Remarkable anisotropic cosmic-ray intensity oscillation

Details Remarkable anisotropic cosmic-ray intensity oscillation Remarkable anisotropic cosmic-ray intensity oscillation

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980georl...7..613d&link_type=abstract

Geophysical Research Letters, vol. 7, Aug. 1980, p. 613-615.

Other

Anisotropy, Cosmic Rays, Harmonic Analysis, Radiant Flux Density, Data Processing, Forbush Decreases, Geomagnetism, Magnetic Disturbances, Periodic Variations, Universal Time

Scientific paper

A large cosmic ray intensity wave in which a single oscillation of the galactic flux with a peak-to-peak amplitude of about 4% and a period of approximately 27 hours, occurred on October 27-28, 1977. This unusual intensity profile was not associated with a classical Forbush decrease. Harmonic analysis in Universal Time of data from a global distribution of stations revealed that in each case the diurnal vector on October 27 differs significantly from those on other days before and after the event. The mechanism which produced this unusual oscillation is not yet understood.

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