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High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991–1996

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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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Authors and Affiliations

  1. Department of Physics, Govt. New Science College, Rewa (M.P.), 486001, India

    Pankaj K. Shrivastava

  2. Department of Physics, Govt. Degree College, Waidhan, Sidhi (M.P.)-, 486886, India

    K.L. Jaiswal

Authors
  1. Pankaj K. Shrivastava
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  2. K.L. Jaiswal
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Shrivastava, P.K., Jaiswal, K. High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991–1996. Solar Physics 214, 195–200 (2003). https://doi.org/10.1023/A:1024080410101

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