13-day oscillation in the cosmic-ray intensity

Details 13-day oscillation in the cosmic-ray intensity 13-day oscillation in the cosmic-ray intensity

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rbrfi..11..653f&link_type=abstract

Revista Brasileira de Fisica, vol. 11, Sept. 1981, p. 653-656.

Physics

Cosmic Rays, Interplanetary Magnetic Fields, Particle Flux Density, Solar Wind Velocity, Kp Index, Solar Rotation

Scientific paper

A relation is established between the 13-day cosmic ray intensity oscillation at Huancayo and Fredericksburg observatories, during 1973-1974, and the modulation associated with the regular, high-speed solar wind streams. It is shown that the trend of the wave for the geomagnetic index Kp is nearly in phase opposition with the cosmic ray intensity, in agreement with Wilcox and Ness (1965), and Fairfield and Ness (1967).

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