development of micro-pattern gaseous detectors – gem - LMU
development of micro-pattern gaseous detectors – gem - LMU
development of micro-pattern gaseous detectors – gem - LMU
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42 Chapter 4 Energy Resolution and Pulse Height Analysis<br />
180<br />
160<br />
140<br />
120<br />
100<br />
80<br />
60<br />
40<br />
20<br />
55Fe Pulse Height<br />
dE<br />
| = 0.1771<br />
E Kα<br />
Cu anode seg<br />
preamp: Canberra<br />
cm<br />
kV<br />
Edrift<br />
= 1.25<br />
cm<br />
kV<br />
Etrans1,2<br />
= Eind<br />
= 2.00<br />
Δ U<strong>gem</strong>3=<br />
330 V<br />
Δ U<strong>gem</strong>2=<br />
330 V<br />
Δ U<strong>gem</strong>1=<br />
330 V<br />
data_<strong>gem</strong>_0221_pulseheight_fit<br />
Entries 19368<br />
Mean 340<br />
RMS 145.3<br />
χ 2 / ndf 980.2 / 550<br />
p0 272 ± 0.6<br />
p1 50 ± 0.0<br />
p2 8 ± 0.0<br />
p3 20.03 ± 0.50<br />
p4 194.5 ± 1.8<br />
p5 66.53 ± 1.78<br />
K α norm 139.4 ± 1.7<br />
K α mean 414.8 ± 0.8<br />
K α σ 31.2 ± 0.6<br />
p9 22.36 ± 2.44<br />
p10 482.7 ± 2.6<br />
p11 25 ± 0.2<br />
muon<br />
Mn K<br />
Mn Kα<br />
Mn K<br />
α esc.<br />
0<br />
0 100 200 300 400 500 600 700 800<br />
voltage [0.244mV]<br />
Figure 4.3: 55 Fe pulse height spectrum as taken with Canberra2004 preamplifier. All peaks are resolved. An<br />
energy resolution <strong>of</strong> dE/E = 17.7% for Kα is observed.<br />
for all tested setups.<br />
<br />
dE<br />
= 0.20 ± 0.03 (4.3)<br />
E FWHM<br />
The statistical limit gives a lower limit for the resolution. The relative mean error <strong>of</strong> a Poisson<br />
distribution is given by [Leo 94]:<br />
σ<br />
µ = 1<br />
√ µ<br />
with the mean µ and the standard deviation σ. Considering the fact that the energy <strong>of</strong> a single Kα<br />
photon can be identified with an ionization <strong>of</strong> µ = N = 223 molecules <strong>of</strong> the filling gas, one receives<br />
theoretically a lower limit for the relative resolution at FWHM:<br />
dE<br />
E<br />
<br />
FWHM<br />
= 2.35 ·<br />
1<br />
õ<br />
<br />
= 2.35 ·<br />
<br />
1<br />
√N<br />
= 2.35 ·<br />
β<br />
(4.4)<br />
1<br />
√ 223 = 0.1576 . (4.5)<br />
The factor 2.35 corresponds to the former presented relation <strong>of</strong> the standard deviation <strong>of</strong> a Gaussian<br />
distribution and the full width at half maximum. Inclusion <strong>of</strong> the Fano factor F [Fano 47] leads to:<br />
σ 2 corr = F · µ . (4.6)<br />
where F characterizes the detecting gas as a function <strong>of</strong> all possible processes <strong>of</strong> particle in the<br />
medium, i.e. including photon excitation [Leo 94]. In the case <strong>of</strong> pure Argon the Fano factor has a<br />
value <strong>of</strong> [Hash 84]:<br />
F = 0.23 . (4.7)