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Diploma thesis in Physics submitted by Florian Freundt born in ...

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5 Results 5.5. Noble gases<br />

3<br />

He [% atm. air]<br />

4<br />

He [% atm. air]<br />

40<br />

Ar [% atm. air]<br />

Aug Sep Oct Nov Dec Jan Feb Mar Apr May<br />

110<br />

105<br />

100<br />

95<br />

90<br />

105<br />

100<br />

95<br />

90<br />

105<br />

100<br />

95<br />

90<br />

Aug Sep Oct Nov Dec Jan Feb Mar Apr May<br />

Date<br />

20<br />

Ne [% atm. air]<br />

22<br />

Ne [% atm. air]<br />

36<br />

Ar [% atm. air]<br />

Aug Sep Oct Nov Dec Jan Feb Mar Apr May<br />

110<br />

105<br />

100<br />

95<br />

90<br />

105<br />

100<br />

95<br />

90<br />

105<br />

100<br />

95<br />

90<br />

Aug Sep Oct Nov Dec Jan Feb Mar Apr May<br />

Figure 5.8: Noble gas concentrations of atmospheric air samples relative to literature values<br />

from Porcelli et al. [2002] for 3 He, 4 He, 20 Ne, 22 Ne, 36 Ar and 40 Ar. All isotopes show an<br />

underestimation of roughly 2 %.<br />

tube volume than A23-I, the measured <strong>in</strong>let pressure is actually 0.6 mbar lower, <strong>in</strong>dicat<strong>in</strong>g a<br />

pressure overestimation on sample A23-I. A comparison of the noble gas concentrations calculated<br />

for these two samples shows that A23-I displays a shift relative to A23-III <strong>by</strong> roughly -2 %<br />

on most noble gas isotopes. Samples A20-IV and A21-VIII show elevated noble gas concentrations<br />

compared with samples from the same depth and roughly the same time as well, however<br />

compar<strong>in</strong>g samples from different sampl<strong>in</strong>g dates can only deliver a vague <strong>in</strong>dication at best. To<br />

quantify the observed behavior of slowly decreas<strong>in</strong>g pressure read<strong>in</strong>gs the Keller gauge and the<br />

<strong>in</strong>let volume were re<strong>in</strong>stalled <strong>in</strong> the mass spectrometer preparation l<strong>in</strong>e and eight atmospheric<br />

air samples were opened. This experiment was unable to replicate the previously observed effect:<br />

the read<strong>in</strong>gs for those <strong>in</strong>stantaneously vented samples did not decrease. However this led to the<br />

observation that the Keller gauge is highly sensitive to its spatial orientation, show<strong>in</strong>g a 1 mbar<br />

difference when rotated <strong>by</strong> 180 ◦ , possibly add<strong>in</strong>g to the observed shift <strong>in</strong> atmospheric noble gas<br />

values.<br />

It was deemed most likely that the read<strong>in</strong>g of the <strong>in</strong>let pressure was executed prematurely, but<br />

consistently, lead<strong>in</strong>g to a systematical overestimation of sample gas amount and there<strong>by</strong> caus<strong>in</strong>g<br />

the offset displayed <strong>by</strong> the atmospheric air samples. Therefore all measured samples’ <strong>in</strong>dividual<br />

noble gas isotope values discussed below (except those that vented slowly) were standardized to<br />

the mean fitted values of the measured atmospheric air.<br />

59<br />

Date

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