De Petris M, Gervasi M, Liberati F
Appl Opt. 1989 May 15;28(10):1785-92. doi: 10.1364/AO.28.001785.
The optical design of two Cassegrain-type telescopes of 1200- and 2500-mm primary mirrors has been studied by wobbling subreflectors to obtain differential measurements in wavelengths ranging from 300 microm to 2 mm of the spectrum. Wide chopping angles in the sky have been reached in spite of the large apertures and high secondary magnifications. Diffraction-limited performances are maintained by tilting the secondary mirror around the primary focus. This work is included in the TIR (Telescopio InfraRosso) project.
通过摆动副反射镜,对两台主镜直径分别为1200毫米和2500毫米的卡塞格伦式望远镜进行了光学设计研究,以获取光谱范围从300微米至2毫米的差分测量结果。尽管孔径大且二次放大率高,但仍实现了较大的天空斩波角。通过围绕主焦点倾斜副镜来保持衍射极限性能。这项工作包含在TIR(红外望远镜)项目中。