摘要
本文对1982.12.20拱形爆发日珥进行了数值模拟,并分析了前沿减速、热传导、辐射损失和加热诸因素对爆发日珥形成过程的影响。结果表明,拱形爆发日珥与冕拱的形成过程有截然不同的动力学性质。
The present paper presents a numerical modeling of the eruptive prominence on Dec. 20, 1982, based on one-dimensional hydrodynamical equations. The effect of various factors, such as front deceleration, thermal conduction, radiation loss and heating, on the formation of the eruptive prominence is preliminarily discussed. The result shows that arch eruptive prominences have completely different dynamic characters from coronal arches.
出处
《天文学报》
1986年第1期47-52,共6页
Acta Astronomica Sinica
