首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >A comparison of the formation and evolution of magnetic flux ropes in solar coronal mass ejections and magnetotail plasmoids
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A comparison of the formation and evolution of magnetic flux ropes in solar coronal mass ejections and magnetotail plasmoids

机译:太阳日冕物质抛射和磁尾等离子体中磁通量绳的形成和演化的比较

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摘要

Solar coronal mass ejections and their interplanetary counterparts often show evidence of a twisted flux rope structure that is nearly identical, though of vastly different spatial scale, to plasmoids observed in the Earth's magnetotail. This paper reviews the current understanding of flux rope formation, morphology, and evolution in coronal mass ejections and magnetotail plasmoids. It highlights the idea that flux rope formation is a common space physics phenomenon and that the physical mechanisms responsible for flux rope formation occur over a wide range of plasma conditions wherever current sheets exist.
机译:太阳日冕物质抛射及其行星际对应物经常显示出扭曲的通量绳结构的证据,尽管其空间尺度差异很大,但它与在地球磁尾中观察到的等离子体均几乎相同。本文综述了目前对冠状物质抛射和磁尾等离子体中磁通绳的形成,形态和演化的理解。它强调了这样一种观念,即通量绳的形成是一种常见的空间物理学现象,而导致通量绳形成的物理机制发生在存在电流板的各种等离子体条件下。

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