Physics
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..174a&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801
Physics
Heliosphere, Periodic Variations, Solar Cosmic Rays, Solar Oscillations, Long Term Effects, Solar Activity Effects, Sunspots
Scientific paper
The results of a statistical search for long-term pulsations of the solar cavity, applying the cyclic-variation analysis of Attolini et al. (1983) to the corrected Huancayo ion-chamber data of Forbush (1958) for the period 1937-1953 and to Climax neutron-chamber data for the period 1953-1979, are presented in graphs and characterized in terms of the time variation of the phase and amplitude stretching indices z(phi) and z(a). Phenomena observed include z(phi) and z(a) peaks at periods near 1 yr with a drift toward 1.3 yr near solar-activity minima, a second group of peaks near 2 yr with a phase inversion around 1958, a small fluctuation signature at 5 yr, and a correlation of cosmic-ray intensity and sunspot number at periods 10.5, 2, and 1.3 yr. with a delay of 6-8 mc.
Attolini M. R.
Cecchini Simone
Galli Marcello
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