ORNL-4191 - the Molten Salt Energy Technologies Web Site
ORNL-4191 - the Molten Salt Energy Technologies Web Site
ORNL-4191 - the Molten Salt Energy Technologies Web Site
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Fig. 18.2.<br />
carbides. 1000~.<br />
carbides. Figure 18.4 shows <strong>the</strong> correspondence<br />
between <strong>the</strong> morphologies of <strong>the</strong> extracted precipitate<br />
and that indicated by <strong>the</strong> autoradiograph.<br />
A selected area diffraction pattern and an electron<br />
probe microanalyzer trace are also included.<br />
This type of precipitate has not yet been identified,<br />
but <strong>the</strong> diffraction pattern does not correspond<br />
to MbC. A comparison of <strong>the</strong> microprobe<br />
results with standards shows that <strong>the</strong> noncarbon<br />
constituents are about 90% Mo and 10% Cr. However,<br />
some M,C carbides are also present after<br />
high-temperature anneals and exist in several<br />
morphologies.<br />
We are concluding our investigation of precipitation<br />
in standard Hastelloy N and will be evaluating<br />
<strong>the</strong> information generated and attempting<br />
to relate our observations to observed changes in<br />
mechanical properties.<br />
Because of <strong>the</strong> attractive in-reactor properties<br />
of <strong>the</strong> titanium-modified Hastelloy N, we are expanding<br />
our studies to include this material. Optical<br />
metallography shows <strong>the</strong> alloy to be quitc<br />
free of precipitate. Initial electron microscopy<br />
studies of two experimental heats revealed that<br />
220<br />
Extraction Replica from Hastelloy N (Heat 5065)Aged 4 hr at 1600OF. All precipitates are M 6 C<br />
a considerable amount of very thin, fine precip-<br />
itate was present in <strong>the</strong> grain boundaries. This<br />
was rarely detected in thin-foil transmission mi-<br />
croscopy but was readily seen by <strong>the</strong> extractim<br />
replica technique.<br />
Selected area electron diffraction studies on<br />
<strong>the</strong> fine grain-boundary precipitates have revealed<br />
at least two phases, which exist in many mor-<br />
phologies. Although <strong>the</strong>se precipitates have not<br />
been positively identified, indications are quite<br />
good that Ti,O is one phase and that it is present<br />
in conjunction with <strong>the</strong> second type. The o<strong>the</strong>r<br />
phase has a face-centered cubic structure with a<br />
lattice parameter of about 4.27 A and may exist<br />
independently of <strong>the</strong> former. Considering chemical<br />
composition, TIC seems to be <strong>the</strong> most likely com-<br />
position of <strong>the</strong> second phase. However, <strong>the</strong> re-<br />
ported lattice parameter for Tic is 4.33 A, com-<br />
pared with our measured value of 4.27 A. TiN and<br />
TiB have lattice parameters more closely related<br />
to <strong>the</strong> measured value; however, chemical analyses<br />
of <strong>the</strong> heats involved show <strong>the</strong> boron and nitrogen<br />
contents to be extremely low.