Počet záznamů: 1
Solar activity impact on the Earth’s upper atmosphere
- 1.0389464 - ÚFA 2013 RIV FR eng J - Článek v odborném periodiku
Kutiev, I. - Tsagouri, I. - Perrone, L. - Pancheva, D. - Mukhtarov, P. - Mikhailov, A. - Laštovička, Jan - Jakowski, N. - Burešová, Dalia - Blanch, E. - Andonov, B. - Altadill, D. - Magdaleno, S. - Parisi, M. - Torta, J. M.
Solar activity impact on the Earth’s upper atmosphere.
Journal of Space Weather and Space Climate. Roč. 3, February (2013), A06/1-A06/21. ISSN 2115-7251. E-ISSN 2115-7251
Grant ostatní: COST(XE) ES0803
Institucionální podpora: RVO:68378289
Klíčová slova: ionosphere * solar activity * storm * total electron content * data analysis
Kód oboru RIV: DG - Vědy o atmosféře, meteorologie
Impakt faktor: 2.519, rok: 2013
http://www.swsc-journal.org/index.php?option=com_article&access=doi&doi=10.1051/swsc/2013028&Itemid=129
The paper describes results of the studies devoted to the solar activity impact on the Earth’s upper atmosphere and ionosphere, conducted within the frame of COST ES0803 Action. Aim: The aim of the paper is to represent results coming from different research groups in a unified form, aligning their specific topics into the general context of the subject. Methods: The methods used in the paper are based on data-driven analysis. Specific databases are used for spectrum analysis, empirical modeling, electron density profile reconstruction, and forecasting techniques. Results: Results are grouped in three sections: Medium- and long-term ionospheric response to the changes in solar and geomagnetic activity, storm-time ionospheric response to the solar and geomagnetic forcing, and modeling and forecasting techniques. Section 1 contains five subsections with results on 27-day response of low-latitude ionosphere to solar extreme-ultraviolet (EUV) radiation, response to the recurrent geomagnetic storms, long-term trends in the upper atmosphere, latitudinal dependence of total electron content on EUV changes, and statistical analysis of ionospheric behavior during prolonged period of solar activity. Section 2 contains a study of ionospheric variations induced by recurrent CIR-driven storm, a case-study of polar cap absorption due to an intense CME, and a statistical study of geographic distribution of so-called E-layer dominated ionosphere. Section 3 comprises empirical models for describing and forecasting TEC, the F-layer critical frequency foF2, and the height of maximum plasma density. A study evaluates the usefulness of effective sunspot number in specifying the ionosphere state. An original method is presented, which retrieves the basic thermospheric parameters from ionospheric sounding data.
Trvalý link: http://hdl.handle.net/11104/0218331
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