SOME FEATURES OF CHROMOSPHERIC FLARES AND ITS CORRESPONDING ACTIVE REGIONS RESPONSIBLE FOR FORBUSH-EFFECT
Journal Article
·
· J. Phys. Soc. Japan
OSTI ID:4754963
- Vladimirsky
An attempt is made to reveal some features of solar flares and their active regions by analyzing flares of importance 2/sup +/ and more responsible for Forbush decrease. Data of IGY are used. It is shown that solid angle of outburst exciting Forbush-effect is the same as from magnetic storm data. A dependence between amplitude and duration of effect in cosmic rays and longitude of corresponding solar flare is revealed. The flares connected with Forbusheffect have larger duration, area in the maxima, and larger intensity in H/ sub aa/. There is no dependence between strengths of the magnetic field in active regions and amplitude of effect in cosmic rays. (auth)
- Research Organization:
- Originating Research Org. not identified
- NSA Number:
- NSA-17-012982
- OSTI ID:
- 4754963
- 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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