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ORNL-4191 - the Molten Salt Energy Technologies Web Site

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As in previous analyses of <strong>the</strong> reactor fuel, it<br />

is clear that a very high fraction of isotopes (such<br />

as *40Ba, 89Sr, 141Ce, 14'Ce, and "Sr) that form<br />

very stable and soluble fluorides is present in <strong>the</strong><br />

circulating fuel. As judged by <strong>the</strong> behavior of<br />

'I, <strong>the</strong> isotopes of iodine also seem to be present<br />

in a high fraction.<br />

On <strong>the</strong> o<strong>the</strong>r hand <strong>the</strong> more noble elements, such<br />

as Mo, Nb, Te, and Ru, are generally present in<br />

much lower fractions. It is worthy of note that<br />

<strong>the</strong>se materials seem to show a much wider scatter<br />

than do <strong>the</strong> "salt seekers"; this may indicate that<br />

<strong>the</strong>y are not present in true solution. It must also<br />

be noted that <strong>the</strong>se noble metals are present in<br />

considerable quantity in <strong>the</strong> gas stream and that<br />

<strong>the</strong>y adhere tenaciously to metal spe-' Limens exposed<br />

to <strong>the</strong>m. It is possible, <strong>the</strong>refore, that a<br />

considerable fraction of <strong>the</strong> material found in <strong>the</strong><br />

"salt" is due to <strong>the</strong> fact that <strong>the</strong> sampler is lowered<br />

and <strong>the</strong>n raised through this gas phase. It is<br />

possible that <strong>the</strong> relatively high values obtained<br />

for g9Mo, lo9Ru, and 132Te in FPll-45, where<br />

no gas was used, may be due to this phenomenon.<br />

This possibility will be verified, if possible, experimentally<br />

in <strong>the</strong> near future.<br />

9.3 EXAMINATION OF MSRE SURVEILLANCE<br />

SPECIMENS AFTER 24,000 Mwhr<br />

A second set of long-term surveillance speci-<br />

mens of MSRE graphite and Hastelloy N was ex-<br />

amined after exposure to circulating molten-salt<br />

fuel in an axial core position of <strong>the</strong> MSRE for<br />

24,000 Mwhr of power operation. During <strong>the</strong> last<br />

92 days of this exposure, <strong>the</strong> MSRE operated at a<br />

steady power of 7.2 Mw essentially without in-<br />

terruption, whereas power operation was frequently<br />

interrupted during <strong>the</strong> previous 7800-Mwhr expo-<br />

sure. Examinations of <strong>the</strong> specimens gave results<br />

very much like those previously reported after a<br />

7800-Mwhr exposure.' -'<br />

Examination of Graphite<br />

As before, three rectangular graphite bars were<br />

available for examination: a 9.5 x 0.47 x 0.66 in.<br />

bar from <strong>the</strong> middle of <strong>the</strong> core, and 4.5 x 0.47 x<br />

0.66 in. bars from <strong>the</strong> bottom (inlet) and top (out-<br />

let) of <strong>the</strong> cote. Visually, <strong>the</strong> graphite appeared<br />

undamaged except for occasional bruises incurred<br />

during <strong>the</strong> dismantling. The two 4.5-in.-long bars<br />

121<br />

gained 0.002 k 0.002 in. in length and 13 mg (0.03%)<br />

in weight. Metallographic examination showed no<br />

radiation or chemical alteration of <strong>the</strong> graphite<br />

structure and no evidence of surface films.<br />

X radiography of thin transverse slices showed<br />

occasional salt penetration into previously exist-<br />

ing cracks that happened to extend to <strong>the</strong> surface<br />

of <strong>the</strong> sample. Similar penetration was observed<br />

in control samples that were exposed to molten<br />

salt but were not irradiated. X-ray diffraction by<br />

th.e graphite surface exposed to fuel gave <strong>the</strong><br />

normal graphite lines except for a very slightly<br />

expanded lattice spacing. A few weak foreign<br />

lines that were probably due to fuel salt were<br />

observed. Autoradiography of <strong>the</strong> samples showed<br />

a high concentration of activity within 10 mils of<br />

<strong>the</strong> surface, with diffuse irregular penetration to<br />

<strong>the</strong> center of <strong>the</strong> cross section. These observa-<br />

tions confirmed previous demonstration of <strong>the</strong><br />

satisfactory compatibility of graphite with fis-<br />

sioning molten salt as far as damage and per-<br />

meation by fuel are concerned.<br />

concentration profiles for fission products in<br />

<strong>the</strong> graphite were determined by milling off layers,<br />

which were dissolved and analyzed radiochemically.<br />

Near <strong>the</strong> surface, layers as thin as 1 mil were ob-<br />

tained; far<strong>the</strong>r in, layers as thick as 10 mils were<br />

collected until a total depth of about 50 mils was<br />

reached. The predominant activities found were<br />

molybdenum, tellurium, ru<strong>the</strong>nium, and niobium.<br />

These elements can be classed as noble ele-<br />

ments since <strong>the</strong>ir fluorides (which are generally<br />

volatile) are relatively imstable. The practical<br />

concern, because of long-term neutron economy,<br />

is with g5Mo, 97Mo, ggTc, and "'Ru, but <strong>the</strong>se<br />

particular isotopes are ei<strong>the</strong>r stable or long-lived<br />

and thus were not amenable to direct analysis.<br />

However, we considered as sound <strong>the</strong> assumption<br />

that <strong>the</strong>ir deposition behavior was indicated by<br />

ei<strong>the</strong>r that of a radioactive isotope of <strong>the</strong> same<br />

element or that of a radioactive noble-metal pre-<br />

cursor with a suitable half-life.<br />

Over 99% of <strong>the</strong> noble-metal activities were en-<br />

countered within <strong>the</strong> first 2 or 3 mils of <strong>the</strong><br />

graphite surface; <strong>the</strong> same was true for 95Zr. This<br />

is illustrated in Figs. 9.1-9.1, The values for<br />

blanks shown in <strong>the</strong> figures were obtained from<br />

samples of about 0.2-g (1 mil) size that were<br />

milled from fresh unexposed graphite in <strong>the</strong> hot<br />

cell and with <strong>the</strong> equipment used for <strong>the</strong> irradiated<br />

specimens. The blanks show that <strong>the</strong> apparent<br />

tails on <strong>the</strong> curves for "Mo, "Nb, and '0611zu are

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