Galactic cosmic-ray modulation effect by solar-wind streams.

Details Galactic cosmic-ray modulation effect by solar-wind streams. Galactic cosmic-ray modulation effect by solar-wind streams.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cajph..73..642e&link_type=abstract

Can. J. Phys., Vol. 73, No. 9 - 10, p. 642 - 646

Physics

3

Cosmic Rays: Solar Modulation, Cosmic Rays: Solar Wind

Scientific paper

Data, from the worldwide network of neutron monitors, recorded at Deep River, Hermanus, Rome, Tokyo, and Huancayo, over two solar cycles (Nos. 20 and 21) are analyzed to study the long-term variations of the solar diurnal variations as they relate to solar-wind speed. The median primary rigidities of response (Rm) for these detectors cover the range 16 GV ≤ Rm ≤ 33 GV. The author discusses the solar diurnal variations (amplitude and phase) of cosmic rays as a function of solar activity.

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