This study deals with the short-term variations of cosmic ray intensity during the interval 1973-78. Daily means of high latitude neutron and meson monitors from the same station and those of a low latitude neutron monitor have been analysed using the Chree method of superposed epochs. The zero epoc
✦ LIBER ✦
High-speed solar wind streams of two different origins and cosmic-ray variations during 1980–1986
✍ Scribed by Pankaj K. Shrivastava; Ravindra P. Shukla
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 441 KB
- Volume
- 154
- Category
- Article
- ISSN
- 0038-0938
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A three-dimensional model for the calculation of cosmic-ray intensity of the Inuvik station during the 20th and 21st solar cycles is given. Especially we have studied the coefficient K of the used parameter of sunspot number in terms of high-speed solar-wind streams and have tried enough successfull