The influence of solar spectral lines on electron concentration in terrestrial ionosphere

Details The influence of solar spectral lines on electron concentration in terrestrial ionosphere The influence of solar spectral lines on electron concentration in terrestrial ionosphere

2012-01-11

arxiv.org/abs/1201.2282v1

Baltic Astronomy, vol. 20, 609-612, 2011

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

Scientific paper

One of the methods of detection and analysis of solar flares is observing the time variations of certain solar spectral lines. During solar flares, a raise of electron concentration occurs in Earth's ionosphere which results in amplitude and phase variations of the recorded very low frequency (VLF) waves. We compared the data obtained by the analysis of recorded VLF signals and line spectra for different solar flares. In this paper we treated the DHO VLF signal transmitted from Germany at the frequency of 23.4 kHz recorded by the AWESOME system in Belgrade (Serbia) during solar flares in the period between 10:40 UT and 13:00 UT on 2011 April 22.

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