Magnetic fields and flares in the region CMP 20 September 1963
Magnetic fields and flares in the region CMP 20 September 1963
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DOI：
10.1007/bf00155163
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发表时间：
1968
期刊：
影响因子：
2.8
通讯作者：
G. Moreton;A. Severny
中科院分区：
文献类型：
--
作者：
G. Moreton;A. Severny
在9月9日的活动大斑点群经过期间，对30个耀斑的亮结在最开始的位置相对于高分辨率纵向分量图(H∥)和横向分量图(H⊥)的位置进行了为期7天的研究。耀斑亮结同时出现在磁极相反的区域，其中大部分与中性线H∥=0相邻，但与这条线不完全重合(图9)。横向磁场H⊥抑制了透镜状的耀斑结节和耀斑亮物质的运动。此外，耀斑与所谓的“分叉区”密切相关(83%)，这些区域发生横向分量的特定交叉(图4-5)。由关系式j=c/4πroth确定的最强(正或负)电流与耀斑结有很好的一致性(80%)。简要讨论了所得结果与已有的一些耀斑理论的关系。
The position of bright knots of 30 flares at their very beginning relative to the high-resolution isogauss maps of the longitudinal component (H∥) and maps of the transverse component (H⊥) of magnetic field are considered for seven days during the passage of the active and large spot group in Sept. 1963 (see Table I and maps on Figures 1–8).The flare bright knots occur simultaneously in regions of opposite magnetic polarity, and the majority of these knots are adjacent to neutral lineH∥= 0, although not coinciding precisely with this line (Figure 9). Lenticular form of flare knots and the motions of bright material of flares is restrained by transversal fieldH⊥. Also flares are closely associated (83%) with so-called ‘bifurcated regions’, where specific crossing of transverse components takes place (Figures 4–5). There is well-expressed (80%) coincidence of flare knots with the strongest (positive or negative) electric currents as determined from the relationj=c/4πrotH. The relation of results obtained to some existing theories of flares is briefly discussed.