Hyde R A
Lawrence Livermore National Laboratory, Mail Stop L-477, 7000 East Avenue, Livermore, California 94550, USA.
Appl Opt. 1999 Jul 1;38(19):4198-212. doi: 10.1364/ao.38.004198.
The Eyeglass is a very large aperture (25-100-m) space telescope consisting of two distinct spacecraft, separated in space by several kilometers. A diffractive lens provides the telescope s large aperture, and a separate, much smaller, space telescope serves as its mobile eyepiece. Use of a transmissive diffractive lens solves two basic problems associated with very large aperture space telescopes; it is inherently launchable (lightweight, packagable, and deployable) it and virtually eliminates the traditional, very tight surface shape tolerances faced by reflecting apertures. The potential drawback to use of a diffractive primary (very narrow spectral bandwidth) is eliminated by corrective optics in the telescope s eyepiece; the Eyeglass can provide diffraction-limited imaging with either single-band (Deltalambda/lambda approximately 0.1), multiband, or continuous spectral coverage.
“眼镜”号是一台口径非常大(25 - 100米)的太空望远镜,由两个不同的航天器组成,在太空中相隔数公里。一个衍射透镜提供望远镜的大口径,而一个单独的、小得多的太空望远镜作为其可移动目镜。使用透射式衍射透镜解决了与超大口径太空望远镜相关的两个基本问题;它本质上是可发射的(重量轻、可包装且可展开),并且几乎消除了反射孔径所面临的传统的、非常严格的表面形状公差。通过望远镜目镜中的校正光学器件消除了使用衍射主镜(非常窄的光谱带宽)的潜在缺点;“眼镜”号可以提供单波段(Δλ/λ约为0.1)、多波段或连续光谱覆盖的衍射极限成像。