Variability of Ionospheric Parameters During Last Two Solar Cycles
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F16%3A00472424" target="_blank" >RIV/68378289:_____/16:00472424 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Variability of Ionospheric Parameters During Last Two Solar Cycles
Original language description
Ionosphere is highly variable system that reflects both the influence of the solar andngeomagnetic activity from above and neutral atmosphere from below. The response of thenionosphere varies during the solar cycle and from one cycle to the subsequent. We look at thenstatistical properties of the ionospheric data with respect to the phases of the solar cycle. Bynmean of the Wavelet Transform (CWT, XWT, WTC) we analyse coherency with solar andnneutral atmosphere parameters. Study involves ionospheric data from several European stationsn(critical frequencies, plasma drifts), stratospheric data, geomagnetic data together with solarnindices. The main goal of the study is to analyse in detail ionospheric response to the solarnforcing during last exceptional low solar minimum. n
Czech name
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Czech description
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Classification
Type
O - Miscellaneous
CEP classification
DG - Atmospheric sciences, meteorology
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA15-24688S" target="_blank" >GA15-24688S: Variability of the ionosphere and neutral atmosphere in midlatitudes</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů