The first four harmonics of the diurnal variation of galactic cosmic rays

Details The first four harmonics of the diurnal variation of galactic cosmic rays The first four harmonics of the diurnal variation of galactic cosmic rays

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..775d&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, Sept.-Oct. 1981, p. 775-780. In Russian.

Physics

2

Cosmic Rays, Diurnal Variations, Galactic Radiation, Spherical Harmonics, Distribution Functions, Kinetic Equations, Particle Motion

Scientific paper

The kinetic equation for the galactic-cosmic-ray distribution function is solved by expanding the distribution function into a spherical-harmonic series with respect to the angles between the particle-momentum direction and the direction of the regular magnetic field. The expansion coefficients are determined and used to analyze data on the diurnal, semidiurnal, eight-hour, and six-hour variations of cosmic-ray intensity.

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