论文标题
通过其磁通量表征的磁场的作用和贡献对太阳大气的统计结构
The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere
论文作者
论文摘要
太阳能上层大气的异常加热是现代天文学的八个关键问题之一。此外，太阳大气的分层是太阳能物理学中出色的关键问题。在这项研究中，发现类似热蝴蝶的图案通过染色体延伸到光球中磁性蝴蝶模式的电晕。因此，我们建议介绍一词蝴蝶体，以描述三维气氛中的蝴蝶图。此外，我们讨论了不同层中所谓的极性亮度。发现它在统计上是在统计上，具有光球和色球球体中的太阳周期，而与电晕的太阳周期相同。因此，我们描述了不同磁通量强度的太阳磁元素的作用和关系，以解释太阳能体内太阳大气的统计结构。
The anomalous heating of the solar upper atmosphere is one of the eight key problems in modern astronomy. Moreover, the stratification of the solar atmosphere is an outstanding key-problem in solar physics. In this study, a hot butterfly-like pattern is found to run through the chromosphere to the corona lying right on top of the magnetic butterfly pattern of sunspots in the photosphere. We thus propose to introduce the term butterfly body to describe the butterfly diagram in the 3-dimensional atmosphere. Besides, we discuss the so-called polar brightening in different layers. It is found to be statistically in anti-phase with the solar cycle in the photosphere and the chromosphere, while in phase with the solar cycle in the corona. Accordingly, we describe the role and relationship of solar magnetic elements of different magnetic flux strengths to explain the statistical structuring of the solar atmosphere with the butterfly body over the solar cycle.
