SBIR-STTR Award

F-band Solid-State Power Amplifier (106-114 GHz)
Award last edited on: 1/23/2023

Sponsored Program
SBIR
Awarding Agency
NASA : JPL
Total Award Amount
$868,000
Award Phase
2
Solicitation Topic Code
S1.04
Principal Investigator
Yon-Lin Kok

Company Information

QuinStar Technology Inc

24085 Garnier Street
Torrance, CA 90505
   (310) 320-1111
   kuno@quinstar.com
   www.quinstar.com
Location: Multiple
Congr. District: 33
County: Los Angeles

Phase I

Contract Number: 80NSSC21C0080
Start Date: 5/4/2021    Completed: 11/19/2021
Phase I year
2021
Phase I Amount
$124,997
QuinStar Technology proposes to develop an efficient, GaN based solid-state power amplifier (SSPA), operating over the 106 to 114 GHz with 4-W output power and power-added efficiency (PAE) > 25%, for the Scanning Microwave Limb Sounder on the Global Atmospheric Composition Mission and the SOFIA (Stratospheric Observatory for Infrared Astronomy) airborne observatory. The proposed amplifier will drive the LO multiplier chain for mixers in the submillimeter-wave detector. QuinStar plans to meet the power and efficiency goals of this program by employing a combination of state-of-the-art (SOA) GaN device technology, innovative circuit design techniques and power combining techniques. We plan to design the MMIC amplifier in a quasi-switching mode with high-Q matching networks implemented on chip. Second, for improved efficiencies, we are proposing to limit the MMIC power level to about 1 watt and use high-efficiency waveguide circuit combining techniques to achieve higher power levels. For this, we propose to use a high-efficiency, 4-way H-tee combiner. Computer simulations show that this approach is capable of realizing combining efficiencies of greater than 95%. QuinStar is the leader in power combining techniques at millimeter-wave frequencies. We have developed both radial and E/H-plane waveguide combiners with SOA power levels and efficiencies in the past decade. Potential NASA Applications (Limit 1500 characters, approximately 150 words): NASA Earth Science missions require submillimeter-wave remote sensing instruments to monitor air quality, climate variability and change, ozone layer stability, weather, and the global hydrological cycle. Due to its shorter wavelength, submillimeter-wave sensors can provide enhanced resolution over lower frequency sensors. A key enabler for this technology is an F-band (106-114 GHz) solid-state power amplifier (SSPA) capable of providing 4-W output power and power-added-efficiency as high as 25% such as the one described in this proposal. Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words): Applications of the W/F-band high-efficiency amplifier technology abound at agencies ranging from helicopter landing and obstacle detection/avoidance radars to cloud radar, UAV, and DoD’s V/W-band (Hotspots) communications systems. Space-based applications include broadband RF cross-links communications constellations and long duration reconnaissance UAV missions in airborne. Duration: 6

Phase II

Contract Number: 80NSSC22CA094
Start Date: 5/4/2022    Completed: 5/3/2024
Phase II year
2022
Phase II Amount
$743,003
An F-band SSPA is required for the Scanning Microwave Limb Sounder on the Global Atmospheric Composition Mission and the SOFIA (Stratospheric Observatory for Infrared Astronomy) airborne observatory. The proposed amplifier will drive the LO multiplier chain for mixers in the submillimeter-wave detector. We are using the state-of-the-art (SOA) GaN device technology based on wide bandgap materials to fabricate a solid-state power amplifier operating at F-band (106-114 GHz) frequencies. GaN devices are operating in a “quasi-switching” mode to achieve high drain efficiencies (>50%); higher efficiencies result in less DC power consumption, less waste heat and smaller heat sinks; the MMIC operate at lower temperatures and have longer lifetimes. A high-Q, matching network is developed on the MMIC to achieve the required power (1.2 Watts) and Power-Added-Efficiency (28%). We are using an innovative power combining network with small form factor to achieve combining power (4+ Watts) and efficiencies of greater than 90% over the band of 106 to 114 GHz. Potential NASA Applications (Limit 1500 characters, approximately 150 words): Future NASA Earth Science missions require submillimeter-wave remote sensing instruments to monitor air quality, climate variability and change, ozone layer stability, weather, and the global hydrological cycle. Submillimeter-wave sensors can provide enhanced resolution over lower frequency sensors. A key enabler for this technology is an F-band (106-114 GHz) solid-state power amplifier (SSPA) as described in this proposal. Other applications include planetary missions which require W/F-band FMCW sensors to assist in planetary landings. Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words): The technology developed in F-band is readily applicable to build amplifiers in communication systems for aeronautical navigation and broadcasting. Applications for this W/F-band high-efficiency amplifier technology also abound at agencies ranging from helicopter landing and obstacle detection/avoidance radars to cloud radar, UAV, and DoD’s V/W-band (Hotspots) communications systems. Duration: 24