On forced electric field oscillations in the ground layer of the atmosphere at gravity-wave frequencies of relativistic binary stellar systems

The work is devoted to the study of forced oscillations of the vertical component of the electric field in the surface layer of the atmosphere at double revolution frequencies of known relativistic binary star systems (RBS) with small eccentricity. Using complex time series, the imaginary part of which is the first finite difference of the original long-term time series, the spectral localization of eigenvectors of its Hermitian density matrix was studied. It has been shown (according to the Smirnov - Kolmogorov criterion) that the amplitude spectra of eigenvectors at the frequencies of gravitational radiation of the RBS have a significantly higher degree of spectral localization.

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