Study of cosmic ray semidiurnal variations
Germogen F. Krymsky, П. А. Кривошапкин, С. К. Герасимова, P. Yu. Gololobov
Abstract
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Germogen F. Krymsky, П. А. Кривошапкин, С. К. Герасимова, P. Yu. Gololobov
Abstract
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On the basis of long-term registration of cosmic rays with the muon spectrograph at Yakutsk (62°01'N, 129°43'E) and multidirectional muon telescope at Nagoya (35°10'N, 136°58'E) the cosmic ray semidiurnal variation seasonal change and the change of cosmic ray semiduirnal variation with the solar activity level has been found. The modeling of the seasonal change has been made.
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On the basis of long-term registration of cosmic rays with the muon spectrograph at Yakutsk (62°01'N, 129°43'E) and multidirectional muon telescope at Nagoya (35°10'N, 136°58'E) the cosmic ray semidiurnal variation seasonal change and the change of cosmic ray semiduirnal variation with the solar activity level has been found. The modeling of the seasonal change has been made.
Key concepts: Cosmic ray, Spectrograph, Variation (astronomy), COSMIC cancer database, Physics, Telescope, Muon, Astronomy