Difference between revisions of "Meeting 1/27/22 - COMTRA"
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== Schedule ==
== Schedule ==
* Joe reviewed schedule again, beam test window
* Joe reviewed schedule again, beam test window shorter at UITF, now from Jun 1 - Oct 31, see slide [[media:220127_COMTRA.pptx]]
Revision as of 12:34, 27 January 2022
- Joe reviewed schedule again, beam test window is shorter at UITF, now from Jun 1 - Oct 31, see slide 4 media:220127_COMTRA.pptx
- Joe proposed moving polarimeter test to non-dispersive "straight" section to avoid any energy dependent position jitter
- Shaun showed UITF beam line, identified how we could remove single spool in 4' pass-through, leaving irradiation line intact
- Joe is confirming this with Matt as first priority location
- Riad showed model/pics of ceramic break & radiator we'd like to use, 6mm thick copper, 1" flat surface for beam, approved for 10 MeV/100uA with cooling
- Riad will discuss with Eric if 6mm okay - then we move to fabricate second ceramic break & radiator
DAQ Procurement List - Chris and Riad
- List of components needed to build two portable DAQ systems: media:ComptonTransPol_DAQ_PurchaseNeeds_2022Jan.xlsx
Detector update - Eric
- I am in contact with the Alpha-Spectra company which was providing BGO crystals for a local project we had in Orsay. This is a US company which provides crystals with a guaranteed 8-9% resolution. At the time we were investigating for an order they were less expensive than Saint-Gobain and turned-out to be more performant (we performed dedicated measurements to test this).
- They should be back to me shortly with information about availability of improved radiation hardness crystals as well as radiation limits of the crystals they are currently providing.
- It should be noted that litterature about radiation aging of BGO crystals indicates that after a rapid loss of about 20% of transmission, the performance is kind of stable. Some experiments chose to first irradiate crystals to operate in that regime.
- We may need tools to control the overall stability of the experimental signal... dedicated cosmic ray calibration run or light illumination... too early stage to provide a direction of answer, but this should be kept in mind.