首页> 外文会议>22nd International Symposium on Space Terahertz Technology 2011. >560 GHz, 664 GHz and 1.2 THz Schottky based MMIC sub-harmonic mixers for planetary atmospheric remote sensing and FMCW radar
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560 GHz, 664 GHz and 1.2 THz Schottky based MMIC sub-harmonic mixers for planetary atmospheric remote sensing and FMCW radar

机译:基于560 GHz,664 GHz和1.2 THz肖特基的MMIC次谐波混频器,用于行星大气遥感和FMCW雷达

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摘要

We present here the development of several sub-milllimeter wave heterodyne receivers based on MMIC Schottky. First, a 560 GHz heterodyne receiver using MMIC Schottky devices has been developed by JPL. It features a 280 GHz tripler and 560 GHz sub-harmonic mixer integrated in a single block. It exhibits a DSB mixer noise temperature of 1400 K and DSB mixer conversion losses of 7.5 dB at 590 GHz. In addition, a 664 GHz receiver using similar MMIC Schottky devices balanced mixer architecture has been developed. It exhibits good performance with a DSB mixer noise temperature of 2500 K and DSB mixer conversion losses below 10 dB at 670 GHz. Finally, the 1200 GHz channel is under development. It includes an LO source inherited from the HIFI project for the generating enough power at 600 GHz, and a novel 1200 GHz MMIC biasable sub-harmonic mixer that is presented.
机译:我们在此介绍基于MMIC肖特基的几种亚毫米波外差接收器的开发。首先,JPL已开发出使用MMIC肖特基器件的560 GHz外差式接收机。它具有集成在单个模块中的280 GHz三路器和560 GHz次谐波混频器。在590 GHz频率下,DSB混频器噪声温度为1400 K,DSB混频器转换损耗为7.5 dB。此外,已开发出使用类似MMIC肖特基器件的平衡混频器架构的664 GHz接收机。它在2500 K的DSB混频器噪声温度和670 GHz下DSB混频器的转换损耗低于10 dB时表现出良好的性能。最后,正在开发1200 GHz信道。它包括一个从HIFI项目继承而来的LO源,用于在600 GHz时产生足够的功率,以及一个新颖的1200 GHz MMIC可偏置次谐波混频器。

著录项

  • 来源
  • 会议地点 Tucson AZ(US);Tucson AZ(US)
  • 作者单位

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA Radiometer Physics GmbH, Meckenheim, Germany;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

    Universite Pierre et Marie Curie-Paris 6, LERMA, Paris, France;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

    NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 微波与超高频技术;微波与超高频技术;
  • 关键词

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