Published August 1985
| Version v1
Report
IMF-sense-dependent cosmic ray anisotropy produced from diffusion-convection in heliosphere
Creators
Description
It was demonstrated that an interplanetary magnetic field (IMF) sense dependent 2nd order anisotropy is produced by the diffusion convection of cosmic rays in the heliomagnetosphere. The result implies that the anisotropy cannot be expressed only by the pitch angle with respect to the IMF axis
Additional details
Publishing Information
- Imprint Title
- Ninteenth International Cosmic Ray Conference. SH sessions, volume 5
- Journal Page Range
- vp.
- Report number
- N--85-34991
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19053516
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANISOTROPY; ANNUAL VARIATIONS; CONVECTION; COSMIC RADIATION; DIFFUSION; INTERPLANETARY MAGNETIC FIELDS; SIMULATION; SOLAR ATMOSPHERE
- Descriptors DEC
- ATMOSPHERES; ENERGY TRANSFER; HEAT TRANSFER; IONIZING RADIATIONS; MAGNETIC FIELDS; RADIATIONS; STELLAR ATMOSPHERES; VARIATIONS