Multi-pixel Ka-band radiometer for the QUIJOTE experiment (Phase II)

J. Cano, E. Villa, J. Cagigas, B. Aja, J. V. Terán, A. Pérez, L. de la Fuente, E. Artal, A. Mediavilla, R. Hoyland
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引用次数: 8

Abstract

This paper presents the configuration of the Ka-band radiometer developed for the Phase II of the QUIJOTE radio astronomy experiment, as well as the design of the different subsystems involved in the instrument. The new configuration, consisting of around 30 modified receivers working in the 26 - 36 GHz band, avoids the need of a rotating polar modulator at cryogenic temperatures, which is a source of mechanical and thermal difficulties. Moreover, the larger number of receivers will increase the instrument sensitivity. These two aspects are a clear advantage over the receiver developed for the experiment Phase I. The present paper also gives detailed information of some designed subsystems such as the feedhorn, the polarizer, the orthomode transducer, the cryogenic low-noise amplifiers and the back-end module.
QUIJOTE实验用多像素ka波段辐射计(二期)
本文介绍了为QUIJOTE射电天文实验二期研制的ka波段辐射计的结构,以及该仪器所涉及的各个子系统的设计。新的配置由大约30个改进的接收器组成,工作在26 - 36ghz频段,避免了在低温下需要旋转极性调制器,这是机械和热难题的来源。此外,接收机数量的增加将提高仪器的灵敏度。这两个方面明显优于为实验阶段开发的接收机。本文还详细介绍了设计的一些子系统,如馈电喇叭、偏振器、正交换能器、低温低噪声放大器和后端模块。
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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