天文光谱学中的激光-2

H. Nieuwenhuijzen
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引用次数: 2

摘要

第一部分介绍了激光电子外差光谱技术。第二部分讨论了两个实验,一个是用激光和气体放电作为实验室光源,另一个是用激光和星光由一个大接收面积的望远镜收集。介绍了这些实验的结果,并描述了光学和电子仪器。从目前的结果来看,似乎可以使用光学混合技术对类星物体进行绝对单色通量和偏振测量。如果激光线移成为可能,就可以用高分辨率和低多普勒频移来分析标准恒星线。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Lasers in astronomical spectroscopy-2

In Part 1 electronic heterodyne spectroscopy using lasers was introduced. Part 2 discusses two experiments, one with a laser and a gas discharge as a laboratory source, the other with a laser and starlight collected by a telescope with a large receiving area. Results of these experiments are presented and optical and electronic instrumentation described. From results so far it seems possible to use the technique of optical mixing for absolute monochromatic flux and polarisation measurements on star-like objects. If laser line shifts become possible standard stellar lines could be analysed with high resolution and low Doppler shifts measured.

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