Share Email Print

Proceedings Paper • new

Development of a low-power cryogenic MMIC HEMT amplifier for heterodyne array receiver application
Author(s): J. Liu; W. Shan; T. Kojima; X. Zhang; Z. Li; Y. Chen
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We present in this paper a study of a low-power consumption cryogenic amplifier with GaAs-based HEMT. A two-stage MMIC low noise amplifier for 2.5-4.5 GHz frequency range has been designed, fabricated and measured at a low-power condition with the temperature range from 300 K to 4 K. To design such a cryogenic MMIC amplifier, firstly we extracted the model of the bare-die transistor at cryogenic temperatures fabricated together with the MMIC. The temperature-dependent DC and RF characteristics of the HEMT have been measured. From the approximate noise model based on the DC characteristics, we verified that the HEMTs offer sufficient gain and reasonably noise at a relative lowpower operation condition. Subsequently, we designed a low-power dissipation cryogenic MMIC amplifier utilizing the cryogenic s2p model of the HEMTs biased at the optimal low-power condition. At cryogenic temperature, the GaAsbased amplifier achieves a gain larger than 20dB and a noise temperature as low as 10 K with a total power consumption of 1.2 mW. The low-power amplifiers can be used as first-stage IF amplifiers in a superconductor-insulatorsuperconductor (SIS) receiver, and are especially useful in focal plane arrays with large pixel count because of the merit of the total power consumption.

Paper Details

Date Published: 9 July 2018
PDF: 8 pages
Proc. SPIE 10708, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, 107082X (9 July 2018); doi: 10.1117/12.2314356
Show Author Affiliations
J. Liu, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Univ. of Chinese Academy of Sciences (China)
W. Shan, National Astronomical Observatory of Japan (Japan)
T. Kojima, National Astronomical Observatory of Japan (Japan)
X. Zhang, Purple Mountain Observatory (China)
Z. Li, Purple Mountain Observatory (China)
Y. Chen, Shanghai Astronomical Observatory (China)

Published in SPIE Proceedings Vol. 10708:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Jonas Zmuidzinas; Jian-Rong Gao, Editor(s)

© SPIE. Terms of Use
Back to Top