天文学进展2016，Vol.34Issue(4)：403-414,12.DOI:10.3969/j.issn.1000-8349.2016.04.04
太阳低层大气辐射磁流体力学数值研究
Numerical Studies of the Radiative MHD Processes in the Lower Solar Atmosphere
摘要
Abstract
The lower solar atmosphere is a layer with a thickness of about 2 000 km, however, it is full of dynamics with different scales and various features with different characteristics. More importantly, it is the only path through which the energy inside the convection zone is transferred into the corona so as to heat the latter to 1 MK. In addition, the lower solar atmosphere is the only layer in the solar atmosphere where the magnetic field can be ac-curately measured so far. All these turn this thin layer into the spotlight of the radiative magnetohydrodynamic research. In this paper, we review all the progress both in numerical research and numerical methods, with the purpose to shed light on future development in this research area.关键词
太阳大气/光球/色球/太阳黑子/发电机/色球加热Key words
solar atmosphere/photosphere/chromosphere/sunspots/solar dynamo theory/chromospheric heating分类
天文与地球科学引用本文复制引用
陈鹏飞,丁明德,方成..太阳低层大气辐射磁流体力学数值研究[J].天文学进展,2016,34(4):403-414,12.基金项目
国家自然科学基金(11373023,11533005)；973(2014CB744203) （11373023,11533005）
