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ORNL-4191 - the Molten Salt Energy Technologies Web Site

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significantly, indicating clearly <strong>the</strong> collimating<br />

effect. The flat top at <strong>the</strong> peak was of <strong>the</strong> same<br />

width as <strong>the</strong> collimator hole and represents <strong>the</strong><br />

resolution of <strong>the</strong> collimator when used with a point<br />

source.<br />

Gamma Scan of <strong>the</strong> MSRE Heat Exchanger<br />

A gamma radiation scan was made on May 19,<br />

1967, over <strong>the</strong> area in <strong>the</strong> reactor cell containing<br />

<strong>the</strong> fuel-to-coolant-salt heat exchanger and fuel<br />

salt line 102.<br />

To accomplish <strong>the</strong> radiation scan, <strong>the</strong> portable<br />

maintenance shield was located over an opening<br />

in <strong>the</strong> reactor cell above <strong>the</strong> heat exchanger, and<br />

<strong>the</strong> collimator and gamma ion chamber were in-<br />

stalled in a hole in <strong>the</strong> portable shield. Measure-<br />

ments were made by moving <strong>the</strong> portable shield<br />

until <strong>the</strong> ion chamber was directly above <strong>the</strong> de-<br />

OR N L- 0 WG 6 7- l I791<br />

PORTAB1.E , [/ ION CIiAMBFii<br />

/<br />

48-in. COLLIMAl-OR TUBE<br />

( 4V3. in. OD)<br />

-.) ~~ --<br />

INCREASING<br />

Y<br />

HEAT EXCHANGER<br />

6 ft -3 in. FF 101<br />

FF 102<br />

I<br />

18 it-9 in<br />

I<br />

13 ft-2 in. 1<br />

Fig. 2.5. Source-Detector Geometry for Gamma Scan<br />

of MSRE Heat Exchanger.<br />

43<br />

sired points in <strong>the</strong> cell. Figure 2.5 shows <strong>the</strong><br />

vertical distances from <strong>the</strong> tip of <strong>the</strong> ion chamber<br />

to items in <strong>the</strong> cell.<br />

The orientation of <strong>the</strong> various ion chamber<br />

traverses of <strong>the</strong> cell along with lines of equal<br />

radiation levels are shown superimposed over <strong>the</strong><br />

heat exchanger and line 102 in Fig. 2.6. It wilI<br />

be noted that <strong>the</strong> maximum radiation levels were<br />

3.5 r/hr above <strong>the</strong> heat exchanger center line<br />

and 300 mr/hr above line 102. When <strong>the</strong> collimator<br />

was removed, <strong>the</strong> radiation level at <strong>the</strong> top of <strong>the</strong><br />

hole in <strong>the</strong> portable shield was 100 r/hr.<br />

These results show that <strong>the</strong> collimated gamma<br />

ion chamber measures radiation levels with very<br />

good resolution of position, even in <strong>the</strong> presence<br />

of high background radiation levels. Therefore,<br />

this method of radiation measurement should be<br />

useful in locating accumulatiot~s of fission products<br />

in reactor components and in planning maintenance<br />

operations.<br />

Gamma <strong>Energy</strong> Spectrum Scan of <strong>the</strong><br />

MSRE Heat Exchanger<br />

On May 20, 1967, a gamma energy spectrometer<br />

was set up over <strong>the</strong> same area in <strong>the</strong> reactor cell,<br />

and measurements were made at several points<br />

over <strong>the</strong> fuel-to-coolant-salt heat exchanger. This<br />

exploratory experiment was made primarily to<br />

evaluate <strong>the</strong> method.<br />

The measurements were made by using a 3- by<br />

3-in, NaI crystal and photomultiplier tube mounted<br />

in a lead shield which had a collimating hole<br />

'/32 in. in diameter and 7 in. long under <strong>the</strong> crystal.<br />

The array was mounted on <strong>the</strong> hole in <strong>the</strong> portable<br />

shield in <strong>the</strong> same manner as <strong>the</strong> collimator for<br />

<strong>the</strong> gamma scan described earlier.<br />

There were strong, well-defined peaks at about<br />

0.48 and 0.78 Mev corresponding to Io3Ru and<br />

"Zr-95Nb. The resolution of <strong>the</strong> NaI crystal was<br />

not good enough to determine whe<strong>the</strong>r <strong>the</strong> second<br />

peak was from g5Nb only or from <strong>the</strong> "Zr decay<br />

chain. The energy resolution could be improved<br />

by using a different crystal, since <strong>the</strong> collimator<br />

did not appear to degrade <strong>the</strong> peaks. The problem<br />

of assigning absolute disintegration rates to <strong>the</strong>se<br />

isotopes is complicated by <strong>the</strong> geometrical arrangement<br />

of <strong>the</strong> heat exchanger and heaters, ihe<br />

effect of gamma energy on absorption by <strong>the</strong> collimator,<br />

<strong>the</strong> source distribution in <strong>the</strong> heat exchanger,<br />

and <strong>the</strong> counter efficiency. It is believed,<br />

however, that some measure of <strong>the</strong> relative

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