F-band Solid-State Power Amplifier (106-114 GHz)

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) gt; 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.nbsp;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,nbsp;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.nbsp;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%.nbsp;QuinStar is the leader in power combining techniques at millimeter-wave frequencies. We havenbsp;developed both radial and E/H-plane waveguide combiners with SOA power levels and efficiencies in the past decade.