Redefining flux ropes in heliophysics
Redefining flux ropes in heliophysics
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DOI：
10.3389/fspas.2023.1114838
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发表时间：
2023-03
期刊：
影响因子：
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通讯作者：
T. Nieves-chinchilla;Sanchita Pal;T. Salman;F. Carcaboso;S. Guidoni;H. Cremades;Ayris Narock;
中科院分区：
文献类型：
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作者：
T. Nieves-chinchilla;Sanchita Pal;T. Salman;F. Carcaboso;S. Guidoni;H. Cremades;Ayris Narock;
磁通绳表现为磁场线的扭曲束。它们在日球层中携带了大量的太阳质量。本文强调了进一步了解日球通量绳基础物理的必要性，并提供了通过新颖和必要的方法来显著改善通量绳研究现状的动力。它简要讨论了目前对通量绳形成和演化的理解，并总结了为理解日球层结构动力学而采取的策略。为解决这些问题而提出的挑战和建议预计将扩大我们对离我们最近的恒星、它的动力学以及它在其影响区域——日球层中的作用的深入了解。
Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance our understanding of the fundamental physics of heliospheric flux ropes and provides the motivation to significantly improve the status quo of flux rope research through novel and requisite approaches. It briefly discusses the current understanding of flux rope formation and evolution, and summarizes the strategies that have been undertaken to understand the dynamics of heliospheric structures. The challenges and recommendations put forward to address them are expected to broaden the in-depth knowledge of our nearest star, its dynamics, and its role in its region of influence, the heliosphere.