Difference between revisions of "Friday, May 11, 2018 2PM ET"

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(Minutes)
 
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==Agenda==
 
==Agenda==
* Simulation concerns
+
* Simulation coding updates
* Beamline backgorund
+
* Shielding update by Cameron (SBU simulation elog 34 - UVA elog https://ace.phys.virginia.edu:80/MollerSpectrometer/373)
 
* Air/Vacuum Study: [https://hallaweb.jlab.org/doc-private/ShowDocument?docid=327 slides]
 
* Air/Vacuum Study: [https://hallaweb.jlab.org/doc-private/ShowDocument?docid=327 slides]
  
Line 20: Line 20:
  
 
Minutes:
 
Minutes:
*
+
 
 +
Updates from Cameron
 +
* Modular geometry implementation using text files and scripts
 +
** Used in shielding optimization by Cameron
 +
** It's available in SBU git repository
 +
* Beam dump is implemented in the remoll
 +
* Cameron is looking at the sky shine from the apparatus and the beam dump see simulation elog 34 for plots
 +
** currently shielding and beam dump background is separated to reduce the simulation time.
 +
* Finalize the shielding by July and August then obtain Photon background in the detector plane
 +
* Generate estimate on sky-shine with current shielding (PREX style estimate)
 +
** Then we run it with Pavel to get his estimate
 +
* Then get feedback from Engineers on the shielding design
 +
* Waiting on engineers for the beam-line update then we can implement it on simulation
 +
* Wouter fixed some issues related multi threading and root Tree I/O
 +
 
 +
Updates from Ciprian
 +
* using Helium to replace a DS vacuum
 +
** Ciprian simulated it and compared with air (DS vacuum can around DS magnet) and vacuum with He
 +
** He filled bag for DS magnet and then between detector and magnet are better than just air and worse little more than vacuum
 +
 
 +
 
  
  

Latest revision as of 14:46, 11 May 2018

Previous meeting: Friday, April 27, 2018 2PM ET

Media:KK's MOLLER Task List.pdf

Task List Summary


Agenda

Attendance:

Attendance: Rakitha, Sakib, Chandan, KK, Ciprian, Kent, Dustin,

Minutes

Minutes:

Updates from Cameron

  • Modular geometry implementation using text files and scripts
    • Used in shielding optimization by Cameron
    • It's available in SBU git repository
  • Beam dump is implemented in the remoll
  • Cameron is looking at the sky shine from the apparatus and the beam dump see simulation elog 34 for plots
    • currently shielding and beam dump background is separated to reduce the simulation time.
  • Finalize the shielding by July and August then obtain Photon background in the detector plane
  • Generate estimate on sky-shine with current shielding (PREX style estimate)
    • Then we run it with Pavel to get his estimate
  • Then get feedback from Engineers on the shielding design
  • Waiting on engineers for the beam-line update then we can implement it on simulation
  • Wouter fixed some issues related multi threading and root Tree I/O

Updates from Ciprian

  • using Helium to replace a DS vacuum
    • Ciprian simulated it and compared with air (DS vacuum can around DS magnet) and vacuum with He
    • He filled bag for DS magnet and then between detector and magnet are better than just air and worse little more than vacuum





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