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dc.creatorPetković, Dušan
dc.creatorOdalović, Oleg
dc.creatorNina, Aleksandra
dc.date.accessioned2022-11-23T14:02:00Z
dc.date.available2022-11-23T14:02:00Z
dc.date.issued2022
dc.identifier.issn1335-1842
dc.identifier.urihttps://www.astro.sk/caosp/Eedition/Abstracts/2022/Vol_52/No_3/index.html
dc.identifier.urihttps://www.astro.sk/caosp/Eedition/Abstracts/2022/Vol_52/No_3/pp116-125_abstract.html
dc.identifier.urihttps://grafar.grf.bg.ac.rs/handle/123456789/2802
dc.description.abstractRecent research indicates that the influence of the ionospheric D-region on the propagation of satellite signals cannot be ignored during the intense X-radiation emitted during solar X-ray flares. In this paper, we investigate the influence of changes in the solar hydrogen Lya radiation, which is manifested in variations of the D-region electron density and, consequently, the total electron content in this region, on the propagation of the Global Navigation Satellite System (GNSS) signals. We consider changes during a solar cycle and year, represented by the smoothed daily sunspot number and the day of year. The obtained results indicate that the influence of the D-region on these signals is not negligible for positioning with a single signal recorded by a single receiver during the period around the maximum of a solar cycle.sr
dc.language.isoensr
dc.publisherAstronomical Institute of the Slovak Academy of Sciencessr
dc.relationinfo:eu-repo/grantAgreement/MESTD/inst-2020/200002/RS//
dc.rightsopenAccesssr
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.sourceContributions of the Astronomical Observatory Skalnate Plesosr
dc.subjectsolar hydrogen Lya radiationsr
dc.subjecttotal electron contentsr
dc.subjectionospheresr
dc.subjectGNSS signal delaysr
dc.titleInfluence of the solar hydrogen Lya line on the GNSS signal delay in the ionospheric D-regionsr
dc.typearticlesr
dc.rights.licenseBY-NC-NDsr
dc.citation.epage125
dc.citation.issue3
dc.citation.rankM23~
dc.citation.spage116
dc.citation.volume52
dc.description.otherSPECIAL ISSUE ASTROPHYSICAL SPECTROSCOPY: A&M DATA - ATMOSPHEREsr
dc.identifier.doi10.31577/caosp.2022.52.3.116
dc.type.versionpublishedVersionsr


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