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Cosmic Ray Signatures of Different Types of Solar Wind Streams
Published online by Cambridge University Press: 19 July 2016
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The earlier concept of average solar wind speed has changed with time. Besides quiet periods of low/average solar wind speeds, two different kinds of solar sources (solar flares and coronal holes) have been identified to produce high speed solar wind streams. In an earlier investigation, it was reported that the high speed streams associated to these sources produce distinctly different effects on the cosmic ray intensity (Venkatesan, et. al., 1982).
- Type
- VI. Chromospheric and Coronal Heating
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 259 - 260
- Copyright
- Copyright © Kluwer 1990
References
REFERENCES
Venkatesan, D., Shukla, A.K., and Agrawal, S.P. (1982), Cosmic ray intensity variations and two types of high speed solar streams, Solar Physics, 81, 375–81.Google Scholar
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