冠状离层
Coronal partings
摘要：
“日冕分离”是一种特殊类型的准一维磁结构，通过日冕X射线和极紫外图像与太阳磁图的比较确定，其基本观测特性得到了研究。它们代表了单极大规模磁场内部相反极性的通道，由指向背景极性的相邻源的磁弧行形成。最重要的特征的partings进行了讨论。从进化和空间的角度来看，可以很自然地假设，分离可以转化为冕洞，反之亦然。确定了全局、相交和复杂的分割类。
英文摘要：
The basic observational properties of "coronal partings" -- the special type of quasi-one-dimensional magnetic structures, identified by a comparison of the coronal X-ray and EUV images with solar magnetograms -- are investigated. They represent the channels of opposite polarity inside the unipolar large-scale magnetic fields, formed by the rows of magnetic arcs directed to the neighboring sources of the background polarity. The most important characteristics of the partings are discussed. It can be naturally assumed that -- from the evolutionary and spatial points of view -- the partings can transform into the coronal holes and visa versa. The classes of global, intersecting, and complex partings are identified.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
