NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
KISS: Kinetics and Structure of Superagglomerates Produced by Silane and AcetyleneThe objective of this study is to understand the process of gas phase agglomeration leading to superagglomerates and a gel-like structure for microgravity (0-g) silane and acetylene flames. Ultimately one would apply this understanding to predicting flame conditions that could lead to the gas phase production of an aero-gel. The approach is to burn acetylene and silane and to analyze the evolution of the soot and silica agglomerates. Acetylene is chosen because it has one of the highest soot volume fractions and there is evidence of super agglomerates being formed in laminar acetylene flames. Silane has the advantage that silica particles are the major combustion product resulting in a particle volume fraction a factor of ten greater than that for a carbonaceous smoke.
Document ID
20010074066
Acquisition Source
Glenn Research Center
Document Type
Conference Paper
Authors
Mulholland, G. W.
(National Inst. of Standards and Technology Gaithersburg, MD United States)
Yang, J. C.
(National Inst. of Standards and Technology Gaithersburg, MD United States)
Scott, J. H.
(National Inst. of Standards and Technology Gaithersburg, MD United States)
Sivithanu, Y.
(En'Urga, Inc. West Lafayette, IN United States)
Date Acquired
August 20, 2013
Publication Date
May 1, 2001
Publication Information
Publication: Sixth International Microgravity Combustion Workshop
Subject Category
Inorganic, Organic And Physical Chemistry
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available