Development of Cryogenic Systems for Astronomical Research

被引:1
|
作者
Balega, Yuri [1 ]
Bolshakov, Oleg [2 ]
Chernikov, Aleksandr [2 ,3 ]
Gunbina, Aleksandra [2 ,4 ]
Edelman, Valerian [5 ]
Efimova, Mariya [2 ]
Eliseev, Aleksandr [2 ]
Krasilnikov, Artem [1 ,2 ]
Lapkin, Igor [2 ]
Lesnov, Ilya [2 ]
Mansfeld, Mariya [1 ,2 ]
Markina, Mariya [4 ,5 ]
Pevzner, Evgenii [2 ]
Shitov, Sergey [4 ,6 ]
Smirnov, Andrey [7 ]
Tarasov, Mickhail [4 ]
Tyatushkin, Nickolay [2 ]
Vdovin, Anton [1 ,2 ]
Vdovin, Vyacheslav [1 ,2 ,7 ]
机构
[1] Special Astrophys Observ RAS, Nizhnii Arkhyz 369167, Russia
[2] AV Gaponov Grekhov Inst Appl Phys RAS, Nizhnii Novgorod 603600, Russia
[3] Joint Inst Nucl Res, Moscow 141980, Russia
[4] Kotelnikov Inst Radio Engn & Elect RAS, Moscow 101990, Russia
[5] PL Kapitza Inst Phys Problems RAS, Moscow 119334, Russia
[6] Natl Univ Sci & Technol MISIS, Lab Cryoelectron Syst, Moscow 119049, Russia
[7] PN Lebedev Phys Inst RAS, Moscow 119333, Russia
基金
俄罗斯科学基金会;
关键词
radio astronomy; cryogenic receivers; cryogenic systems; radio waves; IR and optics ranges; terahertz range; CYCLE DILUTION REFRIGERATOR; MILLIMETER; REFLECTIVITY;
D O I
10.3390/photonics11030257
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The article presents a brief review of cooling systems that ensure various temperature levels (from 0.1 K to 230 K) for radio astronomical receivers of photonic and electronic (or optical and radio) devices. The features of various cooling levels and the requirements for the design of the cooling systems are considered in detail, as well as the approaches to designing interfaces for cooled receivers: vacuum, cryogenic, electrical, mechanical, optical, and other interfaces required for effective operation. The presented approaches to design are illustrated by a series of joint developments of the authors carried out over the past 45 years, including those produced over the past year.
引用
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页数:36
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