Manifestation of Magnetic Flux Ropes in the Structure of Solar Prominences

被引:0
作者
Filippov, B. P. [1 ]
机构
[1] Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere Radio Wave, Moscow 108840, Troitsk, Russia
基金
美国国家航空航天局;
关键词
CORONAL MASS EJECTIONS; ACTIVE-REGION; CHIRALITY; EVOLUTION; MOTIONS; FIELD;
D O I
10.1134/S0016793222600771
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The appearance of quiescent solar prominences most often resembles a wide curtain or a fence made of a vertical palisade. It is hard to imagine that such a structure can be connected or even formed by a magnetic flux rope, that is, a bundle of force lines twisted into a cylindrical helix, which sometimes clearly manifests itself in active region filaments. However, with a relatively small activation of the prominences, when the plasma composing them begins to move along the field lines, the structure of the magnetic flux rope can be discerned. An example of a quiescent prominence is shown, in which rotational motion is observed along helical trajectories outlining the flux rope. The rotation is clearly visible in the time-distance diagram, which is composed of narrow strips of images of the prominence along the trajectory of motion.
引用
收藏
页码:146 / 152
页数:7
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