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2003•Unpublished venueRequires access

Evaluation of Gnevyshev Gap Effects on Cosmic Ray Modulation

M. Storini, Monica Laurenza, Z. Fujii, Fosso del Cavaliere, Piazzale Aldo Moro

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Abstract

Data from three neutron monitors (Climax, Rome, Huancayo/Haleakala) and from the Nagoya multidirectional muon telescope are used to investigate the energy dependence of the Gnevyshev Gap effects on galactic particles during solar activity cycle N. 22. Results suggest that the dual-peak shape of the modulation of galactic cosmic rays should be practically negligible for rigidity particles above 150 ± 20 GV. 1.

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What this paper is about

Data from three neutron monitors (Climax, Rome, Huancayo/Haleakala) and from the Nagoya multidirectional muon telescope are used to investigate the energy dependence of the Gnevyshev Gap effects on galactic particles during solar activity cycle N. 22. Results suggest that the dual-peak shape of the modulation of galactic cosmic rays should be practically negligible for rigidity particles above 150 ± 20 GV. 1.

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Available abstract

Data from three neutron monitors (Climax, Rome, Huancayo/Haleakala) and from the Nagoya multidirectional muon telescope are used to investigate the energy dependence of the Gnevyshev Gap effects on galactic particles during solar activity cycle N. 22. Results suggest that the dual-peak shape of the modulation of galactic cosmic rays should be practically negligible for rigidity particles above 150 ± 20 GV. 1.

Key concepts: Cosmic ray, Neutron monitor, Physics, Astrophysics, Rigidity (electromagnetism), Muon, Astronomy, COSMIC cancer database

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