Characterization of Artificial, Small-Scale, Ionospheric Irregularities in the High-Latitude F Region Induced by High-Power, High-Frequency Radio Waves of Extraordinary Polarization
- Authors: Blagoveshchenskaya N.F.1, Borisova T.D.1, Kalishin A.S.1, Yeoman T.K.2, Schmelev Y.A.1,3, Leonenko E.E.1,3
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Affiliations:
- Arctic and Antarctic Research Institute
- University of Leicester
- St. Petersburg State University of Aerospace Instrumentation
- Issue: Vol 59, No 6 (2019)
- Pages: 713-725
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157736
- DOI: https://doi.org/10.1134/S0016793219060045
- ID: 157736
Cite item
Abstract
The results of experimental studies of characteristics of artificial, small-scale, ionospheric irregularities in the high-latitude ionospheric F region caused by the controlled injection of high-power, high-frequency (HF) radio waves of extraordinary polarization (X mode) are presented. The experiments were carried out at the HF European Scientific Association (EISCAT)/Heating complex (Tromsø, northern Norway (69.6° N, 19.2° E)) in a wide range of heating frequencies (4–8 MHz) with an effective radiation power of 100 to 700 MW. It is shown that the generation of irregularities upon X heating occurs in the regular F region of the ionosphere under quiet magnetic conditions at heating frequencies both lower and higher than the critical frequency of the F2 layer. The rise and relaxation times of the irregularities, as well as the threshold powers of their excitation are determined. It is ascertained that the characteristics of irregularities upon X heating strongly depend on the heating frequency, the relationship between the heating frequency and the critical frequency of the F2 layer, and the conditions preceding the start of the heating cycle (“cold” start in the first X-heating cycle or subsequent X-heating cycles). The characteristics of irregularities upon exposure of the high-latitude ionospheric F region to high-power long radio waves of extraordinary (X mode) and ordinary (O mode) polarization are compared.
About the authors
N. F. Blagoveshchenskaya
Arctic and Antarctic Research Institute
Author for correspondence.
Email: nataly@aari.nw.ru
Russian Federation, St. Petersburg, 199397
T. D. Borisova
Arctic and Antarctic Research Institute
Email: nataly@aari.nw.ru
Russian Federation, St. Petersburg, 199397
A. S. Kalishin
Arctic and Antarctic Research Institute
Email: nataly@aari.nw.ru
Russian Federation, St. Petersburg, 199397
T. K. Yeoman
University of Leicester
Email: nataly@aari.nw.ru
United Kingdom, Leicester, LE1 7RH
Yu. A. Schmelev
Arctic and Antarctic Research Institute; St. Petersburg State University of Aerospace Instrumentation
Email: nataly@aari.nw.ru
Russian Federation, St. Petersburg, 199397; Saint Petersburg, 190000
E. E. Leonenko
Arctic and Antarctic Research Institute; St. Petersburg State University of Aerospace Instrumentation
Email: nataly@aari.nw.ru
Russian Federation, St. Petersburg, 199397; Saint Petersburg, 190000
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