Equations(2)and(6)and the corresponding discussion in the paper[Chin.Phys.Lett.42,056301(2025)]have been corrected.These modiffcations do not affect the results derived in the paper.
快速射电暴(Fast Radio Burst,FRB)的起源及周边磁环境特性,长期以来是天体物理学界的研究热点与核心谜题,而法拉第旋转量(Rotation Measure,RM)作为探测射电波传播路径上磁场与电子密度分布的关键物理量,其变化特征是破解这一谜题的重...快速射电暴(Fast Radio Burst,FRB)的起源及周边磁环境特性,长期以来是天体物理学界的研究热点与核心谜题,而法拉第旋转量(Rotation Measure,RM)作为探测射电波传播路径上磁场与电子密度分布的关键物理量,其变化特征是破解这一谜题的重要突破口.展开更多
文摘Equations(2)and(6)and the corresponding discussion in the paper[Chin.Phys.Lett.42,056301(2025)]have been corrected.These modiffcations do not affect the results derived in the paper.
