谱线形成深度理论及其应用(Ⅲ):太阳矢量磁场结构的推导  

Theory of Line Formation Depth and Its Application (Ⅲ):Derivation of the Structure of Solar Vector Magnetic Fields

作　　者：届中权 丁有济 张霄宇 陈学昆 

出　　处：《天文学进展》1997年第4期303-311,共9页Progress In Astronomy

基　　金：国家自然科学基金;云南省科委应用基础研究基金

摘　　要：叙述了谱线形成深度理论在推导太阳矢量磁场空间结构上的应用，列举了有典型意义的工作，指出了用响应函数比用贡献函数导出的结果更好的原因以及它们的局限性．作为对比，也举例说明了不依赖于这种理论来推导矢量磁场结构的方法．The application of the theory of line formation depth to the dent,ation of the structure ofsolar magnetic fields is described and some typical samples are given. It is pointed out that it ismore excellent for the response function to derive the structure of the line parameters than forthe contribution function, However, the application of both functions have their limitations andthe reason is analyzed. In the comparison with such application, the methods independent of thetheory mentioned above are also given.

关 键 词：太阳 磁场 矢量磁场结构 谱线 深度理论 

分 类 号：P182.7[天文地球—天文学]