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development of micro-pattern gaseous detectors – gem - LMU

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3.5. Methods <strong>of</strong> Signal Analysis 37<br />

3.5 Methods <strong>of</strong> Signal Analysis<br />

Signals by the triple GEM detector and recorded with the flash ADC are processed for further studies<br />

with the following s<strong>of</strong>tware algorithm : an inverse Fermi-function is fitted to the rising edge:<br />

f (x) =<br />

par0<br />

exp par1−x<br />

par2<br />

+ par3 (3.6)<br />

which can be seen in Fig. 3.12. Due to the characteristics <strong>of</strong> the flash ADC, namely its 12bit range and<br />

1 GHz sampling frequency, the axes scaled with a factor mADC = 0.244 mV and 1 ns, respectively.<br />

The behavior <strong>of</strong> the fit function is determined by four parameters, starting with par0 that reflects the<br />

maximum <strong>of</strong> the signal, i.e. the pulseheight.<br />

par 3<br />

par 0<br />

par 2<br />

par 1<br />

> 3 σ max<br />

mean 1<br />

mean 2<br />

Figure 3.12: A typical signal generated by 55 Fe in the GEM detector and recorded with the FADC. The inverse<br />

Fermi-function is shown in red, fitted to the rising edge.<br />

The second parameter par1 provides the inflection point <strong>of</strong> the pulse and therefore a possibility for<br />

calculating the exact event time. In the measurements presented in this work, the signal time should<br />

stay constant, as for cosmics the implemented trigger scintillator deliver a fast signal. This holds also<br />

for the 55 Fe source measurements since in this case the signal is triggering its acquisition.<br />

In the inverse Fermi-function the par2 represents the rise time <strong>of</strong> the signal. Solving equation 3.6<br />

for given values <strong>of</strong> 10% and 90% <strong>of</strong> the maximum pulseheight, one gets a factor <strong>of</strong> 4.4 which has to<br />

multiplied with par2 for receiving the signal’s risetime in this range. The added forth parameter par3<br />

corresponds the <strong>of</strong>fset <strong>of</strong> the preamplifier. In order to record a complete pulse spectrum for measurements<br />

<strong>of</strong> cosmic muons including also very small signals, every pulse passing the discriminator in the<br />

hardware chain was recorded without any further s<strong>of</strong>tware discrimination since every signal triggered<br />

by the scintillators can be considered a real event.<br />

This is not necessarily true for X-ray measurement, where no scintillators are triggering but the first

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