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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.
  • 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. (en)
Title
  • Towards better description of solar activity variation in IRI topside ion composition model
  • Towards better description of solar activity variation in IRI topside ion composition model (en)
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  • Towards better description of solar activity variation in IRI topside ion composition model
  • Towards better description of solar activity variation in IRI topside ion composition model (en)
skos:notation
  • RIV/68378289:_____/13:00426720!RIV14-MSM-68378289
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(LG11032)
http://linked.open...vai/riv/dodaniDat
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  • 111356
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  • RIV/68378289:_____/13:00426720
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  • solar activity; ionosphere; ion composition model (en)
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  • [48A2620EDD49]
http://linked.open...i/riv/mistoVydani
  • Olsztyn
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  • University of Olsztyn
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http://linked.open...vavai/riv/projekt
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http://linked.open...iv/tvurceVysledku
  • Truhlík, Vladimír
  • Třísková, Ludmila
  • Bilitza, D.
http://linked.open...rzeVyzkumneZpravy
  • 1.
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