Figure 4 - uploaded by Luis Otiniano
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Right:Measured secondary cosmic ray charge spectrum (one hour) in the second detector with secondary trigger (green) and an with out (red)
Contexts in source publication
Context 1
... charge histogram of a WCD is obtained by time integration of the individual pulses measured in the WCD (in ADC units). As we expect that cosmic rays produce pulses with at least three bins of time we introduce a secondary trigger for the next bin (after trigger) at adquisition level with the same value of primary trigger (65 ADC), see figure 4. This reduce the data files size from 200 Mb per hour to 20 Mb. ...
Context 2
... charge histogram of a WCD is obtained by time integration of the individual pulses measured in the WCD (in ADC units). As we expect that cosmic rays produce pulses with at least three bins of time we introduce a secondary trigger for the next bin (after trigger) at adquisition level with the same value of primary trigger (65 ADC), see figure 4. This reduce the data files size from 200 Mb per hour to 20 Mb. ...
