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An Ultra Low-noise Radio Frequency Amplifier Based on a DC SQUID
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  • An Ultra Low-noise Radio Frequency Amplifier Based on a DC SQUID
  • An Ultra Low-noise Radio Frequency Amplifier Based on a DC SQUID
저자명
Muck. Michael,Ande. Marc-Olivier,Kinion. Darin,Clarke. John
간행물명
Progress in superconductivity
권/호정보
2000년|2권 1호|pp.1-5 (5 pages)
발행정보
한국초전도학회
파일정보
정기간행물|ENG|
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이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
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기타언어초록

We have developed an extremely sensitive radio frequency amplifier based on the dc superconducting quantum interference device (dc SQUID). Unlike a conventional semiconductor amplifier, a SQUID can be cooled to ultra-low temperatures (100 mK or less) and thus potentially achieve a much lower noise temperature. In a conventional SQUID amplifier, where the integrated input coil is operated as a lumped element, parasitic capacitance between the coil and the SQUID washer limits the frequency up to which a substantial gain can be achieved to a few hundred MHz. This problem can be circumvented. by operating the input coil of the SQUID as a microstrip resonator: instead of connecting the input signal between the two ends of the coil, it is connected between the SQUID washer and one end of the coil; the other end is left open. Such amplifiers have gains of 15 dB or more at frequencies up to 3 GHz. If required, the resonant frequency of the microstrip can be tuned by means of a varactor diode connected across the otherwise open end of the resonator. The noise temperature of microstrip SQUID amplifiers was measured to be between 0.5 K $pm$ 0.3 K at a frequency of 80 MHz and 1.5 K $pm$: 1.2 K at 1.7 GHz, when the SQUID was cooled to 4.2 K. An even lower noise temperature can be achieved by cooling the SQUID to about 0.4 K. In this case, a noise temperature of 100 mK $pm$ 20 mK was achieved at 90 MHz, and of about 120 $pm$ 100 mK at 440 MHz.