Cosmic-ray intensity variations in the 3-dimensional heliosphere

Details Cosmic-ray intensity variations in the 3-dimensional heliosphere Cosmic-ray intensity variations in the 3-dimensional heliosphere

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ssrv...52..121v&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 52, Feb. 1990, p. 121-194. Research supported by the Johns Hopkins University.

Physics

60

Heliosphere, Interplanetary Magnetic Fields, Solar Activity, Solar Cosmic Rays, Diurnal Variations, Interplanetary Medium, Magnetic Field Configurations, Solar Cycles, Solar Neighborhood, Voyager Project

Scientific paper

Studies of time and spatial variations of cosmic-ray intensity in the three-dimensional heliosphere are reviewed. Short-term cosmic-ray intensity decreases such as Forbush decreases and recurrent (corotating) decreases and long-term (11- and 22-year) variations are examined. Results from ground-based, Pioneer, and Voyager 1 and 2 observations of the radial and latitudinal gradients of cosmic rays are summarized. Also, long-term, 27-day, and transient variations in the diurnal anisotropy are discussed.

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