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Thermal imaging of afterburning plumes

Authors: E. AJDARI; E. GUTMARK; T. PARR; K. WILSON; K. SCHADOW;

Thermal imaging of afterburning plumes

Abstract

Afterburning and nonafterburning exhaust plumes were studied experimentally for underexpanded sonic and supersonic conical circular nozzles. The plume structure was visualized using thermal imaging and regular photography. Thermal emission by the plume is mainly dependent on the presence of afterburning. Temperature and reducing power (or unoxidized fuel content) of the exhaust gases, in addition to the nozzle configuration, determine the structure of the plume core, the location where the afterburning is initiated, its size, and intensity. The temperature, through chemical kinetics, determines the presence of afterburning and its initiation location. Its effect is especially critical in marginally afterburning plumes. The fuel content determines the size and intensity of the plume when afterburning occurs. Comparison between single shot and average thermal images of the plume show that afterburning is a highly turbulent combustion process.

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Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
13
Top 10%
Top 10%
Average
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