An Observationally Constrained Model of a Flux Rope that Formed in the Solar Corona
نویسندگان
چکیده
منابع مشابه
The Helicial Flux Rope Structure of Solar Filaments
According to J. B. Taylor’s relaxation theory for magnetized plasmas, helical flux ropes should be the fundamental building blocks of magnetism in the solar atmosphere. Although flux ropes are clearly ejected from the Sun, there has been some controversy about whether they exist in the sun’s atmosphere before ejection. The issue is important because of the need to understand how eruptions are i...
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It is generally believed that the magnetic free energy accumulated in the corona serves as a main energy source for solar explosions such as coronal mass ejections (CMEs). In the framework of the flux rope catastrophe model for CMEs, the energy may be abruptly released either by an ideal magnetohydrodynamic (MHD) catastrophe, which belongs to a global magnetic topological instability of the sys...
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چکیده ندارد.
15 صفحه اولErratum: Observation of an evolving magnetic flux rope before and during a solar eruption
flux rope before and during a solar eruption Jie Zhang, Xin Cheng & Ming-de Ding Nature Communications 3:747 doi: 10.1038/ncomms1753 (2012); Published 20 Mar 2012; Updated 7 Jun 2016 The HTML version of this Article previously published omitted Supplementary Movie 2. This has now been corrected in the HTML version of the Article; the PDF was correct from the time of publication. DOI: 10.1038/nc...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2018
ISSN: 2041-8213
DOI: 10.3847/2041-8213/aab15d