Published August 1985
| Version v1
Report
11- and 22-year variations of the cosmic ray density and of the solar wind speed
Creators
Description
Cosmic ray density variations for 17-21 solar activity cycles and the solar wind speed for 20-21 events are investigated. The 22-year solar wind speed recurrence was found in even and odd cycles. The 22-year variations of cosmic ray density were found to be opposite that of solar wind speed and solar activity. The account of solar wind speed in 11-year variations significantly decreases the modulation region of cosmic rays when E = 10-20 GeV
Additional details
Publishing Information
- Imprint Title
- Ninteenth International Cosmic Ray Conference. SH sessions, volume 4
- Journal Page Range
- vp.
- Report number
- N--85-34729
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19020579
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- COSMIC RAY FLUX; DATA PROCESSING; EXPERIMENTAL DATA; GEV RANGE 10-100; MODULATION; SOLAR ACTIVITY; SOLAR WIND; VARIATIONS; VELOCITY
- Descriptors DEC
- DATA; ENERGY RANGE; GEV RANGE; INFORMATION; NUMERICAL DATA; RADIATION FLUX; STELLAR ACTIVITY; STELLAR WINDS