Abstract
Seasonal changes in the semidiurnal variation of cosmic rays and their changes with the level of solar activity are discovered as a result of the long-term recording of cosmic rays by the spectrograph in Yakutsk (62°01′ N, 129°43′ E) and multidirectional muon telescope at Nagoya (35°10′ N, 136°58′ E). Seasonal changes are simulated using mechanisms proposed earlier by the authors.
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