Ways to improve the current IRI ion composition model with regard to low solar activity and its extension to the plasmasphere

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F12%3A00426525" target="_blank" >RIV/68378289:_____/12:00426525 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Ways to improve the current IRI ion composition model with regard to low solar activity and its extension to the plasmasphere
Original language description
Knowledge of the ion composition in the outer ionosphere and plasmasphere is critically important for fully understanding the propagation of radio waves in this region and for the many applications that use ray-tracing through this region. The TTS-03 model currently used in the International Reference Ionosphere (IRI) it is restricted to altitudes below 2000km and is based on data from the solar activity interval F10.7 daily= 85 to 200. Thus it does not represent well the peculiarities of the ionosphereduring the very low solar activity years 2009 and 2010. By using newly available data from the satellite C/NOFS and recently restored data from the OGO-5 satellite we are working towards overcoming these shortcomings of the current IRI ion compistion model.
Czech name
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Czech description
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Project
<a href="/en/project/LG11032" target="_blank" >LG11032: COSPAR 2011-2013</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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