论文标题
色球环特征和太阳能中动力学的建模
Modeling of Chromospheric Features and Dynamics in Solar Plage
论文作者
论文摘要
色球是一个动态且复杂的层，所有相关的物理过程都发生在很小的时空尺度上。一些可以用作色球诊断的光谱线为我们提供了令人费解的信息，而这些信息很难解释而没有现实的理论模型。这些模型需要包含哪些关键成分？磁场对色球结构具有至关重要的作用。从太阳能磁盘和肢体上可见的色层动态纤维结构的无处不在的存在可以明显看出。本手稿中提出的数值实验说明了当前的建模状态。它们展示了我们的模型在多大程度上再现了各种色球层特征及其动力学。该出版物描述了不同成分对色层模型的影响，并为建立一对一模型提供了食谱。将这些模型与观察结果结合在一起，将洞悉太阳大气中发生的物理过程。
The chromosphere is a dynamic and complex layer where all the relevant physical processes happen on very small spatio-temporal scales. A few spectral lines that can be used as chromospheric diagnostics give us convoluted information that is hard to interpret without realistic theoretical models. What are the key ingredients that these models need to contain? The magnetic field has a paramount effect on chromospheric structuring. This is obvious from the ubiquitous presence of chromospheric dynamic fibrilar structures visible on the solar disk and at the limb. The numerical experiments presented in this manuscript illustrate the present state of modeling. They showcase to what extent our models reproduce various chromospheric features and their dynamics. The publication describes the effect different ingredients have on chromospheric models and provides a recipe for building one-to-one models. Combining these models with observations will provide insight into the physical processes that take place in the solar atmosphere.
