Synthesis and analysis of an aplanatic mirror-lens system with axial symmetry
- 作者: Venetsky A.S.1, Kaloshin V.A.1, Tuan T.2
-
隶属关系:
- Kotelnikov Institute of Radio Engineering and Electronics RAS
- Moscow Institute of Physics and Technology (National Research University)
- 期: 卷 69, 编号 6 (2024)
- 页面: 533-540
- 栏目: ЭЛЕКТРОДИНАМИКА И РАСПРОСТРАНЕНИЕ РАДИОВОЛН
- URL: https://ter-arkhiv.ru/0033-8494/article/view/650661
- DOI: https://doi.org/10.31857/S0033849424060042
- EDN: https://elibrary.ru/IKDFWS
- ID: 650661
如何引用文章
详细
The problems of synthesis and analysis of an axisymmetric aplanatic mirror-lens system that transforms the spherical front of a source into a flat one are considered. Two methods have been developed for solving the problem of synthesizing the system’s generatrices: using a numerical procedure and the Kelleher formula, and also by reducing it to a differential equation with a retarded argument. Formulas are obtained for the eikonal in the aperture of the system when the source is displaced from the focus. The dependence of the mean square aberration of the eikonal on the system parameters has been studied and their optimal values have been found.
作者简介
A. Venetsky
Kotelnikov Institute of Radio Engineering and Electronics RAS
编辑信件的主要联系方式.
Email: red@cplire.ru
俄罗斯联邦, Mokhivaya Str. 11, build. 7, Moscow, 125009
V. Kaloshin
Kotelnikov Institute of Radio Engineering and Electronics RAS
Email: red@cplire.ru
俄罗斯联邦, Mokhivaya Str. 11, build. 7, Moscow, 125009
Trinh Van Tuan
Moscow Institute of Physics and Technology (National Research University)
Email: red@cplire.ru
俄罗斯联邦, Institutskii Lane 9, Dolgoprudny, Moscow region, 141700
参考
- Schmidt B. //Centralzeitung fur Optik und Mechanik. 1931. V. 52. № 2. P. 25.
- Максутов Д. Д. Астрономическая оптика. 2-е изд. Л.: Наука, 1979.
- Михельсон Н. Н. Оптика астрономических телескопов и методы ее расчета. М.: Физматлит, 1995.
- Калошин В. А., Фролова Е. В. // Журн. радиоэлектроники. 2015. № 12. http://jre.cplire.ru/jre/dec15/19/text.pdf.
- Kelleher K. S.// J. Appl. Phys. 1950. V. 21. № 6. P. 573.
补充文件
