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A HYDRODYNAMIC MODEL OF THE IMPULSIVE PHASE OF A SOLAR-FLARE LOOP
GAN, WQ ; FANG, C ; ZHANG, HQ
1991
Source PublicationASTRONOMY AND ASTROPHYSICS
ISSN0004-6361
Volume241Issue:2Pages:618-624
AbstractWith improvements in modeling of the chromospheric radiative loss and in the resolution of the transition region, together with the introduction of the mechanism of chromospheric heating by coronal soft X-rays, we have numerically simulated the hydrodynamic response of a solar flare loop to the thermal energy deposition around the top of the loop. Detailed evolutionary pictures have been obtained during the early stage of the impulsive phase for the conductively heated model, showing the fast heating of the flaring atmosphere, the formation and the development of chromospheric evaporation and condensation, the motion of the transition region, the consequences of the high-speed collision of evaporated material at the top, and so on. A comparison with previous work is also discussed.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8565
Collection期刊(老文献)
Recommended Citation
GB/T 7714
GAN, WQ,FANG, C,ZHANG, HQ. A HYDRODYNAMIC MODEL OF THE IMPULSIVE PHASE OF A SOLAR-FLARE LOOP[J]. ASTRONOMY AND ASTROPHYSICS,1991,241(2):618-624.
APA GAN, WQ,FANG, C,&ZHANG, HQ.(1991).A HYDRODYNAMIC MODEL OF THE IMPULSIVE PHASE OF A SOLAR-FLARE LOOP.ASTRONOMY AND ASTROPHYSICS,241(2),618-624.
MLA GAN, WQ,et al."A HYDRODYNAMIC MODEL OF THE IMPULSIVE PHASE OF A SOLAR-FLARE LOOP".ASTRONOMY AND ASTROPHYSICS 241.2(1991):618-624.
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