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Ultrasensitive Mid-Infrared In Situ Spectrometer for Planetary Atmospheric Analysis, Phase I
Completed
Description
The Small Business Innovative Research Phase I proposal seeks to develop a compact, robust in situ spectrometer capable of detecting multiple gas-phase species in planetary atmospheres with ultra-high sensitivity and selectivity. This instrument will employ a novel room-temperature, widely tunable mid-infrared laser source in conjunction with cavity ringdown spectroscopy. During Phase I, the 3.3 to 3.5 µm spectral region will be targeted, which overlaps the spectral absorption features of variety of hydrocarbons, including methane, ethane, and formaldehyde. The ultra-high sensitivity of the proposed system will enable these species to be detected at concentrations below 7*107/cm3 per minute, which corresponds to a detection limit of <30 pptv in Earth?s atmosphere.
Details
| Technology area | Sensors and Instruments > In Situ Instruments and Sensors > Atomic and Molecular Species Assessment |
| Program | Small Business Innovation Research/Small Business Tech Transfer (SBIR/STTR) |
| Lead organization | Langley Research Center, Hampton, VA |
| Start date | 2004-01-16 |
| End date | 2004-07-19 |
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How to get involved
This is a mature technology (TRL 7+) — the realistic path in is usually NASA's Technology Transfer Program: licensing an existing NASA patent, or a Space Act Agreement to use NASA facilities/expertise directly. NASA also runs a startup licensing program with no upfront fee for companies formed to commercialize a specific NASA technology.
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