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磁通量喷发的大气响应Ⅰ.日冕物质喷射机制
引用本文:胡友秋,郑惠南. 磁通量喷发的大气响应Ⅰ.日冕物质喷射机制[J]. 中国天文和天体物理学报, 1991, 0(2)
作者姓名:胡友秋  郑惠南
作者单位:中国科学技术大学地球和空间科学系(胡友秋),中国科学技术大学地球和空间科学系(郑惠南)
摘    要:本文对盔状冕流底部磁通量喷发的大气响应进行数值模拟。数值结果表明:在喷发磁场的作用下,原冕流中的物质将受到压缩并向上运动,形成高密度亮环结构,同时在环的前方出现快磁声波,在环的下方出现低密度暗区。据此我们认为,磁通量喷发可能是触发环形日冕物质喷射的一种重要机制。

关 键 词:太阳  磁场  日冕物质喷射

Solar Atmospheric Responses to. Magnetic Flux Eruptions I. A Mechanism for Coronal Mass Ejections
Hu Youqiu Zheng Huinan. Solar Atmospheric Responses to. Magnetic Flux Eruptions I. A Mechanism for Coronal Mass Ejections[J]. Chinese Journal of Astronomy and Astrophysics, 1991, 0(2)
Authors:Hu Youqiu Zheng Huinan
Abstract:This paper presents a numerical simulation of the solar atmosheric response to a magnetic flux eruption from the base of a helmet streamer. The numerical results show that the material contained originally in the streamer is compressed and lifted upward by the erupting magnetic field, forming a high density bright loop. At the same time, fast magnetosonic waves occur in front of the loop, and a dark region with low density comes out below it. Based on these, we believe that the magnetic fltx eruption is probably an important mechanism in triggering loop-like coronal mass ejections.
Keywords:Sun-magnetic field-coronal mass ejection
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