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Evaluation of payload performance for a sounding rocket vacuum ultraviolet spatial heterodyne spectrometer to observe C IV (lambda)(lambda)1550 emissions from the Cygnus Loop

机译:评估探空火箭真空紫外空间外差光谱仪的有效载荷性能,以观察天鹅座环的C IV(λ)(λ)1550排放

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摘要

The results of a project to develop a spatial heterodyne spectrometer (SHS) for a sounding rocket mission to study the Cygnus Loop, a prototypical middle-aged supernova remnant, are discussed. The goal was to obtain a radial velocity-resolved spectrum of the C IV (lambda)(lambda)1550 emission line from bright features of the Cygnus Loop, as a test for mapping the diffuse hot interstellar medium (ISM). A full Fourier-transform analysis of Cygnus Loop emission data is presented, showing lack of velocity-resolved C IV emission detection. Optics contamination is shown to be the most likely problem, and ways to eliminate this contamination for future SHS sounding rocket and satellite missions are discussed.
机译:讨论了开发空间外差光谱仪(SHS)进行探空火箭飞行任务以研究天鹅座环(一种典型的中年超新星遗留物)的项目的结果。目的是从天鹅座环的明亮特征中获得C IV(λ)(λ)1550发射线的径向速度分辨谱,以作为绘制散布的星际热介质(ISM)的测试。提出了对天鹅环排放数据的完整傅里叶变换分析,表明缺乏速度分辨C IV排放检测。光学污染被证明是最可能的问题,并讨论了在未来的SHS探测火箭和卫星任务中消除这种污染的方法。

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