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AN ATTEMPT OF ANALYZING COSMIC-RAY STORMS

Journal Article · · J. Phys. Soc. Japan
OSTI ID:4764893
It is shown that a beam model can explain the sequences of Forbush decreases and storm sudden commencements characteristic of cosmic-ray storms. It is also shown that there does not exist a regular 27-day period in the appearance of cosmic-ray storms associated with the return of active regions. (auth)
Research Organization:
Inst. of Physics, Uppsala
NSA Number:
NSA-17-012948
OSTI ID:
4764893
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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