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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w<br />
M O+<br />
MoF +<br />
II<br />
145<br />
...... ~ .......<br />
I 1<br />
MoFJ'<br />
7 - 1 - - -<br />
MoF.<br />
MnDF2+ MoOFZ<br />
MOF+ M"Oi+<br />
MOO+<br />
<strong>ORNL</strong>--DWG 67 -103403<br />
r-<br />
~<br />
.J. ....<br />
90 (00 110 120 ,130 140 150 160 170 180 490 XO<br />
ornu<br />
Fig. 11.1. Mass Spectra of Sample I1 (MoF3) During a Heating Cycle from 25OoC to 725°C.<br />
<strong>the</strong> MoOF, '/MoF3+, MoOF, t/MoF4t, and MoF5'<br />
peaks at 375°C is shown in Fig. 11.2. This shows,<br />
for illustrative purposes, <strong>the</strong> combined spectra for<br />
<strong>the</strong> various isotopes and compounds in <strong>the</strong> mass<br />
range from 150 to 194 amu. At 725OC <strong>the</strong> peak<br />
height for <strong>the</strong> MoF,+ relative to <strong>the</strong> height of <strong>the</strong><br />
Mop,' peaks as compared with <strong>the</strong> spectrum at<br />
375O allowed calculation of a tentative cracking<br />
patteni assigned to MoF,. This is seen only at<br />
elevated temperatures. An impurity at m/e - 167<br />
wiis assigned <strong>the</strong> probable fonnula Si 20F,.<br />
Mass analysis of <strong>the</strong>se species is facilitated by<br />
<strong>the</strong> unique isotopic abundance ratios of molybdenum<br />
isotopes and <strong>the</strong> difference of 3 amu between oxy-<br />
gen and fluorine. This yields, if one selects ad-<br />
jacent pairs of species from <strong>the</strong> Mo0,F2+/M~~OF3t/<br />
MoF4+ family of peaks, three unique peaks for each<br />
species, allowing a precise calculation of <strong>the</strong> peak<br />
height ratios for <strong>the</strong> "overlapping" peaks to be<br />
made. The dimer Mo,F, has, of course, <strong>the</strong> 15<br />
peaks which would be expected from <strong>the</strong> seven<br />
stable molybdenum isotopes. Figure 11.3 shows<br />
<strong>the</strong> good agreement between <strong>the</strong> calculated and <strong>the</strong><br />
-- I - r<br />
155 171 193<br />
m/e<br />
PHOTO 89172<br />
Fig. 11.2. Oscilloscope Trace of Mass Spectrum of<br />
Sample II (MoF3).