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SSME Propellant Path Leak DetectionThe primary objective of this phase of the investigation is the experimental validation of techniques for detecting and analyzing propellant path external leaks which have a high probability of occurring on the SSME. The selection of candidate detection methods requires a good analytic model for leak plumes which would develop from external leaks and an understanding of radiation transfer through the leak plume. One advanced propellant path leak detection technique is obtained by using state-of-art technology of infrared (IR) thermal imaging systems combined with computer, digital image processing and expert systems for the engine protection. The feasibility of the IR leak plume detection will be evaluated on subscale simulated laboratory plumes to determine sensitivity, signal to noise, and general suitability for the application. The theoretical analysis was undertaken with the objective of developing and testing simple, easy-to-use models to predict the amount of radiation coming from a radiation source, background plate (BP), which can be absorbed, emitted and scattered by the gas leaks.
Document ID
19960020647
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Roger Crawford
(Center for Advanced Space Propulsion Tullahoma, TN United States)
Ahmad Ali Shohadaee
(Center for Advanced Space Propulsion Tullahoma, TN United States)
W T Powers
(Center for Advanced Space Propulsion Tullahoma, TN United States)
Date Acquired
August 17, 2013
Publication Date
October 31, 1995
Publication Information
Publication: Center for Advanced Space Propulsion
Subject Category
Propellants and Fuels
Spacecraft Propulsion And Power
Accession Number
96N71230
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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