Spectral Analysis of a Quiescent Filament

Spectral Analysis of a Quiescent Filament

We have determined principal plasma parameters in a filament by applying the appropriate cloud model to several observed spectral lines. Then we compared them to prominence models from the recent numerical NLTE modelling of Gouttebroze et al . (1993) (referred to as GHV). Some preliminary results of...

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Veröffentlicht in:International Astronomical Union Colloquium 1994, Vol.144, p.361-363
Hauptverfasser: Kotrč, P., Heinzel, P., Gorshkov, A. V., Kononovich, E. V., Kupryakov, Yu. A., Smirnova, O. B.
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Sprache:eng
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Zusammenfassung:We have determined principal plasma parameters in a filament by applying the appropriate cloud model to several observed spectral lines. Then we compared them to prominence models from the recent numerical NLTE modelling of Gouttebroze et al . (1993) (referred to as GHV). Some preliminary results of such an attempt are described and related problems are briefly discussed.
ISSN:0252-9211
DOI:10.1017/S0252921100025616