In the paper, the mathematical equations for the output signals of the stellar meridian observation are presented via analysing the processes of the observation.
本文通过恒星子午观测过程的分析，给出了输出信号所应满足的数学关系式。
2
In the end, the applications of infrared CCD, ultraviolet CCD and weak-light CCD in the observation of sun magnetic field and sun stellar magnetic field are introduced.
本文最后还对红外CCD、紫外ccd、弱光CCD在太阳磁场测量和太阳恒星磁场观测的应用进行了介绍。
3
The output signals of the stellar meridian observation using a photon counter are obtained by means of combining the computed signals wiry recording noises.