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sphenix-emcal-l - Re: [Sphenix-emcal-l] sPHENIX EMCal meeting on Tuesday

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Subject: sPHENIX EMCal discussion

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  • From: Craig Woody <woody AT bnl.gov>
  • To: Sean Stoll <stoll AT bnl.gov>
  • Cc: sphenix-emcal-l AT lists.bnl.gov
  • Subject: Re: [Sphenix-emcal-l] sPHENIX EMCal meeting on Tuesday
  • Date: Wed, 14 Mar 2018 08:30:07 -0400

Sean,
  Thanks for making the measurement of the light guide transmission so quickly. Admittedly we should have checked this before, but the light guides came in so late that we didn't really think about this at the time. From your plot it does look like the NN light guide has lower transmission, but since the lower transmission extends to very long wavelengths, I worry whether this is just a surface effect. I presume Bill machined and polished the ends of the sample you measured ? Also, I presume you avoided the screw hole in all cases ?
   Just as a reminder, it was decided at the "Light Guide Design Review" to switch to the UVT material based on measurements that were done with completely different material than the one actually used to manufacture the light guides we got from the supplier. They were based on samples of UVT and UVA acrylic that we had on hand (or maybe Bill ordered) that were irradiated with gammas up to 1 Mrad (far higher than we will ever see at RHIC). If you look at the radiation induced absorption coefficient from those measurements, the difference between UVA and UVT is imperceptible at 100 Krad.
    I'm not so sure the comparison of the transmission of the 4 samples you measured yesterday is telling us the whole story, and a 9% loss in light output won't explain our current problems with the lack of the detector response at low energies, but we may want to revisit the transmission issue of the light guides before ordering more of them.

Craig

On 3/13/2018 7:25 PM, Sean Stoll wrote:
I added some slides to the Indico page for today's mtg comparing the optical transmission of the V2.1 lightguides to the V2.0 lightguides. Bottom line - they have ~9% lower absolute transmission at the BCF12 emission peak (though they transmit further into the UV.  As a reminder, we selected the UVT material because the transmission edge is further from the BCF12 emission peak, and so will be less likely to change over time with accumulated gamma exposure.

Sean


On 3/11/2018 3:40 PM, Sickles, Anne M wrote:
Hi,

We’ll have an sPHENIX EMCal meeting on Tuesday.  The primary item for discussion is the progress on the data taking at Fermilab.  I expect a discussion of the current status led by John.  Jin, could you provide a summary of the up to date plots from the slack channel?

The agenda is here:

https://indico.bnl.gov/event/4355/

Best,
Anne
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