AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
CIRCE
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Entry time:
Tue Mar 6 15:29:55 2018
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<p>On 23/02/2018:</p> <p>We moved the target ladder to position 7, 5.019mm, with the alpha source facing downsteam.</p> <p>At 17:17 we started the DAQ for a 15 minute alpha spectrum on the downstream S2. Save name: /Remote_Objs/RData_1/180223172135</p> <p>The trigger rate ~ 160 Hz, Event Mult. = 5.8, Dead time = 0%</p> <p>Note: For both this alpha spectrum and the beam measurement at 3.45 MeV 7Li (See entry #20) the pulser test input was also plugged into the diode preamp, hence the pulser peak appears at a lower channel in the S2 spectra. It still does not overlap the alpha peaks.</p> <p>See attached "180223_Alpha_S2FrontStrip_ADC2CH20.png" for sample alpha spectrum of front S2 strip</p> <p>See attached "180223_Alpha_S2BackStrip_ADC4CH24.png" for sample alpha spectrum of back S2 strip</p> <p> </p> <p>In the S2 front strips we observed some additional peaks at lower channels ,~500, to the alpha peaks, but were unsure what they were. We decided to run a background to confirm whether this was caused by the source.</p> <p>We moved the target ladder to position 1, 95.010mm, to position the alpha source as far from the central beam axis as possible. We then collected a background run for 5 minutes 16 seconds. Save name: /Remote_Objs/RData_1/180223174450.</p> <p>We did not observe these low channel peaks in the background run, suggesting they are the result of the alpha source - perhaps a geometry effect.</p>
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Attachment 1:
180223_Alpha_S2FrontStrip_ADC2CH20.png
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Attachment 2:
180223_Alpha_S2BackStrip_ADC4CH24.png
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