首页> 外文会议>22nd International Symposium on Space Terahertz Technology 2011. >A quasi-optical NbN HEB mixer with 800K DSB noise temperature at 2.5 THz
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A quasi-optical NbN HEB mixer with 800K DSB noise temperature at 2.5 THz

机译:准光学NbN HEB混频器,在2.5 THz时具有800K DSB噪声温度

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摘要

This paper presents the heterodyne measurement results of a quasi-optical NbN mixer at 2.5 THz. The HEB device was developed at LERMA in the frame of a CNES research project and the European programme Radionet FP7. It consists of a 2 μm wide, 0.2 urn long and about 3.5 nni thick NbN bridge on a silicon substrate. THz radiation is coupled to the HEB device through a quasi-optical circuit including an integrated spiral antenna and an anti-reflection coated hyper-hemispherical Si lens. The noise temperature measurement was performed at SRON using an optically pumped FIR gas laser as LO and a hot/cold load setup in vacuum to obtain the Y-factor. Two methods have been employed to measure the receiver noise temperature, either by adjusting the LO power at a fixed bias voltage between the hot and cold load to suppress the direct detection effect or by scanning the LO power when the bias voltage is kept constant to overcome the laser power fluctuations and the direct detection. The double sideband receiver noise temperatures obtained by both methods and without any corrections are as low as 800 K at 2.5 THz.
机译:本文介绍了准光学NbN混频器在2.5 THz时的外差测量结果。 HEB设备是在LERMA的CNES研究项目和欧洲计划Radionet FP7的框架下开发的。它由一个2μm宽,0.2 um长和大约3.5 nni厚的NbN桥组成,位于硅衬底上。太赫兹辐射通过包括集成螺旋天线和防反射涂层的超半球形硅透镜的准光学电路耦合到HEB设备。噪声温度的测量是在SRON上进行的,使用的是光泵浦FIR气体激光器作为LO,并将热/冷负载设置在真空中以获得Y因子。已经采用了两种方法来测量接收器噪声温度,或者通过在热负载和冷负载之间的固定偏置电压下调整LO功率以抑制直接检测效果,或者在偏置电压保持恒定以克服时通过扫描LO功率来测量接收机噪声温度。激光功率波动和直接检测。通过两种方法获得且未经任何校正的双边带接收机噪声温度在2.5 THz时低至800K。

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

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France Purple Mountain Observatory, NAOC, CAS, Nanjing, Jiangsu 210008, China;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    Purple Mountain Observatory, NAOC, CAS, Nanjing, Jiangsu 210008, China;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LERMA, Observatoire de Paris, UPMC, CNRS, 75014 Paris, France;

    LPN, Laboratoire de Photonique et de Nanostructures, 91460 Marcoussis, France;

    SRON Netherlands Institute for Space Research, 9747 AD Groningen, The Netherlands;

    SRON Netherlands Institute for Space Research, 9747 AD Groningen, The Netherlands Kavli Institute of Nanoscience, Delft University of Technology, 2628 CJ Delft, The Netherlands;

    Purple Mountain Observatory, NAOC, CAS, Nanjing, Jiangsu 210008, China;

  • 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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