X- to Ka- Band Cryogenic LNA Module for Very Long Baseline Interferometry

Fung, Andy; Samoska, Lorene; Bowen, James; Montanez, Steve; Kooi, Jacob; Soriano, Melissa; Jacobs, Christopher; Manthena, Raju; Hoppe, Daniel; Akgiray, Ahmed; Lai, Richard; Mei, Xiaobing; Barsky, Michael

The JPL Technical Report Server is migrating to the JPL Open Repository in January 2023. Please update bookmarks to https://jor.jpl.nasa.gov/ for external access and https://jori.jpl.nasa.gov for internal access.

X- to Ka- Band Cryogenic LNA Module for Very Long Baseline Interferometry

Fung, Andy; Samoska, Lorene; Bowen, James; Montanez, Steve; Kooi, Jacob; Soriano, Melissa; Jacobs, Christopher; Manthena, Raju; Hoppe, Daniel; Akgiray, Ahmed; Lai, Richard; Mei, Xiaobing; Barsky, Michael

URI: http://hdl.handle.net/2014/52327

Date: 2020-06-21

Publisher: Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2020

Citation: IMS 2020 International Microwave Symposium, Los Angeles, California, June 21-26, 2020

Abstract:

We report a new result of a packaged low noise amplifier (LNA) module with wide bandwidth of 5 to 35 GHz with low noise temperature performance of 10 - 18 K, while operated at 10 K ambient. The LNA used 3-stages of sub-50 nm gate length, 100% indium channel content indium phosphide (InP) high electron mobility transistors (HEMTs). Wideband cryogenic LNAs are important for future radio astronomy observatories. To our knowledge these results represent the lowest noise achieved in a wideband amplifier from 5-35 GHz.

Show full item record