Relation of a typical structure of an interplanetary plasma flow with geomagnetic Pc1 pulsations

Details Relation of a typical structure of an interplanetary plasma flow with geomagnetic Pc1 pulsations Relation of a typical structure of an interplanetary plasma flow with geomagnetic Pc1 pulsations

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ge%26ae..17..110i&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 17, Jan.-Feb. 1977, p. 110-115.) Geomagnetism and Aeronomy, vol. 17, Aug. 1977, p. 71-74. Tran

Computer Science

Geomagnetic Pulsations, Magnetohydrodynamic Flow, Solar Flares, Solar Terrestrial Interactions, Solar Wind, Cold Plasmas, Correlation, Dense Plasmas, Magnetic Signatures, Magnetic Storms, Plasmapause, Satellite-Borne Instruments

Scientific paper

In the present paper, the structure of the plasma flow generated by the solar flare of February 2, 1969 is compared with Pc1 pulsations. The structure of the flow under consideration is representative of the 'typical structure' introduced by Ivanov (1975). Diagrams showing a distinct relationship between Pc1 pulsations and the hydromagnetic structure of the plasma flow, and the close association of the Pc1 characteristics with the elements of the substructure, are presented and discussed.

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