The Superconducting Spectroscopic Array Receiver (SSAR) for Millimeter-wave Radio Astronomy

J. Yang, W. Shan, S. Shi, Q. Yao, Y. Zuo, S.H. Chen, A. Cao, Z.H. Lin
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引用次数: 8

Abstract

The studies on formation and evolution of interstellar molecular clouds and star formation give rise to high demands on imaging capability of millimeter-wave spectroscopic receiver. The Superconducting Spectroscopic Array Receiver (SSAR) of 3times3 pixels has been designed to work over 85-116 GHz. A number of new technological approaches are applied in the development of SSAR including of 4-K cooled superconducting SIS mixers using sideband separating scheme, automatically tuned digital bias, cooled SiGe HBT amplifiers, and digital FFT spectrometers. Development of the receiver system is undergoing. Upon completion, this instrument will enhance significantly the mapping capability in millimeter-wave line observations with high spectroscopic resolution. This paper introduces the main technological features applied in design and development of the receiver system.
毫米波射电天文超导光谱阵列接收机(SSAR)
星际分子云的形成演化和恒星形成的研究对毫米波光谱接收机的成像能力提出了很高的要求。设计了3x3像素的超导光谱阵列接收机(SSAR),工作频率为85-116 GHz。许多新技术方法应用于SSAR的开发,包括使用边带分离方案的4-K冷却超导SIS混频器,自动调谐数字偏置,冷却SiGe HBT放大器和数字FFT光谱仪。接收机系统的研制正在进行中。该仪器建成后,将显著提高高光谱分辨率毫米波线观测的制图能力。本文介绍了接收机系统设计与开发的主要技术特点。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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