Peculiarities of Galactic Cosmic Ray (GCR) anisotropy variation in connection with the recurrent and sporadic Forbush effects

Details Peculiarities of Galactic Cosmic Ray (GCR) anisotropy variation in connection with the recurrent and sporadic Forbush effects Peculiarities of Galactic Cosmic Ray (GCR) anisotropy variation in connection with the recurrent and sporadic Forbush effects

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..289n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 289-292 (SEE N85-34991 23-93)

Physics

Anisotropy, Cosmic Rays, Forbush Decreases, Solar Flares, Solar Wind, Charged Particles, Geomagnetism, Interplanetary Medium

Scientific paper

It has been established, that the beginning of the change of vector of
Solar-diurnal anisotropy of Galactic Cosmic Rays (GCR) preceeds due to
disturbed region (DR) of Solar wind existing time of which is Tau or = 8
days. The meridional gradient delta theta eta of density during the
recurrent FD is valued.

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