Non-recurrent geomagnetic disturbances from high-speed streams

Details Non-recurrent geomagnetic disturbances from high-speed streams Non-recurrent geomagnetic disturbances from high-speed streams

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983p%26ss...31..865b&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 31, Aug. 1983, p. 865-870.

Other

4

Geomagnetism, Magnetic Disturbances, Solar Activity Effects, Solar Wind Velocity, Periodic Variations, Solar Cycles, Solar Terrestrial Interactions, Twenty-Seven Day Variation

Scientific paper

It is shown that, at any phase of the solar activity cycle, the earth is circumflown mainly by high speed solar wind streams (M-streams). The attention is called to the fact that M-streams cause not only the well-known recurrent geomagnetic disturbances at the declining phase of solar cycle, but also numerous non-recurrent disturbances at all the other phases. The intensity and duration of a typical non-recurrent M-disturbance are less than those of a recurrent one.

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