ISSN 0474-8662. Information Extraction and Processing. 2017. Issue 45 (121)
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Detection the wave processes in atmosphere on the basis of ultraviolet supervision

Kalita B. I.
Lviv Centre of the Institute of Space Research NAS and SSA of Ukraine
Karatayeva L. M.
Lviv Centre of the Institute of Space Research NAS and SSA of Ukraine
Melnyk M. O.
Lviv Centre of the Institute of Space Research NAS and SSA of Ukraine

https://doi.org/10.15407/vidbir2017.45.077

Keywords: ultraviolet, acousto-gravitation waves, recorder of ultraviolet, dynamics of wave processes

Cite as: Kalita B. I., Karatayeva L. M., Melnyk M. O. Detection the wave processes in atmosphere on the basis of ultraviolet supervision. Information Extraction and Processing. 2017, 45(121), 77-82. DOI:https://doi.org/10.15407/vidbir2017.45.077


Abstract

It is proved that the electromagnetic ultraviolet radiation, penetrating through an atmosphere, can be recorded by the analysis of the direction, spatial form and the period of change of acoustogravitational waves. An ultraviolet radiation is partly dissipated into acousto-gravitational waves and its intensity acquires a time profile that coincides with the form of acousto-gravitational waves. The ultraviolet radiation fluxes are sensitive to the dynamics of wave processes in the atmosphere. Based on supervision the ultraviolet using the multichannel concentrator allow one to set the direction, spatial form and period of change of acousto-gravitational waves. Based on the supervision of the ultraviolet (UV) using the multichannel concentrator one can set the direction, spatial form and period of change of acousto-gravitational waves. The purpose of the research is to investigate the relation between UV photons in the range from 200 to 400 nm, solar activity, and processes in the atmosphere. Experiments showed that maximum daily variations of UV photons values in the range from 200 to 400 nm are out of phase with solar activity. One can suppose that a part of UV photons are the result of interaction of the galactic cosmic rays with atmosphere.


References

    1. Smolentsev, N.K. Basics of wavelet theory in MATLAB. DMK Press: Moscow, 2008; p 448. (in russian)

    2. Kramer, G.; Lidbetter, M. Stationary random processes. Mir: Moscow, 1968; p 39. (in russian)

    3. Rytov, S.M. Introduction to Statistical Radiophysics. Fizmatgiz: Moscow, 1976; p 494. (in russian)

    4. Dragan, Ya. P.; Rozhkov, V.A.; Javorskyj, I.N. Methods of probabilistic analysis of the rhythm of oceanic processes. Gidrometeoizdat: Leningrad, 1987; p 319. (in russian)

    5. Serebrennikov, M.G.; Pervozvansky, A.A. Detection of hidden frequencies. Nauka: Moscow, 1965; p 24. (in russian)

    6. Javorskyj I.N., On the estimation of the period of periodically correlated random processes. Otbor i peredacha informatcii. 1986; 73, 12-21. (in russian)