in high-velocity streams of the solar wind is assessed in order to determine whether the properties of the magnetic field in such streams differ appreciably from magnetic-field properties in the quiet solar wind. An analysis of IMF variability shows that the field-strength modulus in high-velocity streams varies appreciably less than in the quiet solar wind. This result is found to be associated with the origin of the high-velocity streams; the field structure produced in such streams is less complex, i.e., more regular, than in the quiet solar wind.

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