In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 52, no. 3
A. Nina - V.m. Čadež - L.č. Popović - M. Radovanović
Detaily:
Rok, strany: 2022, 132 - 141
Jazyk: eng
Kľúčové slová:
solar hydrogen Lyα line, ionospheric D-region, QIonDR model, VLF signals
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2022/Vol_52/No_3/pp132-141_abstract.html
O článku:
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.
Ako citovať:
ISO 690:
Nina, A., Čadež, V., Popović, L., Radovanović, M. 2022. Influence of variations in the solar hydrogen Lyα radiation on the ionospheric D-region electron density during a year and solar cycle. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 52, no.3, pp. 132-141. 1335-1842. DOI: https://doi.org/10.31577/caosp.2022.52.3.132
APA:
Nina, A., Čadež, V., Popović, L., Radovanović, M. (2022). Influence of variations in the solar hydrogen Lyα radiation on the ionospheric D-region electron density during a year and solar cycle. Contributions of the Astronomical Observatory Skalnaté Pleso, 52(3), 132-141. 1335-1842. DOI: https://doi.org/10.31577/caosp.2022.52.3.132
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 12. 2022
Verejná licencia:
