Spectrum of cosmic-ray intensity fluctuations in the polar stratosphere in a solar activity minimum.

Details Spectrum of cosmic-ray intensity fluctuations in the polar stratosphere in a solar activity minimum. Spectrum of cosmic-ray intensity fluctuations in the polar stratosphere in a solar activity minimum.

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..128l&link_type=abstract

Geomagn. Aeron., Vol. 31, No. 1, p. 128 - 129

Physics

Cosmic Rays: Fluctuations, Cosmic Rays: Solar-Terrestrial Relations

Scientific paper

Calculations of the frequency spectrum of the intensity of galactic cosmic rays in the stratosphere according to data from a balloon experiment are presented. The experiment was carried out at the Tiksi Observatory (L = 5.57, φ = 65.°, Λ = 195.2°) on 27 - 28 July 1985 near minimum of the beginning of the 21st cycle of solar activity. A series of stable periods was established reliably: 2.9, 3.7, 4.7, 7.9, 14.9, ≡31.0, and 54.0 minutes. Some of the observed periods of the cosmic-ray fluctuations coincide with the periods of fluctuation of the Sun's dimensions.

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