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Gravitational macrosegregation in binary Pb-Sn alloy ingotsA space shuttle experiment employing the General Purpose (Rocket) Furnace (GPF) in its isothermal mode of operation is manifested on MSL-3, circa 1989. The central aim of this experiment is to investigate the effect of reduced gravity levels on the segregation behavior in a slowly, and isothermally, cooled sample of a binary Pb-15 wt pct Sn alloy. This experiment should be able to simulate, in a small laboratory sample, some aspects of the segregation phenomena occurring in large industrial ingots. Ground-based experiments conducted in the single-cavity simulator of the GPF, in support of the microgravity experiment are described in detail. The results of the MSFC experiments are compared with other related experiments conducted at Case Western Reserve University (CWRS), wherein the isothermal constraints were relaxed. The isothermally processed samples indicate a small and gradual increase in fraction eutectic, and a corresponding increase in tin content, from the bottom to the top of the ingot. The radial variations are minimal near the ingot bottom, but there are large radial variations in the top half. In the CWRU experiments, more severe segregations, including segregation defects known as freckles. Follow up experiments employing the GPF without the isothermal constraints, or other suitably modified space shuttle hardware are suggested.
Document ID
19880053984
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Laxmanan, V.
(Case Western Reserve Univ. Cleveland, OH, United States)
Studer, A.
(Case Western Reserve Univ. Cleveland, OH, United States)
Wang, L.
(Case Western Reserve Univ. Cleveland, OH, United States)
Wallace, J. F.
(Case Western Reserve University Cleveland, OH, United States)
Winsa, E. A.
(NASA Lewis Research Center Cleveland, OH, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1987
Subject Category
Materials Processing
Accession Number
88A41211
Distribution Limits
Public
Copyright
Other

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