Magnetic fluctuation and cosmic ray diurnal variations

Details Magnetic fluctuation and cosmic ray diurnal variations Magnetic fluctuation and cosmic ray diurnal variations

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..159b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 159-162 (SEE N85-34991 23-93)

Physics

Anisotropy, Cosmic Rays, Diurnal Variations, Harmonic Analysis, Interplanetary Magnetic Fields, Magnetic Variations, Pitch (Inclination), Adiabatic Equations, Boltzmann Transport Equation, Magnetic Rigidity, Mean Free Path, Steady State

Scientific paper

A unified theory of cosmic ray diurnal variations has been proposed in which the first 3 harmonics of the cosmic ray daily variation all results from a single anisotropy produced by the combined effects of adiabatic focusing and anisotropic pitch angle scattering. The theoretical description of steady state cosmic ray anisotropies are simplified and improved. Preliminary results of a study of correlations between cosmic ray diurnal variations and the fluctuation characteristics of the interplanetary magnetic field are presented and discussed in light of the theory.

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