publication . Article . Preprint . 2016


Yuming Wang; Bin Zhuang; Qiang Hu; Rui Liu; Chenglong Shen; Yutian Chi;
Open Access
  • Published: 19 Aug 2016 Journal: Journal of Geophysical Research: Space Physics, volume 121, pages 9,316-9,339 (issn: 2169-9380, Copyright policy)
  • Publisher: American Geophysical Union (AGU)
Magnetic flux ropes (MFRs) are one kind of fundamental structures in the solar physics, and involved in various eruption phenomena. Twist, characterizing how the magnetic field lines wind around a main axis, is an intrinsic property of MFRs, closely related to the magnetic free energy and stableness. So far it is unclear how much amount of twist is carried by MFRs in the solar atmosphere and in heliosphere and what role the twist played in the eruptions of MFRs. Contrasting to the solar MFRs, there are lots of in-situ measurements of magnetic clouds (MCs), the large-scale MFRs in interplanetary space, providing some important information of the twist of MFRs. Th...
arXiv: Physics::Space PhysicsAstrophysics::Solar and Stellar Astrophysics
free text keywords: Magnetic field, Physics, Magnetic flux, Twist, Astrophysics, Interplanetary spaceflight, Flux, Heliosphere, Space physics, Coronal mass ejection, Astrophysics - Solar and Stellar Astrophysics, Physics - Plasma Physics, Physics - Space Physics
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publication . Article . Preprint . 2016


Yuming Wang; Bin Zhuang; Qiang Hu; Rui Liu; Chenglong Shen; Yutian Chi;