Hydromagnetic precursors of flare streams of interplanetary plasma

Details Hydromagnetic precursors of flare streams of interplanetary plasma Hydromagnetic precursors of flare streams of interplanetary plasma

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..489g&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, May-June 1984, p. 489-491. In Russian.

Physics

1

Cosmic Plasma, Interplanetary Medium, Magnetohydrodynamic Waves, Planetary Magnetic Fields, Plasma-Electromagnetic Interaction, Space Plasmas, Geomagnetic Pulsations, Magnetic Field Configurations, Magnetic Flux, Magnetic Storms, Sudden Storm Commencements

Scientific paper

The hydromagnetic-precursor hypothesis states that, before a flare stream reaches the magnetosphere, specific magnetic-field oscillations are observed which are due to the penetration into the magnetosphere of hydromagnetic waves preceding the flare stream. This paper gives a theoretical description of this phenomenon and examines relevant experimental data. It is noted that flare-stream precursors may be sought in geomagnetic pulsations preceding sudden storm commencements.

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