High-resolution astronomical spectrograph design method with a single echelle grating

被引:2
作者
Kukushkin, Dmitrii E. [1 ]
Sazonenko, Dmitrii A. [2 ]
Valyavin, Gennady G. [2 ]
Bakholdin, Alexey [1 ]
机构
[1] ITMO Univ, Appl Opt Ctr, 49 Kronverkskyi pr, St Petersburg 197101, Russia
[2] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
关键词
SOLAR-TELESCOPE; SPECTROMETER;
D O I
10.1364/AO.484192
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The paper presents a method for calculation of the main paraxial and energy parameters of a high-resolution astronomical spectrograph with a single echelle grating in a wide spectral range, without cross-dispersion elements. We consider two variants of the system design, namely, with a fixed grating (spectrograph) and with a movable grating (monochromator). Based on the analysis of the spectral resolution dependence on the echelle grating characteristics and the collimated beam diameter, the limits of the achievable maximum spectral resolution of the system are determined. The results obtained in this work can simplify the choice of the starting point for spectrograph designing. As an example of the presented method application design of the spectrograph for the Large Solar Telescopecoronagraph LST-3, operating in the spectral range of 390-900 nm, with spectral resolving power of R = 200,000 and minimum diffraction efficiency of the echelle grating Ig > 0.68, is considered. (c) 2023 Optica Publishing Group
引用
收藏
页码:3004 / 3015
页数:12
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