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SEMIEMPIRICAL FLARE MODELS WITH CHROMOSPHERIC CONDENSATION
GAN, WQ ; RIEGER, E ; FANG, C
1993
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume416Issue:2Pages:886-892
AbstractUsing Halpha line profiles observed for two flares, we have constructed series of semiempirical models with chromospheric condensation. From the semiempirical point of view, it is shown for the first time that chromospheric condensations are responsible for the Halpha line asymmetries, not only for the red-asymmetry, but also for the blue-asymmetry with a central reversal. The properties of the condensation and its calculated evolutionary tendency seem to be consistent with the results of current hydrodynamical models of solar flares. The results also show that for the first flare, the Halpha can be explained merely by introducing the condensation without any need to heat the chromosphere, while for the second flare, the condensation has to overlap a heated chromosphere.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8523
Collection期刊(老文献)
Recommended Citation
GB/T 7714
GAN, WQ,RIEGER, E,FANG, C. SEMIEMPIRICAL FLARE MODELS WITH CHROMOSPHERIC CONDENSATION[J]. ASTROPHYSICAL JOURNAL,1993,416(2):886-892.
APA GAN, WQ,RIEGER, E,&FANG, C.(1993).SEMIEMPIRICAL FLARE MODELS WITH CHROMOSPHERIC CONDENSATION.ASTROPHYSICAL JOURNAL,416(2),886-892.
MLA GAN, WQ,et al."SEMIEMPIRICAL FLARE MODELS WITH CHROMOSPHERIC CONDENSATION".ASTROPHYSICAL JOURNAL 416.2(1993):886-892.
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