Preferred Bartels days of high speed solar wind streams: An update |
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| Authors: | G. K. Rangarajan H. Mavromichalaki |
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| Affiliation: | (1) Indian Institute of Geomagnetism, Colaba, 400 005 Bombay, India;(2) Dept. of Physics, University of Athens, 10680 Athens, Greece |
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| Abstract: | Comparison of distribution of solar wind streams as a function of Bartels rotation days for two successive epochs indicates several significant differences. These are likely to be due to the differing nature of IMF and solar wind in the two solar cycles 20 and 21. |
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