The galactic magnetic field derived from cosmic-ray electrons

H. Okuda, Y. Tanaka
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引用次数: 2

Abstract

An estimate of the galactic magnetic field is obtained by combining new results in the cosmic-ray electron spectruin and the recent radio data. The lower and upper limits of the magnetic field in the galactic disk are derived from two alternative models of field configuration; i.e. (0.5-1.0) X gauss near the solar system and (1.0-2.0) X gauss near the galactic center, respectively. The magnetic field in the halo is estimated to be larger than 2.5 X gauss.
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星系磁场来自宇宙射线电子
对银河系磁场的估计是通过结合宇宙射线电子能谱的新结果和最近的无线电数据得到的。银河系盘中磁场的下限和上限是由两种可供选择的磁场结构模型推导出来的;即太阳系附近为(0.5-1.0)X高斯,银河系中心附近为(1.0-2.0)X高斯。据估计,晕中的磁场大于2.5 X高斯。
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