毫米空间天文台高分辨率光谱仪混频器的研制

IF 3.9 2区 工程技术 Q2 ENGINEERING, ELECTRICAL & ELECTRONIC
Ivan V. Tretyakov;Andrey V. Khudchenko;Kirill I. Rudakov;Irina V. Ivashentseva;Natalia S. Kaurova;Boris M. Voronov;Maria S. Kirsanova;Tatiana I. Larchenkova;Gregory N. Goltsman;Andrey M. Baryshev;Ronald Hesper;Fedor V. Khan;Elena S. Zhukova;Artem M. Chekushkin;A. V. Melentev;K. V. Zhivetev;A. V. Terentiev;Valery P. Koshelets;S. F. Likhachev
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引用次数: 0

摘要

研究宇宙中水的起源和运移是“毫米波”空间天文台科学计划的重要组成部分。这将通过在单碟模式下使用机载仪器-高分辨率光谱仪(HRS)进行观测而成为可能。该仪器包含工作在$0.5 -2.7$太赫兹范围内的外差阵列接收器,包括工作频率低于1.3太赫兹的超导体-绝缘体-超导体混频器的3像素阵列和基于观察频率高于1.3太赫兹的NbN HEB混频器的7像素矩阵接收器。本文介绍了计划用于毫米空间天文台HRS仪器的混合器的研制现状。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Development of Mixers for the High-Resolution Spectrometer of the Millimetron Space Observatory
The study of the origin and transport of water in the universe is an important part of the scientific program of the Millimetron space observatory. This will be made possible by observations conducted in single-dish mode using an onboard instrument—the high-resolution spectrometer (HRS). This instrument incorporates heterodyne array receivers operating within the range $0.5 -2.7$ THz, comprising 3-pixel arrays of superconductor–insulator–superconductor mixers operating at frequencies below 1.3 THz and 7-pixel matrix receivers based on NbN HEB mixers observing above 1.3 THz. This article presents the current status of development for a mixers planned for use in the HRS instrument of the Millimetron space observatory.
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来源期刊
IEEE Transactions on Terahertz Science and Technology
IEEE Transactions on Terahertz Science and Technology ENGINEERING, ELECTRICAL & ELECTRONIC-OPTICS
CiteScore
7.10
自引率
9.40%
发文量
102
期刊介绍: IEEE Transactions on Terahertz Science and Technology focuses on original research on Terahertz theory, techniques, and applications as they relate to components, devices, circuits, and systems involving the generation, transmission, and detection of Terahertz waves.
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