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用于空间红外望远镜上的中红外光谱仪的像差校正凹面光栅。

Aberration-corrected concave grating for the mid-infrared spectrometer aboard the Infrared Telescope in Space.

作者信息

Onaka T

出版信息

Appl Opt. 1995 Feb 1;34(4):659-66. doi: 10.1364/AO.34.000659.

Abstract

A mechanically ruled aberration-corrected concave grating was developed for use in the low-resolution mid-infrared spectrometer aboard the cryogenically cooled Infrared Telescope in Space. The design and the performance testing of the grating are reported. The spectrometer requires a wide spectral range (4.5-11.7 µm) and a wide field of view (8 × 8 arcmin) with a low wavelength resolution (Δλ ≤ 0.3 µm). The aberration-corrected concave grating provides a flat focal plane with a small aberration in the spatial direction compared with those caused by the finite size of the entrance slit. It also permits a simple design for the spectrometer, which is advantageous for applications in space cryogenic instruments. The measurements of the wavelength resolution and the spatial resolution are shown to be in good agreement with the predicted performance. The diffraction efficiency of the grating is more than 80% at the blaze wavelength (6 µm) and fairly high (>30%) over the entire wavelength range in question. The grating produces polarization of less than 10% for λ < 6.4 µm and of 10-20% for 6.7 µm <λ 9.7 µm. These results indicate the potential applicability of this type of grating to the wide-field IR spectroscopic observations.

摘要

为用于搭载在太空低温冷却红外望远镜上的低分辨率中红外光谱仪,研制了一种机械刻划的像差校正凹面光栅。报告了该光栅的设计和性能测试情况。该光谱仪需要宽光谱范围(4.5 - 11.7微米)和宽视场(8×8角分),且波长分辨率低(Δλ≤0.3微米)。与由有限尺寸的入射狭缝所引起的像差相比,像差校正凹面光栅在空间方向上提供了一个像差小的平面焦面。它还允许光谱仪采用简单的设计,这对于太空低温仪器中的应用是有利的。波长分辨率和空间分辨率的测量结果与预测性能吻合良好。该光栅在闪耀波长(6微米)处的衍射效率超过80%,在所讨论的整个波长范围内相当高(>30%)。对于λ < 6.4微米,该光栅产生的偏振小于10%;对于6.7微米 < λ < 9.7微米,偏振为10 - 20%。这些结果表明这种类型的光栅在宽视场红外光谱观测中的潜在适用性。

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