Solar Flux Tube Models with Radiative Transfer

这项研究继续研究强磁通管的平衡结构，通过求解细磁通管近似下的静磁方程来计算。在过去的研究中，最重要的是包含了圆柱几何中的多流辐射传输，以及辐射能量传输和对流能量传输之间的连续转换。然而，没有考虑通量管对环境介质的影响，因此限制了以前的工作。这个效应对于研究水平温度变化，特别是在通量管和外部介质之间的界面上的温度变化是重要的。在这项研究中，PI将使用圆柱几何中的辐射传递的多维处理来包括这种影响。

This study continues investigating the equilibrium structure of intense magnetic flux tubes, as calculated by solving the magnetostatic equation sin the thin flux tube approximation. Most significant about past studies was the inclusion of multistream radiative transfer in cylindrical geometry, and the continuous transition between radiative and convective energy transport. The flux tube's influence on the ambient medium was not taken into account, however, thus limiting previous work. This effect is important for examining the horizontal temperature variation, especially at the interface between the flux tube and external medium. In this study, the PIs will use a multidimensional treatment of radiative transfer in cylindrical geometry to include this effect.