Rozumenko V. Action of High-Energy Sources on Atmospheric and Space Radio Channels

Українська версія

Thesis for the degree of Doctor of Science (DSc)

State registration number

0521U101627

Applicant for

Specialization

  • 01.04.03 - Радіофізика

14-05-2021

Specialized Academic Board

Д 64.051.02

V.N. Karazin Kharkiv National University

Essay

The dissertation is concerned with solving a topical problem, the experimental and theoretical study of the impact of high-energy sources of natural and artificial origins on the characteristics of radio waves and on atmospheric and space radio channels that are used in radar, radio navigation, telecommunications, direction-finding radio system, etc. The goal of the dissertation is to study the main physical processes in the atmosphere and geospace that accompanied the impact of the Chelyabinsk and Kamchatka meteoroids on the environment, the influence of geospace storms, typhoons, earthquakes, launches of large rockets, and of the firing of orbital maneuvering thrusters, as well as the influence of high-power nanosecond radio emissions, which all are important for radio wave propagation and radio channel performance. The theoretical and experimental studies of disturbances in the atmospheric and space radio channels, radio wave characteristics, as well as in the parameters of the atmosphere and the ionosphere, which arise under the action of powerful natural (earthquakes, typhoons, large meteoroids, and geospace storms) and anthropogenic sources (main engine and orbital maneuvering system engine burns), have been conducted for many years. For the first time, numerical values for the disturbances in both radiowave and atmospheric-ionospheric parameters have been obtained. The Sun–interplanetary–medium–magnetosphere–ionosphere–atmosphere–Earth and Earth-atmosphere-ionosphere-magnetosphere formations are found to be complex open dynamic nonlinear stochastic systems. The basic principles of the systems paradigm have been developed. The demonstration has been given of the Chelyabinsk celestial body entry and explosion to cause appreciable (or large) disturbances in all geospheres. Using long-term observational data, local time and seasonal dependences of the magnitude, direction, zonal and meridional components of the wind velocity in the mesosphere have been obtained. Its magnitudes have been shown likely to be 10 – 80 m/s with 3 – 7 m/s error. The electron heating in the 30 – 60-km altitude range by an ultra-short pulse has been established to be essential even when the pulse length  = 1 ns and power P = 1 GW. The atmospheric breakdown in the 30 – 60-km altitude range begins to occur when P min =0.3–1.3 GW and the frequency f  10 GHz. The capability of observing the dynamic processes accompanying a moderate earthquake of Richter magnitude M  5.9 has been proved to be successful. The action of the super typhoon has been shown to be accompanied by enhancements in the wave activity in the atmosphere, when wave processes are generated with periods of 2 to 7 min and of 12–15 to 60–150 min. The coupling occurring in the atmosphere–upper-atmosphere–ionosphere has been confirmed to be carried by acoustic and gravity atmospheric waves. The greatest effect that the typhoon had on the ionosphere was revealed to occur when it had maximum energetics (8, 10, and especially 9 October 2019). A new classification of the ionospheric storms vs geomagnetic state has been advanced. The first group is comprised of strong ionospheric storms, which accompany strong magnetic storms (K p  8). The second group is comprised of strong ionospheric storms, which accompany minor magnetic storms. The third group is comprised of moderate ionospheric storms, which accompany strong magnetic storms. Naturally, moderate ionospheric storms accompany moderate magnetic storms. Experiments conducted for many years have revealed that disturbances exhibit three groups of speeds: 0.5 – 0.7 km/s and smaller, 2 – 3 km/s, and 10 – 25 km/s. They correspond to acoustic and atmospheric gravity waves, slow MHD, and gyrotropic waves, respectively. The experimental studies used the instrumentation located at the V. N. Karazin Kharkiv National University Radiophysical Observatory (MF radar, ionosonde, HF Doppler radar transmitting at vertical incidence, and fluxmeter magnetometer) and the multi-frequency multiple path HF Doppler radio system for oblique-incidence sounding of the ionosphere, which employs a software defined technology, at the Harbin Engineering University, PRC. In some cases, the incoherent scatter radar was employed (Institute for the Ionosphere of NAS and MES of Ukraine).

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