ASIC meeting June 14, 2010

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Revision as of 19:57, 13 June 2010 by Yvhaarle (Talk | contribs) (Remaining tests)

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Meeting Time and Place

Monday June 11, 2010 at 10:00am At Jefferson Lab, the meeting will be held in room F326-327

Connections

To connect from the outside, please use ESNET
1.) ESNET: 8542553
2.) Phone:
+1-800-377-8846 : US
+1-888-276-7715 : Canada
+1-302-709-8424 : International
then enter participant code: 77438230# (remember the "#")

Agenda

Status of the new ASIC

Performance Plots for the ASIC at CMU

The following links go to pages that compare the performance of the older preamplifier to the newest version of the ASIC. We note that the interposer board was not used for the older preamplifier and that the Struck FADCs we have at CMU are set to a scale such that 1 volt coresponds to about 4000 channels. We note that the new preamplifier does not exceed ~2000 channels here because the output voltage is now (apparently) limited to 0.5V.

The following sets of plots were taken simply by swapping the old and new preamplifier on the CDC. The high voltage settings were the same and the gas mixture were the same for both. For the case of the cosmics with a reduced gain in the new ASIC, we would expect the location of the minimum ionizing peak for cosmics to go down by about a factor of three. Oddly, by just about any reasonable measure, it has moved up. We find this extremely confusing.

2050V - cosmics - max amplitude histogram

old preamp, cosmics, amplitude, 50/50 Ar/CO2, 2050V
new preamp, cosmics, amplitude, 50/50 Ar/CO2, 2050V

2050V- cosmics - energy

old preamp, cosmics, energy, 50/50 Ar/CO2, 2050V
new preamp, cosmics, energy, 50/50 Ar/CO2, 2050V

The following plots are taken with the Fe-55 source for the same pairs of configuration. Here we are limited by a great deal of overflow and saturation in both cases so it is difficult to draw a strong conclusion on where the gain really is on the new ASIC

Efficiency Plots for the CDC

The following plot is taken from our NIM article that shows the chamber efficiency as a function of the high voltage setting for various gas mixtures. As can be seen, for the optimal gas mixture (around 50/50), the plateau starts at about 2100 V and there is no efficiency below around 1900V.

HV plateau curve aka efficiency plots.

Status from the FDC

gas gain

efficiency

plateau

amplitude and energy histograms with cosmics & Fe-55

scaling to experiment

Remaining tests

  • At CMU, we are in the process of repeating the efficiency measurements with the new ASIC to see if the combination of the reduced noise and apparent increased gain could be mapped onto the appropriate dynamic range for the CDC. It takes at least a week to collect the cosmic data, and then sometime to analyze.
  • These are all not tracked results so one can compare to previous spectra - fadc range is half the range as in previous spectra:
new preamp, new fadc range (=1/2 old one), amplitudes, 50/50 Ar/CO2, 1750V
new preamp, new fadc range (=1/2 old one) , energy, 50/50 Ar/CO2, 1750V
new preamp, new fadc range (=1/2 old one), amplitudes, 50/50 Ar/CO2, 1850V
new preamp, new fadc range (=1/2 old one) , energy, 50/50 Ar/CO2, 1850V
new preamp, new fadc range (=1/2 old one), amplitudes, 50/50 Ar/CO2, 1950V
new preamp, new fadc range (=1/2 old one) , energy, 50/50 Ar/CO2, 1950V


  • And now the icing -> Low statistics efficiency plot (hv -curve) of channel 7 (had most tracks going through it)
new preamp, new fadc range (=1/2 old one), Efficiency plot or HV curve, 50/50 Ar/CO2

Schedule to completion

Impact to

detector tests

to installation

Minutes