SBIR-STTR Award

Powerful and Compact SSPA Modules for Active Remote Sensing
Award last edited on: 3/27/2023

Sponsored Program
SBIR
Awarding Agency
NASA : JPL
Total Award Amount
$874,893
Award Phase
2
Solicitation Topic Code
S1.02
Principal Investigator
Theodore Reck

Company Information

Virginia Diodes Inc (AKA: VDI)

979 Second Street Se Suite 309
Charlottesville, VA 22902
   (434) 297-3257
   vdirfq@virginiadiodes.com
   www.vadiodes.com
Location: Single
Congr. District: 05
County: Charlottesville city

Phase I

Contract Number: 80NSSC19C0408
Start Date: 8/19/2019    Completed: 2/18/2020
Phase I year
2019
Phase I Amount
$124,992
This proposal is responsive to NASA SBIR Subtopic S1.02: Technologies for Active Microwave Remote Sensing; specifically the item titled “1 Watt G-band (167-175 GHz) Solid State Power Amplifier for Remote Sensing Radars.” The technical goal is a compact and reliable amplifier module with one-watt of output power and 20% power added efficiency (PAE) at the stated frequency band of interest. As described in the solicitation, the NASA applications include SmallSat based cloud, water, and precipitation missions, similar to the highly successful RainCube (which operated at 37.5 GHz). Compact size and power efficiency are required for the SmallSat form factor and also to reduce costs for the envisioned swarm mission technology. The Phase I research includes the completion of the simulation and design study for the new amplifier chip and the demonstration of the waveguide power combining technology that will be required to achieve the one-watt goal without sacrificing significant PAE. The deliverable results will include two primary items that should prove the feasibility of the technology. These are the design report from that states the expected performance of the new amplifier MMIC and the delivery of a prototype amplifier module operating at the frequency band of interest that utilizes the four-way power combining with sufficient efficiency to meet the NASA goals. Potential NASA Applications (Limit 1500 characters, approximately 150 words) NASA applications include cloud, water, and precipitation missions that require radar sources above 100 GHz, particularly SmallSat and CubeSat missions, as well as swarm missions. Higher power amplifier modules will also enable higher power terahertz sources for radio astronomy local oscillators; most relevant are astronomical measurements of molecular lines at including ~1.4, ~1.9, ~2.6, and 4.7 THz; especially for the case of large arrays with many dozens of pixels. Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words) More powerful and efficient amplifier modules, coupled with frequency multiplier with greater power handling ability, will benefit the entire terahertz community. Applications include dynamic nuclear polarization enhanced nuclear magnetic resonance, electron paramagnetic resonance, plasma diagnostics, imaging radars and higher frequency test & measurement equipment.

Phase II

Contract Number: 80NSSC20C0147
Start Date: 7/14/2020    Completed: 7/13/2022
Phase II year
2020
Phase II Amount
$749,901
The goal is a compact and reliable amplifier module with one-watt output power and high power added efficiency (PAE) within the frequency band of interest. As described in the solicitation, NASA applications include SmallSat based cloud, water, and precipitation missions, similar to the highly successful RainCube (which operated at 37.5 GHz). Compact size and power efficiency are required for the SmallSat form factor as well as to reduce costs for the envisioned swarm mission technology. The Phase I research included the completion of the design study for the new amplifier chip and the demonstration of the power combining technology that is required to achieve the one-watt goal. The deliverables include two primary items that demonstrate the feasibility of the technology. These are the Teledyne design report showing the expected performance of the new amplifier MMIC and the prototype amplifier module that demonstrates the four-way power combining. Although significant challenges remain, VDI is confident that the primary solicitation goals can be achieved through Phase II development Potential NASA Applications (Limit 1500 characters, approximately 150 words) NASA applications include cloud, water, and precipitation remote sensing missions that require radar sources above 100 GHz, particularly SmallSat and CubeSat missions, as well as swarm missions. This include both Earth and planetary missions. Higher power amplifier modules will also enable higher power terahertz sources for radio astronomy local oscillators; the most relevant are astronomical measurements of molecular lines at including ~1.4, ~1.9, ~2.6, and 4.7 THz; especially for the case of large arrays with many dozens of pixels. Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words) The SSPAs are required for a broad range of scientific an commercial applications. These include DNP-NMR and ESR systems for biology and chemistry, transmitters for 6G R&D, plasma diagnostic systems, imaging systems for security scanners. The new amplifiers can also be paired with high power frequency multipliers to create more powerful and efficient sources throughout the 300 - 5,000 GHz range.