Comparative study of the features of propagation of ordinary and extraordinary modes of short waves in the ionosphere

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Resumo

The field parameters of ordinary and non-ordinary waves are compared each other while short waves propagate in the ionosphere.

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Sobre autores

K. Raubo

Immanuel Kant Baltic Federal University

Email: VEZakharov@kantiana.ru

Institute of High Technology

Rússia, Alexander Nevsky Str.14, Kaliningrad, 236041

V. Zakharov

Immanuel Kant Baltic Federal University

Autor responsável pela correspondência
Email: VEZakharov@kantiana.ru

Institute of High Technology

Rússia, Alexander Nevsky Str.14, Kaliningrad, 236041

Bibliografia

  1. Лукин Д. С., Палкин Е. А., Ипатов Е. Б. и др. // Сб. докл. XXV Всерос. открытой науч. конф. «Распространение радиоволн». Томск. 4–9 июля 2016. Томск: Изд-во ТУСУР, 2016. Т. 1. С. 40.
  2. Крюковский А. С., Лукин Д. С., Кирьянова К. С. // РЭ. 2012. Т. 57. № 9. С. 1028.
  3. Bilitza D., Altadill D., Zhang Y. et al. / // J. Space Weather and Space Climate. 2014. V. 4. A07.
  4. Hedin A. E. // J. Geophys. Res. 1991. V. 96. № A1. P. 1159.
  5. Захаров В. Е. // РЭ. 2019. Т. 64. № 6. С. 525.

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2. Fig. 1. The modulus of the Cartesian projection |fx| (curve 1), |fy| (curve 2) and |fz| (curve 3) of the polarization vector of an ordinary wave at f = 5 (a), 10 (b) and 15 MHz (c).

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3. Fig. 2. The module of the Cartesian projection |fx| (curve 1), |fy| (curve 2) and |fz| (curve 3) of the polarization vector of the extraordinary wave at f = 5 (a) and 10 MHz (b).

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4. Fig. 3. Results of calculations of the attenuation factor of an ordinary wave at f = 5 (a), 10 (b) and 15 MHz (c): curve 1 is the contribution from absorption, curve 2 is the contribution from beam divergence, curve 3 is the total attenuation factor.

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5. Fig. 4. Results of calculations of the attenuation factor of the extraordinary wave at f = 5 (a) and 15 MHz (b): curve 1 is the contribution from absorption, curve 2 is the contribution from the divergence of the rays, curve 3 is the total attenuation factor.

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