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
β¦ LIBER β¦
Effects of two types of solar wind streams on intensity variations of cosmic rays
β Scribed by R. S. Yadav; N. K. Sharma; Badruddin
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 347 KB
- Volume
- 151
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Cosmic ray intensity variations and two
β
D. Venkatesan; A. K. Shukla; S. P. Agrawal
π
Article
π
1982
π
Springer
π
English
β 436 KB
Cosmic ray modulation: Effects of high s
β
Badruddin
π
Article
π
1996
π
Springer Netherlands
π
English
β 829 KB
The effect of transverse-variation of so
β
Robert C. Newman
π
Article
π
1969
π
Elsevier Science
π
English
β 655 KB
High-speed solar wind streams of two dif
β
Pankaj K. Shrivastava; Ravindra P. Shukla
π
Article
π
1994
π
Springer
π
English
β 441 KB
Effects of active solar regions on the g
β
E. Antonucci; G. Cini Castagnoli; M. A. Dodero
π
Article
π
1971
π
Springer
π
English
β 454 KB
During the year 1969 two long-lived centres were active on the Sun at Carrington longitudes 50 ~ < L < 100 ~ and 250 ~ < L < 300 ~ About 80 % of the flares of importance I> 1B, produced during this period, originated in these zones. The solar modulation of galactic cosmic ray intensity during 1969
Areas of minimum intensity of soft X-ray
β
J. BochnΔ±ΜΔek; P. Hejda
π
Article
π
2002
π
Elsevier Science
π
English
β 497 KB