反射狭缝光学元件的制造

N. Page, P. Lam, Robert E. Parks, J. Rodgers
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引用次数: 0

摘要

在设计地球遥感仪器可见光/红外成像光谱仪光学系统时,对反射狭缝光学元件提出了要求。在该光学系统中,反射狭缝位于施密特望远镜的焦点处,作为视场透镜、视场平坦器和双波段视觉/红外成像光谱仪的入口孔径。这些多重功能使反射狭缝成为光学设计中的关键元素。这一点以及对制造这种光学元件的能力的考虑,决定了在进一步开发光学设计之前,必须制造并验证面包板狭缝。光学系统的结构如图1所示。与通常的光谱仪不同的是,望远镜聚焦处的辐射(前光学)通过狭缝反射而不是透射到光谱仪中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Manufacture of a Reflecting Slit Optical Element
The requirement for a reflecting slit optical element resulted from design of a visual/IR imaging spectrometer optical system for an earth remote sensing instrument. In this optical system, the reflecting slit is located at the focus of a Schmidt telescope and serves as a field lens, field flattener, and entrance aperture to a two band visual/IR imaging spectrometer. These multiple functions make the reflecting slit a critical element in the optical design. This and concern for the ability to manufacture such an optical element dictated that a breadboard slit be manufacturer and verified before proceeding further with the development of the optical design. The configuration of the optical system is shown in Fig. 1. Unlike the usual spectrometer arrangement, radiation at the focus of the telescope (fore-optic) is reflected, instead of transmitted, by the slit into the spectrometer.
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