The existing methods of measurements of the magnetic fields of celestial bodies are mainly based on the Zeeman effect of magneto-sensitive spectral lines.

• 现有的天体磁场测量方法主要根据磁场敏感谱线的塞曼效应,而解释观测资料的理论基础是斯托克斯(Stokes)参数的形成及其转移方程的求解。