The large scale dynamics of the outer heliosphere and the long-term modulation of galactic cosmic rays

Details The large scale dynamics of the outer heliosphere and the long-term modulation of galactic cosmic rays The large scale dynamics of the outer heliosphere and the long-term modulation of galactic cosmic rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..193m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 193-196 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Heliosphere, Interplanetary Space, Solar Activity, Solar Magnetic Field, Diffusion Coefficient, Galactic Radiation, Gradients, Interplanetary Medium, Interstellar Radiation

Scientific paper

The network of cosmic-ray observatories reaching across the heliosphere has given new insight into the process of solar modulation, establishing that the decreases occur principally in the outer heliosphere and are produced by interplanetary flow systems; that the hysteresis effects appear to be produced by changes in the rigidity dependence of the diffusion coefficient and that the predicted effects on the cosmic ray gradients associated with the reversal of the solar magnetic field polarity are not observed.

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