太阳不同纬度的自转差别造成了它的磁力线随时间扭曲,引起磁场回路(magnetic field loops) 因此,太阳上的温度绝不会低于3500摄氏度。人们又通过对温度和光的辩证关系的分析,也逐渐地掌握了太阳的温度。
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The reason for the high temperatures is unknown but thought to be related to the rapidly changing magnetic field loops that channel solar plasma.
其高温的原因至今是个未解之谜，但是人们认为这是与联通太阳的等离子体的快速变化的磁场循环有关。
The oppositely directed magnetic fields reconnected there, and half of the newly formed field lines shifted rapidly downward, where they stacked up on existing magnetic loops.
方向彼此相反的磁场在此处重连，半数新生成的磁力线迅速向底部移动，堆叠在既有的磁环上面。
The critical temperature of superconducting network which is composed of square unit loops in external magnetic field is solved by means of analytic method and numeric method I.
详细介绍了用解析解法和数值解法(即矩阵方程的多项式解法)分别求出了基元回路为正方形的“田”字形超导网络在外磁场中的临界温度，结果表明两种计算方法是完全等价的。
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