INTENSITY-TIME RELATIONSHIP OF COSMIC RAY UNUSUAL INCREASE, NOT CHARACTERIZED BY IMPACT ZONE EFFECTS
Journal Article
·
· J. Phys. Soc. Japan
OSTI ID:4764316
Under an assumption that the solar-produced cosmic rays are able to reach the earth only after the diffusion process through interplanetary space, the intensity-time relationsiup at an observed point is studied theoretically. By comparison of the observed intensity-time relationship with the theoretical one, it is possible to determine the initial time and the injection period of cosmic rays which are injected into interplanetary space from the source, to determine the diffusion constant with which the cosmic rays propagate in space, and to estimate the total number of cosmic rays injected during the injection period. (auth)
- Research Organization:
- Nagoya Univ., Japan
- NSA Number:
- NSA-17-012990
- OSTI ID:
- 4764316
- Journal Information:
- J. Phys. Soc. Japan, Journal Name: J. Phys. Soc. Japan Vol. Vol: 17: Suppl. A-II
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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