High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991–1996 |
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Authors: | Shrivastava Pankaj K Jaiswal KL |
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Institution: | (1) Department of Physics, Govt. New Science College, Rewa (M.P.), 486001, India;(2) Department of Physics, Govt. Degree College, Waidhan, Sidhi (M.P.)-, 486886, India |
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Abstract: | High-speed plasma streams identified in the solar wind measurements can be separated into two categories: coronal-hole-associated streams and flare-generated streams. Effects of these plasma streams on cosmic-ray intensity are studied for the period of 1991–1996. It is investigated that both of these high-speed solar wind plasma streams (CS and FGS) are found equally effective in producing the cosmic-ray intensity decrease on short-term basis. |
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