Coronal holes, solar wind streams, and recurrent geomagnetic disturbances - 1973-1976

Details Coronal holes, solar wind streams, and recurrent geomagnetic disturbances - 1973-1976 Coronal holes, solar wind streams, and recurrent geomagnetic disturbances - 1973-1976

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...49..271s&link_type=abstract

Solar Physics, vol. 49, Aug. 1976, p. 271-278. ERDA-sponsored research;

Physics

67

Geomagnetic Pulsations, Satellite-Borne Instruments, Solar Activity Effects, Solar Corona, Solar Flares, Solar Wind Velocity, Interplanetary Magnetic Fields, Long Term Effects, Magnetospheric Instability, Periodic Variations, Spectroheliographs, Twenty-Seven Day Variation

Scientific paper

Observations of coronal holes, solar-wind streams, and geomagnetic disturbances during 1973-1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane.

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