Physical Processes in Solar and Stellar Coronal Loops

摘要：

Physical processes in coronal magnetic loops on the Sun and stars like particle acceleration, plasma heating, osciUations, and coronal mass ejection are con sidered. Paradoxes of particle acceleration mechanisms are discussed. Arguments in favor of acceleration in DC electric field are eiven We have shown that parametric resonance between loops and p-modes is a promising way to heat corona. A kink oscillation as a driver for ballooning instability of a loop is suggested.

关键词： magnetic loops solar and stellar coronae magnetic loops physical processes

作者: A.V.Stepanov V.V.Zaitsev

作者单位: Pulkovo Observatory,Saint Petersburg,Russia Institute of Applied Physics,Nizhny Novgorod,Russia

会议类型: 国际会议

会议名称: The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)

会议地点: 昆明

会议语种:英文

页码: 73-75

在线出版日期: 2008-08-03（万方平台首次上网日期，不代表论文的发表时间）