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The Relationship of Magnetic Twist and Plasma Motion in a Magnetic Cloud

  • Authors: Ake Zhao, Yuming Wang, Hengqiang Feng, Bin Zhuang, Xiaolei Li, Hongbo Li, and Hong Jia

2019 The Astrophysical Journal 885 122.

  • Provider: AAS Journals

Caption: Figure 3.

Distribution of the average axial velocity in peeled flux ropes (panels (a)–(c)) and the axial velocity in flux rope layers (panels (d)–(f)). The red horizontal lines indicate the corresponding layer of the azimuthal magnetic flux, i.e., 0%–20%, 20%–40%, 40%–60%, 60%–80%, and 80%–100%. The results of the randomized noise test are shown in panels (b) and (e), and the test results for orientation of the MC axis are shown in panels (c) and (f).

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