耀斑脉冲相半经验模型

本文在文献9]的基础上,通过增加二个时刻的模型计算,给出了更完整的1983年2月3日2B级耀斑脉冲相色球半经验模型,从而进一步描述了脉冲相色球物理过程,并对耀斑动力学参量及能量过程作了初步讨论。 

Semiempirical Models of the Impulsive Phase of the Chromospheric Flare

In this paper,the detailed semiempirical models representing the chromospheric state during the impulsive phase of the 2B flare on Feb.3,1983 are proposed.The physical pictures of total evolutionary pattern of the impulsive phase of the flare are improved either quantitatively or qualitatively in comparison with the former work we did.Based on these semiempirical models,some dynamical properties and energy processes are also discussed.