Wave disturbances in the ionosphere during a lasting solar activity minimum.

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Bibliographic Details
Title: Wave disturbances in the ionosphere during a lasting solar activity minimum.
Authors: Burmaka, V.1 viktor_burmaka@ukr.net, Chernogor, L.2 Leonid.F.Chernogor@univer.kharkov.ua
Source: Geomagnetism & Aeronomy. Apr2012, Vol. 52 Issue 2, p183-196. 14p.
Subject Terms: *Ionosphere, *Electrons, *Atmosphere, *Solar activity, *Ionization (Atomic physics)
Abstract: Using the Kharkov incoherent scatter radar, observations of wave disturbances in electron concentration N in the ionosphere at heights of 120-600 km are conducted. The measurements were carried out in the periods of the spring and fall equinoxes and winter and summer solstices. The height-time dependences of the absolute Δ N and relative Δ N/ N amplitudes of wave disturbances, as well as their spectral composition, were analyzed. It is shown that wave disturbances in the ionosphere with periods of 10-180 min were present at almost any time of the day and in all seasons. Their absolute and relative amplitudes varied from 6 × 10 to 6 × 10 m and from 0.01 to 0.5, respectively. The maximum values of Δ N and Δ N/ N were observed at a height of ∼200 km. The passage of the solar terminator changed substantially the wave disturbance parameters. [ABSTRACT FROM AUTHOR]
Database: Energy & Power Source
Description
Abstract:Using the Kharkov incoherent scatter radar, observations of wave disturbances in electron concentration N in the ionosphere at heights of 120-600 km are conducted. The measurements were carried out in the periods of the spring and fall equinoxes and winter and summer solstices. The height-time dependences of the absolute Δ N and relative Δ N/ N amplitudes of wave disturbances, as well as their spectral composition, were analyzed. It is shown that wave disturbances in the ionosphere with periods of 10-180 min were present at almost any time of the day and in all seasons. Their absolute and relative amplitudes varied from 6 × 10 to 6 × 10 m and from 0.01 to 0.5, respectively. The maximum values of Δ N and Δ N/ N were observed at a height of ∼200 km. The passage of the solar terminator changed substantially the wave disturbance parameters. [ABSTRACT FROM AUTHOR]
ISSN:00167932
DOI:10.1134/S001679321202003X