CAOSP abstracts, Volume: 52, No.: 3, year: 2022

Author(s): Nina, A.; Čadež, V.M.; Popović, L.Č.; Radovanović, M.
Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 52, no. 3, p. 132-141.
Date: 12/2022
Title: Influence of variations in the solar hydrogen Lyα radiation on the ionospheric D-region electron density during a year and solar cycle
Keyword(s): solar hydrogen Lyα line, ionospheric D-region, QIonDR model, VLF signals
Pages: 132 -- 141
DOI: https://doi.org/10.31577/caosp.2022.52.3.132
NASA ADS Abstract Service: 2022CoSka..52c.132N
Citation:
License: This work is licensed under a Creative Commons Attribution 4.0 International License

Abstract: The hydrogen Lyα radiation emitted from the Sun is the main source of photo-ionization processes and, consequently, of the free electron production in the ionospheric D-region. Variations in the intensity of the incoming Lyα radiation affect changes in the electron density and they show up as periodic daily and seasonal changes, and changes during a solar cycle. The Quiet Ionospheric D-Region (QIonDR) model describes these periodic changes. In this study, we analyse how changes during a year and changes in the smoothed daily sunspot number (both processes affect the intensity of incoming radiation in the D-region) affect the electron density changes related to quiet conditions. The presented modelling is based on the results of the QIonDR model obtained for the part of Europe defined by the positions of the very low frequency (VLF) signal transmitters ICV (Sardinia, Italy) and DHO (Lower Saxony, Germany), and the AWESOME (Atmospheric Weather Electromagnetic System for Observation Modeling and Education) receiver position (Belgrade, Serbia) in application of the QIonDR model on real signals.