一种利用会聚光束色散来观测远紫外恒星光谱的火箭搭载式光电分光光度计。

A rocket-borne photoelectric spectrophotometer using convergent beam dispersion to observe far ultraviolet stellar spectra.

作者信息

Sudbury G C

出版信息

Appl Opt. 1969 Oct 1;8(10):2013-7. doi: 10.1364/AO.8.002013.

DOI:10.1364/AO.8.002013

PMID:20072564

Abstract

The advantages of the Monk-Gillieson dispersion system using a plane grating off axis in the convergent beam from a paraboloidal collecting mirror have been applied to obtain low resolution photoelectric spectra of over forty bright stars in the 1500-3000 A region. Techniques of construction, alignment, calibration, and dc and pulse counting output data handling are described. The flight performance,in unstabilized Skylark rockets, is discussed.

摘要

蒙克 - 吉利森色散系统利用抛物面收集镜汇聚光束中的离轴平面光栅的优势，已被用于获取1500 - 3000埃区域内四十多颗亮星的低分辨率光电光谱。文中描述了该系统的构建、对准、校准以及直流和脉冲计数输出数据处理技术。还讨论了该系统在未稳定化的云雀火箭中的飞行性能。