Chin. Phys. Lett.  2007, Vol. 24 Issue (6): 1778-1781    DOI:
Original Articles |
Noise Behaviour of a THz Superconducting Hot-Electron Bolometer Mixer
ZHANG Wen 1,3;LI Ning1;JIANG Ling1;MIAO Wei1;LIN Zhen-Hui1;YAO
Qi-Jun1;SHI Sheng-Cai1;CHEN Jian2;WU Pei-Heng2;S. I. Svechnikov3;Yu. B. Vachtomin3;S. V. Antipov3;B. M. Voronov3;G. N. Gol'tsman3
1Purple Mountain Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Nanjing 2100082Department of Electronic Science and Engineering, Nanjing University, Nanjing 2100933Department of Physics, Moscow State Pedagogical University, Moscow 119992, Russia
Cite this article:   
ZHANG Wen, LI Ning, JIANG Ling et al  2007 Chin. Phys. Lett. 24 1778-1781
Download: PDF(452KB)  
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract A quasi-optical superconducting NbN hot-electron bolometer (HEB) mixer is measured in the frequency range of 0.5--2.5THz for understanding of the frequency dependence of noise temperature of THz coherent detectors. It has been found that noise temperature increasing with frequency is mainly due to the coupling loss between the quasi-optical planar antenna and the superconducting HEB bridge when taking account of non-uniform distribution of high-frequency current. With the coupling loss corrected, the superconducting HEB mixer demonstrates a noise temperature nearly independent of frequency.
Keywords: 95.55.Jz      95.85.Bh     
Received: 05 March 2007      Published: 17 May 2007
PACS:  95.55.Jz (Radio telescopes and instrumentation; heterodyne receivers)  
  95.85.Bh (Radio, microwave (>1 mm))  
TRENDMD:   
URL:  
https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2007/V24/I6/01778
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
ZHANG Wen
LI Ning
JIANG Ling
MIAO Wei
LIN Zhen-Hui
YAOQi-Jun
SHI Sheng-Cai
CHEN Jian
WU Pei-Heng
S. I. Svechnikov
Yu. B. Vachtomin
S. V. Antipov
B. M. Voronov
G. N. Gol'tsman
[1] Phillips T G and Keene J 1992 Proc. IEEE 80 1662
[2] Siegel P H 2002 IEEE Trans. Microwave Theory Tech. 50910
[3] Karpov A, Miller D, Rice F, Zmuidzinas J, Stern J A, Bumble B, andLeduc H G 2001 Proc. 8th Int. Supercond. ElectronConf. 521 (Osaka Japan 19--22 June 2001)
[4] Gao J R, Hovenier J N, Yang Z Q, Baselmans J J A, BaryshevA, Hajenius M, Klapwijk T M, Adam A J L, Klaassen T O, Williams B S,Kumar S, Hu Q and Reno J L 2005 Appl. Phys. Lett. 86 244104
[5] Baselmans J J A, Hajenius M, Gao J R, Baryshev A, Kooi J,Klapwijk T M, Voronov B, de Korte P, and Gol'tsman G 2005 IEEETrans. Appl. Supercond. 15 484
[6] Gershenzon E M, Goltsman G N, Gogidze, Eliantev A I, KarasikB S and Semenov A D 1990 Sov. Phys. Supercond. 3 1582
[7] Hajenius M, Barends R, Gao J R, Klapwijk T M, Baselmans J JA, Baryshev A, Voronov B and Gol'tsman G 2005 IEEE Trans. Appl.Supercond. 15 495
[8] Richards P L 1994 J. Appl. Phys. 76 1
[9] Ekstrom H, Karasik B S, Kollberg E L and Yngvesson K S 1995 IEEE Trans. Microwave Theory Tech. 43 938
[10] Zhang W, Jiang L, Lin Z H, Yao Q J, Shi S C, Svechnikov S I,Vachtomin Y B, Antipov S V, Voronov B M, Kaurova N S and Gol'tsman G N2005 Proc. 16th Int. Symp. on Space Terahertz Technology (GoteborgSweden 2--4 May 2005) p 209
[11] Jiang L, Miao W, Zhang W, Li N, Lin Z H, Yao Q J, Shi S C,Svechnikov S I, Vachtomin Y B, Antipov S V, Voronov B M, Kaurova N S,and Gol'tsman G N 2006 IEEE Trans. Microwave Theory Tech. 542944
[12] Instruction manual for the FIRL100 1995 EdinburghInstruments Ltd
[13] Mylar Polyester Films 2006 Dupont Corporation USA
[14] Semenov A D, Hubers H W, Schubert J, Gol'tsman G N,Elantiev A I, Voronov B M and Gershenzon E M 2000 J. Appl.Phys. 88 6758
[15] Semenov A D, Richter H, Hubers H W, Gunther B, Smirnov A, II'in KS, Siegel M and Karamarkovic J P 2007 IEEE Trans. Microwave TheoryTech. 55 239
[16] Ansoft High Frequency Structure Simulator (Version 8.0), AnsoftCo.
[17] Jiang L, Zhang W, Li N, Lin Z H, Yao Q J, Miao W, Shi S C,Svechnikov S I, Vakhtomin Y B, Antipov S V, Voronov B M, Gol'tsman G N2007 IEEE Trans. Appl. Supercond. (in press)
Related articles from Frontiers Journals
[1] LI Jing, WANG Ming-Jye, SHI Sheng-Cai, Hiroshi Matsuo. Terahertz Detection with Twin Superconductor--Insulator--Superconductor Tunnel Junctions[J]. Chin. Phys. Lett., 2007, 24(2): 1778-1781
[2] YU Zhi-Yao. Thin Circular Disc Shells of Radio Sources Around Supernova Remnant G16.2-2.7[J]. Chin. Phys. Lett., 2002, 19(11): 1778-1781
[3] ZHOU Guo-Cheng, WU Ching-Sheng, WANG De-Ju, CHEN Yan-Ping,. Excitation of Electromagnetic Waves by an Electron Ring Beam in a Magnetized Plasma Waveguide[J]. Chin. Phys. Lett., 2002, 19(10): 1778-1781
[4] YU Xing-Feng, YAO Jin-Xing. Numbers of Electrons in Solar Flares as Deduced from Microwave and X-Ray Bursts [J]. Chin. Phys. Lett., 2001, 18(3): 1778-1781
[5] JARKEN Esimbek, ZHENG Xing-Wu,. Does the Masing Gas Fall Inward VY CMa?[J]. Chin. Phys. Lett., 2001, 18(3): 1778-1781
[6] YU Xing-Feng, YAO Jin-Xing. Mapping Analysis of Solar Radio Burst at 17GHz on 1992 October 27[J]. Chin. Phys. Lett., 2000, 17(8): 1778-1781
[7] XU Fu-Ying, LIU Yu-Ying, FU Qi- Jun, WU Hong-Ao. The First Spectral Analysis of Solar Radio Spike Event[J]. Chin. Phys. Lett., 2000, 17(6): 1778-1781
[8] XU Fu-Ying, LIU Yu-Ying, YAO Qi-Jun, FU Qi-Jun, MENG Xuan, WU Hong-Ao. Some New Observing Features of a Solar Radio Spectral Event on August 25,1999[J]. Chin. Phys. Lett., 2000, 17(11): 1778-1781
Viewed
Full text


Abstract