Short-period variations in cosmic-ray intensity
Journal Article
·
· Sov. Phys. - Usp. (Engl. Transl.); (United States)
The origin and propagation mechanisms of fluctuations in the cosmic rays observed by instruments on the ground, in the stratosphere, and in space are discussed. Recent experimental results on fluctuations at frequencies from 10/sup -3/ to 10/sup -6/ Hz are discussed. The primary cause of the statistically significant fluctuations in the cosmic rays is the scattering of charged particles of the cosmic rays by random inhomogeneities of the interplanetary magnetic field.
- Research Organization:
- Institute of Terrestrial Magnetism, the Ionosphere and Radio Wave Propagation, Academy of Sciences of the USSR, Troitsk (Moscow District)
- OSTI ID:
- 6450108
- Journal Information:
- Sov. Phys. - Usp. (Engl. Transl.); (United States), Journal Name: Sov. Phys. - Usp. (Engl. Transl.); (United States) Vol. 28:3; ISSN SOPUA
- Country of Publication:
- United States
- Language:
- English
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