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Terahertz Quantum Cascade Laser Local Oscillator
Completed
Description
NASA and NASA funded missions/instruments such as Aura (EOS CH-1)/MLS (Microwave Limb Sounder), SOFIA/GREAT and STO have demonstrated the need for local oscillator (LO) sources between 30 and 300 um (1 and 10 THz). For observations >2 THz, technologically mature microwave sources typically have microwatt power levels which are insufficient to act as LOs for a heterodyne receivers. LongWave Photonics is proposing to develop a compact, frequency agile, phase/frequency locked, power stabilized, single mode quantum cascade laser (QCL) system with > 2mW power output. The system includes distributed feedback grating (DFB) QCL arrays packed with multiple devices on a single semiconductor die with individual devices lasing at different frequencies. The source will be frequency agile over 150 GHz with center frequencies ranging from 2 to 5 THz range. The DFB QCL array will be packaged in a high-reliability Stirling cycle cooler. The source will be phase/frequency locked to a stable microwave reference synthesizer which allows continuous phase-locking ability over the THz laser tunable range with 2 THz, with reduction of LO linewidth, and absolute frequency accuracy and with output power stabilized to reduce system noise. The whole system will be in a compact package which can be further reduced for a flight instrument.
Details
| Technology area | Sensors and Instruments > Remote Sensing Instruments and Sensors > Lasers |
| Program | Small Business Innovation Research/Small Business Tech Transfer (SBIR/STTR) |
| Lead organization | LongWave Photonics, LLC, Mountain View, CA |
| Start date | 2018-06-07 |
| End date | 2018-10-31 |
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