Abstract
The observed frequencies of internnal gravity waves (IGWs) and their contribution to the variability of the brightness temperatures were determined on the basis of spectral analysis of the temporal dynamics of the thermal radio emission of the atmosphere at the frequencies 53.5, 54.0, 54.5, and 55.0 GHz. Methods for reconstructing from multifrequency measurements in the O2 lines the altitude distribution of the perturbation of the temperature of IGWs from the spectral amplitudes of their contribution to the brightness temperature were developed.
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