Modeling of the auroral hiss spatial structure and comparison with the observed results

A. S. Nikitenko; Никитенко А. С.; Yu. V. Fedorenko; Федоренко Ю. В.; J. Manninen; Маннинен Ю.; O. M. Lebed; Лебедь О. М.; E. B. Beketova; Бекетова Е. Б.

doi:10.31857/S0367676522700259

Modeling of the auroral hiss spatial structure and comparison with the observed results

Autores: Nikitenko A.S.¹, Fedorenko Y.V.¹, Manninen J.², Lebed O.M.¹, Beketova E.B.³
Afiliações:
1. Polar Geophysical Institute
2. Sodankylä Geophysical Observatory
3. Murmansk Arctic State University, Branch in Apatity
Edição: Volume 87, Nº 1 (2023)
Páginas: 134-140
Seção: Articles
URL: https://rjpbr.com/0367-6765/article/view/654517
DOI: https://doi.org/10.31857/S0367676522700259
EDN: https://elibrary.ru/JVARNR
ID: 654517

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Resumo

We present the results of the auroral hiss propagation modeling from the source region to the ground and its comparison with the observed results. We analyzed propagation conditions explaining locality of the auroral hiss illuminated area observed on the ground. It is shown that quasielectrostatic waves with random amplitudes, phases and wavenormals directions representing the auroral hiss propagating to the ground form two wave beams in the meridional plane. The scattering of these waves at altitudes of 800–1300 km can cause the observed locality of the illuminated area.

Bibliografia

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