Origin of Both the Fast Hot Jet and the Slow Cool Jet from Magnetic Flux Emergence and Advection in the Solar Transition Region

摘要：

In the solar atmosphere,the jets are ubiquitous and found to be at various spatia-temporal scales.They are significant to understand energy and mass transport in the solar atmosphere.Recently,the high-speed transition region jets are reported from the observation.Here we conduct a numerical simulation to investigate the mechanism in their formation.Driven by the supergranular convection motion,the magnetic reconnection between the magnetic loop and the background open flux occurring in the transition region is simulated with a two-dimensional MHD model.

作者: 杨利平 Hardi Peter 何建森 涂传诒 张磊

作者单位: 中国科学院国家空间科学中心 北京 100190 马克斯普朗克研究中心 德国 北京大学 北京 100871

会议类型: 国内会议

会议名称: 2015年中国地球科学联合学术年会

会议地点: 北京

会议语种:英文

页码: 2711-2711

在线出版日期: 2015-10-11（万方平台首次上网日期，不代表论文的发表时间）