Modelling the emission of the outer solar atmosphere

该项目旨在改进从色球到日冕的外层太阳大气发射的模型，无论是在特定的太阳特征中还是在太阳作为恒星的情况下，因此也可以改进类太阳恒星的发射模型。改进将包括在模型中加入原子物理过程，以及根据对太阳大气、从X射线到近红外辐射的现有观测结果的详细分析，增加半经验约束。

The project aims at improving the modelling of the emission of the outer solar atmosphere, from the chromosphere to the corona, both in specific solar features and in the Sun as a star, so models of the emission of solar-like stars can also be improved. The improvements will involve adding atomic physics processes to the models, as well as adding semi-empirical constraints based on detailed analyses of available observations of the emission from the solar atmosphere, from the X-rays to the near-infrared.