Change of cosmic ray anisotropy with solar activity

Details Change of cosmic ray anisotropy with solar activity Change of cosmic ray anisotropy with solar activity

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..155k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 155-158 (SEE N85-34991 23-93)

Computer Science

Anisotropy, Cosmic Rays, Energy Spectra, Interstellar Magnetic Fields, Magnetic Variations, Solar Activity, Atmospheric Temperature, Diurnal Variations, Ionization Chambers, Muons, Solar Wind

Scientific paper

Muon telescope data at various depths underground in Yakutsk within
energy range 10 to 300 GeV for 1957 to 1984 are analyzed. The 22-year
variation of the interplanetary magnetic field aligned component is
found. The variation is caused by interaction of heliomagnetosphere with
the local galactic field and interstellar wind.

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