Abstract
The complexity of obtaining continuous series of precise, frequent, and reliable data on meteorological parameters makes it difficult to use the ground-based records on the muon component of cosmic rays. This work proposes to determine the temperature conditions of the atmosphere directly from the solution of a set of equations for cosmic ray variations. We demonstrate the possibility of, on the one hand, accounting for the temperature effect of the muon component without the use of aerological data and, on the other hand, diagnostics of the temperature conditions of the atmosphere from cosmic ray monitoring.
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