The influence of solar spectral lines on electron concentration in terrestrial ionosphere
arXiv:1201.2282 · doi:10.1515/astro-2017-0346
Abstract
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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- Diagnostics of plasma in the ionospheric D-region: detection and study of different ionospheric disturbance types
- Ionospheric D-region temperature relaxation and its influences on radio signal propagation after solar X-flares occurrence