17 February 2003 W band power amplifier development for the Herschel HIFI instrument
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This paper summarizes the development of W Band amplifiers for the Local Oscillator (LO) chains for the Herschel HIFI (Heterodyne Instrument for Far Infrared) Instrument. Key amplifier development issues and their solutions are presented, which have been applied on the way to realizing stable, wide-band amplifiers capable of producing 240 mW or greater RF power output across the 71 to 106 GHz frequency range. The HIFI power amplifier design embodiment is based on an A-40 silicon-aluminum alloy package with six GaAs(Gallium Arsenide) HEMT(High Electron Mobility Transistors) MMIC(Monolithic Microwave Integrated Circuit) amplifier chips used in each amplifier. Development challenges addressed include: MMIC chip designs which initially had a variety of oscillation or "moding" propensities (mostly out-fo-band), signal splitter and combiner development and matching across the band, matching of chip characteristics for those chips installed in the parallel power combined arms of the amplifier, power output control and leveling. The chosen design solutions are presented, including device, component and material selection for amplifier operation at cryogenic temperatures. Room temperature and cryogenic (120 Kelvin) data is also shown for the amplifier.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robert Ferber, Robert Ferber, Todd C. Gaier, Todd C. Gaier, John C. Pearson, John C. Pearson, Lorene A. Samoska, Lorene A. Samoska, Mary Wells, Mary Wells, Gerard Swift, Gerard Swift, Paul Yocom, Paul Yocom, Yun Chung, Yun Chung, April Campbell, April Campbell, } "W band power amplifier development for the Herschel HIFI instrument", Proc. SPIE 4855, Millimeter and Submillimeter Detectors for Astronomy, (17 February 2003); doi: 10.1117/12.459192; https://doi.org/10.1117/12.459192


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