Towards better description of solar activity variation in IRI topside ion composition model
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F13%3A00426720" target="_blank" >RIV/68378289:_____/13:00426720 - isvavai.cz</a>
Result on the web
<a href="http://www.uwm.edu.pl/kaig/iri_workshop_2013/media/pdf/Truhlik.pdf" target="_blank" >http://www.uwm.edu.pl/kaig/iri_workshop_2013/media/pdf/Truhlik.pdf</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Towards better description of solar activity variation in IRI topside ion composition model
Original language description
Reported large differences between IRI and C/NOFS equatorial upp een IRI and C/NOFS equatorial upper transition height (1000km vs 700km)showed a problem of the IRI ion composition model (both TTS03 and DY85) which were not constructed for such a low solar activity like 2008-2009 solar minimum. We have proposed improvement of the TTS03 model called TBTion model based on absolute ion densities and which employs linear interpolation in log of absolute densities of individual ions.
Czech name
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Czech description
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Classification
Type
A - Audiovisual production
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
<a href="/en/project/LG11032" target="_blank" >LG11032: COSPAR 2011-2013</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
ISBN
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Place of publication
Olsztyn
Publisher/client name
University of Olsztyn
Version
1.
Carrier ID
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