Anomalous increase of solar anisotropy above 150GV in 1981-1983

Details Anomalous increase of solar anisotropy above 150GV in 1981-1983 Anomalous increase of solar anisotropy above 150GV in 1981-1983

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..147u&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 147-150 (SEE N85-34991 23-93)

Physics

Anisotropy, Cosmic Rays, Diurnal Variations, Magnetic Rigidity, Muons, Solar Activity, Solar Magnetic Field, Amplitudes, Harmonic Analysis, Magnetic Variations

Scientific paper

An analysis was carried out of the observed data with Nagoya (surface). Misato (34mwe) and Sakashita (80mwe) multidirectional muon telescope, for the solar activity maximum period of 1978-1983. These data respond to primaries extending over the median rigidity range 60GV to 600GV. The observed amplitude at Sakashita station in 1981-1983 increased, especially in 1982; the amplitude is twice as large as that in 1978-1980, when those at Nagoya and Misato stations are nearly the same as those in 1978-1980. Uni-directional anisotropy is derived by the best fit method by assuming the flat rigidity spectrum with the upper cutoff rigidity Pu. The value of Pu obtained is 270GV in 1981-1983 and 150GV in 1978-1980.

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