Proton Calorimetry/Meetings/2017/01/25: Difference between revisions
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** Drop in gain somewhere around 20kHz.  | ** Drop in gain somewhere around 20kHz.  | ||
* Finished analysing Caen ADC and waveform data from November 2016 runs:  | * Finished analysing Caen ADC and waveform data from November 2016 runs:  | ||
**   | ** http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_analysis.pdf  | ||
**   | ** http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_waveform_analysis.pdf  | ||
Latest revision as of 14:56, 25 January 2017
Minutes for UCL Proton Calorimetry Meeting, 25th January 2017 (D17, Physics & Astronomy, UCL)
Present
Simon Jolly, Anastasia Basharina-Freshville, Andreas Christou, Adam Knoetze, Matthieu Hentz
AC:
- Working on analysis of scope waveform data.
- ROOT will now identify bad pulses!
 - ROOT TSpectrum will analyse waveforms for double peaks based on histogram distribution.
 
 - Will next try and fit to good waveforms to train pulse filtering and integration.
 - Anastasia suggests looking at low and high rate files with no absorber.
 - Will also complete Java code to import binary files directly into ROOT: need to include input arguments.
 
AK:
- Looking at various output spectra from Caen detector emulator.
 - Trying to set spectrum of waveform magnitudes (Caen instructions plus trial and error...).
 - Taking average of "large" waveforms to produce mean waveform for emulator.
 - Detector emulator time resolution much coarser than scope data (~160MHz): need to extract subset of individual waveform data to produce approximation of our waveforms.
 - Next step is to put output of detector emulator into digitiser and try and recreate Clatterbridge results.
 - Will also replicate Anastasia's experiments with LED light pulser injected into scintillator+PMT.
 
MH:
- Specification of components for Clatterbridge beamline.
 - Need to check position and construction of dose monitors.
 - SJ will send current document to Clatterbridge and Carsten Welsch (Liverpool) for checking.
 
ABF:
- Looking into frequency-dependent gain from scope data for last Clatterbridge run.
 - Using LED light pulser to inject light into scintillator+PMT to corroborate gain changes:
- Results seem to confirm gain variation seen with experimental results.
 - Drop in gain somewhere around 20kHz.
 
 - Finished analysing Caen ADC and waveform data from November 2016 runs: