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Measurement of the Atmospheric Background in the Mesosphere

Completed TRL 6 (started at 4, targeting 6)

Description

Next generation sub-orbital vehicles will provide an innovative platform for the characterization to 300,000 feet. With considerable existing data on the infrared background at stratospheric altitudes, the need to characterize absorption and emission features in the mesosphere becomes apparent. This project comprises a compact infrared spectrometer for measuring atmospheric absorption and emission profiles on a routine basis at moderate spectral resolutions (R < 10,000) at near and mid-infrared wavelengths. The instrument consists of COTS optical components with a stand-alone power system and flight computer separate from the sub-orbital vehicle.

Benefits

The characterization of atmospheric absorption and emission profiles within the Earth's mesosphere using an infrared spectometer will benefit astonomers in the selection of required altitudes for future infrared observations at altitudes above those of airborne or balloon-based experiments.

Details

Technology areaSensors and Instruments > In Situ Instruments and Sensors > Extreme Environments Related to Critical System Health Management
ProgramFlight Opportunities (FO)
Lead organizationSilicon Valley Space Center
Start date2016-08-19
End date2022-08-12

Project contacts

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How to get involved

This is early/mid-stage (TRL 6) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.

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