Short-period variations in cosmic-ray intensity

Details Short-period variations in cosmic-ray intensity Short-period variations in cosmic-ray intensity

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985svphu.145..403d&link_type=abstract

(Uspekhi Fizicheskikh Nauk, vol. 145, Mar. 1985, p. 403-440) Soviet Physics - Uspekhi (ISSN 0038-5670), vol. 28, March 1985, p.

Physics

Cosmic Rays, Interplanetary Magnetic Fields, Periodicals, Solar Wind, Block Diagrams, Plasmas (Physics), Stratosphere, Wave Propagation

Scientific paper

The origin and propagation mechanisms of cosmic ray fluctuations observed by instruments on the ground, in the stratosphere, and in space are discussed. The study of such fluctuations by observing various secondary cosmic ray components is addressed. Fluctuational phenomena as studied by different ground instruments are compared. Fluctuations during Forbush decreases in the cosmic ray intensity at the earth are addressed, including the correlation between these fluctuations and those of the interplanetary magnetic field. Observations of cosmic ray fluctuations at the ground during solar flares are discussed. Fluctuation studies at various heights in the atmosphere, near the earth outside the atmosphere, and in interplanetary space are examined. The origin of the fluctuations and their possible relationship with processes in the interplanetary medium are discussed.

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