天体磁场
天体磁场-
斯托克斯参数与天体向量磁场测量
Stokes Parameters and Measurements of the Vector Magnetic Fields of Celestial Bodies
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偏振光谱的观测和研究是我们了解太阳表面以及遥远天体上磁场的基本方法。
Observations and researchs of polarized spectra are basic methods to know the magnetic field in solar atmosphere and other remote stars .
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弯曲磁场广泛存在于各类天体中的实际磁场，特别是激波中形成的磁场，虽然目前尚难以了解其形成过程，但用均匀场处理则肯定不真实。
Regarding the realistic magnetic fields widely exist in various cosmic sources , especially that formed behind the shock , although we still have no any idea of the formation process , the treatment in the uniform fields is definitely not correct .