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Completed TRL 4 (started at 3, targeting 4)
The mid-infrared (MIR) spectral range (2.5-5 μm) is of particular interest for remote sensing of planetary atmospheres and surfaces, as this provides considerable information on composition. The current generation of MIR spectrometers are typically large in size, weight and power, limiting their selectability for missions. Our long-term goal is to develop a revolutionary MIR spectrometer based on integrated photonics technology that offers ultra-small size, weight and power with non-moving parts and lower cost for future planetary missions. This proposal will demonstrate a PIC-based, near-infrared (NIR) spectrometer which will prove the technique with available, low-cost hardware and pave the way for a MIR version.
This work will demonstrate key technologies with a wide range of potential sensing applications.
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