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Completed TRL 6 (started at 4, targeting 6)
We propose to fly PAMSS on a balloon to demonstrate autonomous operation and trace gas sensing over a large range of pressures, temperatures, and concentrations. Success will advance PAMSS to TRL6. The resulting technology will be available for proposal for planetary mission instrumentation to detect trace species in the atmospheres of Mars, Venus, Titan, or giant planets.
Papers:
Planetary Atmospheres Minor Species Sensor (PAMSS) (2014)
Planetary atmospheres minor species sensor balloon flight test to near space (2015)
Problem Statement Trace gases can have a large impact on chemical reactions that control larger abundances of important atmospheric gases, such as pollutants and greenhouse gases. Trace gases can indicate for geologic and biologic activities. Knowledge of the presence, concentration, and spatial distribution is important on other planets as well as on Earth. A problem is that current methods of high sensitivity trace gases must interrogate over a range of altitudes and areas to obtain sufficient signal, and they are unable to quantify local concentrations and rapid spatial variations. An opportunity is PAMSS, the first mid-infrared intracavity laser absorption spectrometer. PAMSS achieves tens of kilometer effective optical path lengths in a small, light package with low power requirements.
Summary of 3/8/2015 Flight Test
A World View balloon reached an altitude of 105,000 feet and loitered above 98,425 feet for nearly an hour and 45 minutes to test University of Central Florida’s (UCF), Orlando, Planetary Atmospheres Minor Species Sensor (PAMSS) experiment. UCF’s PAMSS is the first mid-infrared, intra-cavity laser absorption spectrometer that will be detecting trace gases and sensing over a large range of pressures, temperatures and concentrations while operating autonomously. This technology could be used for future planetary missions as well as the study of the Earth’s atmosphere.
The Infrared Intracavity Laser Absorption Spectroscopy (ICLAS) technology will be used to detect trace vapors and gases on planets, which can benefit future NASA missions and other government agencies such as the military. In the event the technology is used for medical diagnostic purposes, it will benefit the entire nation.
Future Customers
The resulting technology will be available for proposal for planetary mission instrumentation to detect trace species in the atmospheres of Mars, Venus, Titan, or giant planets. In addition the technology can be used for Earth atmosphere sensing as well as for detecting trace gases that may pose a health hazard to workers or a scientific contamination hazard to spacecraft instrumentation. The technology has many other applications, incl. sensing for explosives and medical breath analysis.
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