Latitudinal variations of the power spectrum of cosmic-ray fluctuations

Details Latitudinal variations of the power spectrum of cosmic-ray fluctuations Latitudinal variations of the power spectrum of cosmic-ray fluctuations

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..368l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, May-June 1988, p. 368-372. In Russian.

Physics

Cosmic Rays, Geomagnetism, Power Spectra, Fluctuation Theory, Geomagnetic Pulsations, Latitude, Magnetic Rigidity

Scientific paper

The mean power spectra of cosmic-ray fluctuations at frequencies ranging from 0.000006 to 0.00166 Hz are calculated for different periods on the basis of neutron monitor and telescope data. Rigidity dependences of cosmic-ray fluctuations are obtained for 1977-1982. A divergence between theoretical and experimental results on the latitudinal variations of such fluctuations is detected which is due to a failure to account for asymptotic particle arrival directions in the range of small rigidities.

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