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The Analysis three Solar, Geomagnetic and Ionospheric Storms |
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Spomenko J. Mihajlović 1, Milena Cukavac1, Elra Hasanagić1, Spomenko J. Mihajlović 1, Rudi Čop2, Lazo Pekevski3, Jovica Jankovic1, Miodrag Rašić1 |
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(1) Republic Geodetic Authority, Bulevar Vojvode Mišića 39, 11000 Belgrade, Serbia, This email address is being protected from spambots. You need JavaScript enabled to view it. (2) Zavod Terra Viva, Sv. Peter 123, 6333 Sečovlje, Slovenija (3) University “Sts. Cyril and Methodius”, Seismological Observatory, Skopje, Macedonia |
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Solar-geophysical processes which determine changes in the index of solar-geomagnetic activity will be analyze in this study. Conditions in space or solar weather often can be determined by activity of CMEs emission (Coronal Mass Ejections), or by eruptions of coronal plasma and energy. Solar weather is changed as is changed number of registered solar storms, number and speed of magnetic clouds and if they were observed by moderate or intensive magnetic storms.These are changes in the speed and power of the Solar Wind, the appearance of intense solar flares, which are associated with the emission of Coronal Mass Ejections (CMEs) and the radiation of coronal holes (CH). The geo-effective impact of solar-geomagnetic disturbances will be analyzed on the case of three solar, geomagnetic and ionospheric storms (March 2013, March 2015 and September 2017). |
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