Effects of solar magnetic field on cosmic rays

Details Effects of solar magnetic field on cosmic rays Effects of solar magnetic field on cosmic rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..457g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 457-460 (SEE N85-34729 23-92)

Other

Convective Flow, Curvature, Diffusion Coefficient, Galactic Cosmic Rays, Magnetic Field Inversions, Modulation, Rigidity, Solar Magnetic Field, Cosmic Ray Showers, Kinetic Energy, Solar Cycles

Scientific paper

Aspects of the problem of galactic cosmic ray propagation, including inversion of the solar total magnetic field and an analysis of data related to the heliomagnetic cycle are discussed. It is noted that the global structure of the solar magnetic field results in an additional flux of galactic cosmic rays generated by curvature and gradient drifts. An analysis of heliomagnetic cycle data shows that the latitudinal gradient results in a N-S asymmetry, with the amplitude of the effect growing with depth in the atmosphere. The inversion of the solar total magnetic field, drift effects, and other space distributions are found to contribute to a 22-year cycle of solar activity.

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