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Bulletin of the Astronomical Institutes of the Netherlands最新文献

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The galactic magnetic field derived from cosmic-ray electrons 星系磁场来自宇宙射线电子
Pub Date : 1968-05-15 DOI: 10.1139/p68-315
H. Okuda, Y. Tanaka
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.
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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引用次数: 2
The formation of absorption bands and the distribution of photon optical paths in a scattering atmosphere 散射大气中吸收带的形成和光子光路的分布
Pub Date : 1963-10-01 DOI: 10.1086/148708
W. Irvine
Absorption lines and bands in scattering and absorbing medium elucidated by study of distribution of photon optical paths in scattering atmosphere
散射大气中光子光路分布的研究阐明了散射和吸收介质中的吸收谱线和吸收带
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引用次数: 59
On the origin of smoke particles in the interstellar gas (Errata : 10 146) 星际气体中烟雾粒子的起源(勘误表:10 146)
Pub Date : 1943-11-01 DOI: 10.1086/144669
D. Haar
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引用次数: 4
Formation of molecular hydrogen in interstellar space 星际空间中氢分子的形成
Pub Date : 1900-01-01 DOI: 10.1017/s0252921100118512
H. Knaap, C. V. D. Meijdenberg, J. Beenakker, H. V. Hulst
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引用次数: 3
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Bulletin of the Astronomical Institutes of the Netherlands
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