Radiation Temperature and Extinction of Transient Gaseous Diffusion Flames in Microgravity

Arvind Atreya; David A Everest; Sanjay Agrawal; Michael K Anderson

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NASA NTRS · 19970020557

Radiation Temperature and Extinction of Transient Gaseous Diffusion Flames in Microgravity

Arvind Atreya·David A Everest·Sanjay Agrawal·Michael K Anderson

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Abstract

The absence of buoyancy-induced flows in micro-g and the resulting increase in the reactant residence time significantly alters the fundamentals of many combustion processes. Substantial differences between 1-g and micro-g flames have been reported in experiments on candle flames, flame spread over solids, droplet combustion and others. These differences are more basic than just in the visible flame shape. Longer residence times and higher concentration of combustion products in the flame zone create a thermochemical environment which changes the flame chemistry and the heat and mass transfer processes. Processes such as flame radiation (and its interaction with flame chemistry), that are often ignored under normal gravity, become very important and sometimes even controlling. This is particularly true for conditions at extinction of a micro-g diffusion flame.

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Arvind Atreya, David A Everest, Sanjay Agrawal, Michael K Anderson. 1997-05-01. Radiation Temperature and Extinction of Transient Gaseous Diffusion Flames in Microgravity. https://ntrs.nasa.gov/citations/19970020557

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