Radiation Hydrodynamics of the Solar Atmosphere

斯坦博士和霍利博士将为分析太阳大气中的动态现象建立模型并开发诊断方法。他们的理论计算将遵循辐射和等离子体运动在磁场存在和不存在的情况下响应驱动运动和快速能量注入的详细相互作用。线轮廓的分析，当与观测相比较时，将约束光球、色球和过渡区的动力学，并揭示所发现的运动类型。他们还将对这些大气区域的行为进行建模，以响应耀斑期间的能量注入，并将模型与观测结果进行比较。***

Stein, Robert AST 96-16886 Drs. Stein and Hawley will model and develop diagnostics for analyzing dynamic phenomena in the solar atmosphere. Their theoretical calculations will follow the detailed interaction of the radiation and plasma motions in response to driving motions and rapid energy injection both in the presence and in the absence of magnetic fields. The analysis of line profiles, when compared to observation, will constrain the dynamics of the photosphere, chromosphere, and the transition region and shed light on the types of motions found. They will also model the behavior of these regions of the atmosphere in response to energy injection during flares and compare models with observations. ***