In this paper, some basic properties of polarization observations of radio pulsars and their theoretical explanation in the Inverse Compton Scattering (ICS) model are briefly reviewed.

• 但现有理论对众多观测事实尚无法给出完整的说明。综述了脉冲星的偏振观测特征，并利用逆康普顿散射模型对这些特性进行了解释。