Zobrazeno 1 - 10
of 17
pro vyhledávání: '"D. Šulić"'
Publikováno v:
Applied Sciences
Volume 11
Issue 16
Applied Sciences, Vol 11, Iss 7194, p 7194 (2021)
Volume 11
Issue 16
Applied Sciences, Vol 11, Iss 7194, p 7194 (2021)
Solar flares (SFs) and intense radiation can generate additional ionization in the Earth’s atmosphere and affect its structure. These types of solar radiation and activity create sudden ionospheric disturbances (SIDs), affect electronic equipment o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::257cf34d832f87b78bff0f0036bd86ed
Publikováno v:
Zbornik Radova: Geografski institut "Jovan Cvijić", Vol 67, Iss 3, Pp 221-233 (2017)
Zbornik Radova: Geografski institut "Jovan Cvijić", Vol 67, Iss 3 (2017)
Zbornik Radova: Geografski institut "Jovan Cvijić", Vol 67, Iss 3 (2017)
Solar flare X-ray energy can cause strong enhancements of the electron density in the Earth’s atmosphere. This intense solar radiation and activity can cause sudden ionospheric disturbances (SIDs) and further create ground telecommunication interfe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::271337bea79dd24959f40b844e9210df
https://doi.org/10.2298/ijgi1703221s
https://doi.org/10.2298/ijgi1703221s
Publikováno v:
Advances in Space Research. 57:1029-1043
In this paper we confine our attention to the analysis of amplitude and phase data acquired by monitoring VLF/LF radio signals emitted by four European transmitters during a seven-year period (2008–2014). All the data were recorded at a Belgrade si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76bf8dd532225c3d07a3f2764c197931
https://doi.org/10.1016/j.asr.2015.12.025
https://doi.org/10.1016/j.asr.2015.12.025
Autor:
Lj. M. Ignjatović, N. M. Sakan, Milan S. Dimitrijević, D. Šulić, Vladimir A. Srećković, D. Jevremović
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (1), pp.1131-1136. ⟨10.1093/mnras/stx3237⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (1), pp.1131-1136. ⟨10.1093/mnras/stx3237⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::231f65e1e67b13ba5b74cfdf82d51178
https://hal.archives-ouvertes.fr/hal-02293174
https://hal.archives-ouvertes.fr/hal-02293174
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms. 279:106-109
In this paper, we present a model for determination of a weakly time dependent effective recombination coefficient for the perturbed terrestrial ionospheric D-region plasma. We study consequences of a class M1.0 X-ray solar flare, recorded by GOES-15
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::740d4e737b7d39733539bf8a20670efc
https://doi.org/10.1016/j.nimb.2011.10.026
https://doi.org/10.1016/j.nimb.2011.10.026
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 69:775-792
VLF amplitude enhancements of the NAA/24.0 kHz signal (Maine, USA), registered by the Belgrade AbsPAL facility during solar flares, have been related to solar X-ray fluxes measured by the GOES-12 satellite. The observed regular appearance of the VLF
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::93efc9bb09ce9a3311e884e484218876
https://doi.org/10.1016/j.jastp.2007.01.012
https://doi.org/10.1016/j.jastp.2007.01.012
Akademický článek
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Akademický článek
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In this paper, we study the influence of solar flares on electron concentration in the terrestrial ionospheric D-region by analyzing the amplitude and phase time variations of very low frequency (VLF) radio waves emitted by DHO transmitter (Germany)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d2f458da758cac0bef5f8375cc1a12d
http://arxiv.org/abs/1204.4306
http://arxiv.org/abs/1204.4306
Publikováno v:
Scopus-Elsevier
NASA Astrophysics Data System
Open Astronomy, Vol 20, Iss 4, Pp 609-612 (2011)
NASA Astrophysics Data System
Open Astronomy, Vol 20, Iss 4, Pp 609-612 (2011)
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec9e685471828538d0d2ae7fc325aa0a
https://doi.org/10.1515/astro-2017-0346
https://doi.org/10.1515/astro-2017-0346