Identification of high-velocity streams and coronal holes by means of geomagnetic pulsations

Details Identification of high-velocity streams and coronal holes by means of geomagnetic pulsations Identification of high-velocity streams and coronal holes by means of geomagnetic pulsations

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..102b&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 20, Jan.-Feb. 1980, p. 102-105.) Geomagnetism and Aeronomy, vol. 20, Aug. 1980, p. 64-66. Tran

Physics

Coronal Holes, Geomagnetic Pulsations, Solar Physics, Solar Wind Velocity, Equatorial Atmosphere, Interplanetary Magnetic Fields, Solar Activity Effects

Scientific paper

The relationship between geomagnetic micropulsation patterns and high-speed streams from coronal holes and other sources is investigated for the period of diminishing solar activity and for the activity minimum. Micropulsation classes are used to relate the streams to specific sources. The analysis of the micropulsations provides a way to classify high-speed streams.

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