Features of the Ionospheric Artificial Airglow Caused by Ohmic Heating and Plasma Turbulence-Accelerated Electrons Induced by HF Pumping of the Sura Heating Facility


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We present the results of studying the ionospheric F2 region airglow in the atomic-oxygen red line (λ = 6300Ǻ) when the ionosphere is pumped by high-power HF radio waves. Either thermal modulation of the background airglow brightness or, simultaneously with it, the red-line intensity enhancement were observed, depending on the ionospheric and plasma-wave parameters. Analysis of the red-line emission behavior makes it possible to separate the influence of the ohmic heating and acceleration of electrons by plasma turbulence on the airglow features.

Sobre autores

V. Klimenko

N. I. Lobachevsky State University of Nizhny Novgorod; Institute of Applied Physics of the Russian Academy of Sciences

Autor responsável pela correspondência
Email: klimenko@appl.sci-nnov.ru
Rússia, Nizhny Novgorod; Nizhny Novgorod

S. Grach

N. I. Lobachevsky State University of Nizhny Novgorod

Email: klimenko@appl.sci-nnov.ru
Rússia, Nizhny Novgorod

E.N. Sergeev

N. I. Lobachevsky State University of Nizhny Novgorod

Email: klimenko@appl.sci-nnov.ru
Rússia, Nizhny Novgorod

A.V. Shindin

N. I. Lobachevsky State University of Nizhny Novgorod

Email: klimenko@appl.sci-nnov.ru
Rússia, Nizhny Novgorod

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