Место издания:VEDA Publishing House of the Slovak Academy of Sciences Tatranska Lomnica
Первая страница:361
Последняя страница:363
Аннотация:The authors have determined principal plasma parameters in a filament by applying the appropriate cloud model to several observed spectral lines. Then they compared them to prominence models from the recent numerical NLTE modelling of Gouttebroze et al. (1993). Some preliminary results of such an attempt are described and related problems are briefly discussed.
Bibliographic Code: 1994scs..conf..361K