Galactic cosmic ray currents and magnetic field irregularity degree in high-speed solar wind streams

Details Galactic cosmic ray currents and magnetic field irregularity degree in high-speed solar wind streams Galactic cosmic ray currents and magnetic field irregularity degree in high-speed solar wind streams

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..250k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 250-253 (SEE N85-34991 23-93)

Computer Science

Cosmic Rays, Galactic Radiation, Interplanetary Magnetic Fields, Solar Wind, Convection, Diffusion, Interplanetary Medium, Magnetic Field Configurations, Solar Activity

Scientific paper

Currents of galactic cosmic rays (GCR) obtained by global survey method are analyzed. The cases of almost total disappearance of GCR currents are compared with the results of direct measurements of the solar wind parameters. The conclusion is made on restricted application of the convective-diffusive mechanism of the GCR modulation by the solar wind during the occurrence of stationary and regular magnetic fields in the interplanetary medium.

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