Published 1981
| Version v1
Book
Cosmic ray variations connected with the dynamics of solar activity longitudinal distribution
- 1. AN SSSR, Moscow. Fizicheskij Inst.
- 2. Leningrad Branch of Izmiran, Leningrad (USSR)
- 3. Moskovskij Gosudarstvennyj Univ. (USSR). Nauchno-Issledovatel'skij Inst. Yadernoj Fiziki
Description
The regular changes in the longitude distribution of solar activity after 1960 caused the solar activity variations with periods T=27-40 days. However, such changes cannot account for the increase in the mean period of the cosmic ray variations associated with the Sun's rotation up to 28.7+-0.3 days. The increase may probably be explained by the fact that the modulating factor appears predominantly at high heliographic latitudes or at high altitudes in the Sun's atmosphere rather than in the entire sunspot formation zone
Additional details
Publishing Information
- Publisher
- Commissariat a l'Energie Atomique.
- Imprint Place
- Paris, France
- ISBN
- 2-7272-0060-5
- Imprint Title
- Conference papers. 17. International cosmic ray conference, Paris, 13-25 July 1981
- Imprint Pagination
- 384 p.
- Journal Page Range
- v. 4 p. 68-71.
Conference
- Title
- 17. International cosmic ray conference.
- Dates
- 13 - 25 Jul 1981.
- Place
- Paris, France.
INIS
- Country of Publication
- France
- Country of Input or Organization
- France
- INIS RN
- 13655156
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC RADIATION; SOLAR ACTIVITY; VARIATIONS
- Descriptors DEC
- IONIZING RADIATIONS; RADIATIONS