A Light-Emitting-Diode (LED) non-dispersive absorption sensor for early fire and hazardous gases detection

Kyle Thurmond, Justin Urso, Michael Villar, William P. Partridge, Subith S. Vasu

Research output: Contribution to conferencePaperpeer-review

Abstract

With compact, economical, low-power sensors that are able to continually monitor gases that are characteristic of burning materials, a distributed sensor array could be implemented on space vehicles that would allow early detection of fires, gas leaks, or other critical events. With careful selection of targeted gases, it may be possible to identify the material that is burning or smoldering, better informing the crew so that they may respond and prioritize high emergency events. A lab proto type of such a sensor has been developed using robust, low-cost light-emitting-diodes (LEDs) that is currently configured to simultaneously resolve transient CO and CO2 concentrations, which are trace gases that increase in the presence of smoldering/burning materials. This early stage system has been shown to be cable of a detectability limit of 400ppm for CO and 30ppm for CO2, with no cross interference between the gases. The signal is well resolved for fluctuations up to 250Hz. Work is currently being done to improve CO measurements to meet NASA's maximum allowable concentration of 10ppm and to extend to additional gases such as N2O, hydrocarbons, and polymer vapors.

Original languageEnglish
StatePublished - 2016
Event2016 Spring Technical Meeting of the Eastern States Section of the Combustion Institute, ESSCI 2016 - Princeton, United States
Duration: Mar 13 2016Mar 16 2016

Conference

Conference2016 Spring Technical Meeting of the Eastern States Section of the Combustion Institute, ESSCI 2016
Country/TerritoryUnited States
CityPrinceton
Period03/13/1603/16/16

Funding

Research at UCF was supported by financial assistance from Federal Aviation Administration Center of Excellence for Commercial Space Transportation (FAA COE-CST) with Ken Davidian and Nickolas Demidovich as program managers, and Florida Space Institute. The authors would like to acknowledge travel support provided by the ORAU. Z.L. thanks NSF and DOE SULI for partially supporting this effort. The Oak Ridge National Laboratory research was sponsored by the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Office, with Gurpreet Singh, Ken Howden, and Leo Breton as the Program Managers.

FundersFunder number
DOE SULI
Florida Space Institute
Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Office
National Science Foundation
U.S. Department of Energy
Oak Ridge Associated Universities
Federal Aviation Administration

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