A POSSIBLE MECHANISM FOR THE METEOR-CORRELATED VARIATION IN THE COSMIC-RAY INTENSITY.
Journal Article
·
· Sov. Astron. AJ (Engl. Transl.) 13: 1044-6(May-Jun 1970).
OSTI ID:4128817
- Research Organization:
- Ioffe Inst. of Physics and Tech., Moscow
- NSA Number:
- NSA-24-030176
- OSTI ID:
- 4128817
- Journal Information:
- Sov. Astron. AJ (Engl. Transl.) 13: 1044-6(May-Jun 1970)., Other Information: Orig. Receipt Date: 31-DEC-70; Related Information: Translated from Astron. Zh.; 46: 1330-2(Nov-Dec 1969).
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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OSTI ID:4128817
Related Subjects
N32300* -Physics-Cosmic Radiation
N32150 -Physics- Astrophysics-Solar Phenomena
ELECTRIC CHARGES
INTERPLANETARY SPACE
MAGNETIC FIELDS
METEORS
PRIMARY COSMIC RADIATION
SOLAR WIND
ULTRAVIOLET RADIATION
VARIATIONS
X RADIATION
SOLAR DISTURBANCES/cycle of
effects on meteor- correlated cosmic-ray intensity variations
(T)
COSMIC RADIATION/intensity variation of
mechanism for meteor-correlated
(T)
METEORS/effects of streams of
on cosmic-ray intensity variation
(T)
N32150 -Physics- Astrophysics-Solar Phenomena
ELECTRIC CHARGES
INTERPLANETARY SPACE
MAGNETIC FIELDS
METEORS
PRIMARY COSMIC RADIATION
SOLAR WIND
ULTRAVIOLET RADIATION
VARIATIONS
X RADIATION
SOLAR DISTURBANCES/cycle of
effects on meteor- correlated cosmic-ray intensity variations
(T)
COSMIC RADIATION/intensity variation of
mechanism for meteor-correlated
(T)
METEORS/effects of streams of
on cosmic-ray intensity variation
(T)