4-12 GHz and 25-34 GHz cryogenic MHEMT MMIC low noise amplifiers for radio astronomy
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Aja Abelán, Beatriz
; Seelmann-Eggebert, Matthias; Leuther, Arnulf; Massler, Hermann; Schlechtweg, Michael; Gallego Puyol, Juan Daniel; López Fernández, Isaac; Diez González, María del Carmen; Malo Gómez, Inmaculada; Villa Benito, Enrique
; Artal Latorre, Eduardo
Fecha
2012Derechos
© 2012 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.
Publicado en
IEEE/MTT-S International Microwave Symposium Digest, Montreal, Quebec, Canada, 2012, 1244-1246
Editorial
Institute of Electrical and Electronics Engineers, Inc.
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Palabras clave
Cryogenic
Low noise amplifier
MMIC
mHEMT
Resumen/Abstract
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorphic High Electron Mobility Transistor (mHEMT) process have been developed. Cryogenic performance of a 4–12 GHz and a 25–34 GHz LNAs is presented. The 4–12 GHz LNA cooled at 15 K exhibits an associated gain of 31.5 dB ± 1.8 dB and average noise temperature of 5.3 K with a low power dissipation of 8 mW. Cooled to 15 K the 25–34 GHz amplifier has demonstrated a flat gain of 24.2 dB ± 0.4 dB with 15.2 K average noise temperature, and a very low power dissipation of 2.8 mW on chip. The mHEMT based LNA MMICs have demonstrated excellent noise characteristics at cryogenic temperatures for their use in radio astronomy applications.
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