Difference between revisions of "Radiation Simulation Meeting September 17 2018"

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==Agenda==
 
==Agenda==
* Rakitha's summary slides
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# Rakitha's summary [https://moller.jlab.org/wiki/images/Radiation_Benchmark.pdf slides]
* Kent's notes on summary slides
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#* Ideal = 40cm lead, 50 cm concrete, 75cm poly
* Cameron MOLLER log entry [https://ace.phys.virginia.edu:80/MollerSpectrometer/377 | elog:377]
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#* need to pay attention to lead collar.  Potential source for sky shine, also slit scattering
 +
#* Bare minimum reduces side of lead.  All others remain the same.  Slide 17 summarizes results from this configuration.
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#* "side wall" detector uses a 1/2 meter radius cut at the beam dump entrance.
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#* results for LH2 only: used magnetic fields, but no other material than target.
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# Kent's [https://moller.jlab.org/wiki/images/Notes180917.pdf notes] on Rakitha's slides
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# Cameron MOLLER log entry [https://ace.phys.virginia.edu:80/MollerSpectrometer/376 elog:376] (no shielding) [https://ace.phys.virginia.edu:80/MollerSpectrometer/377 elog:377] (with full shielding)
  
 
==Attendance:==
 
==Attendance:==

Latest revision as of 14:49, 26 September 2018

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Agenda

  1. Rakitha's summary slides
    • Ideal = 40cm lead, 50 cm concrete, 75cm poly
    • need to pay attention to lead collar. Potential source for sky shine, also slit scattering
    • Bare minimum reduces side of lead. All others remain the same. Slide 17 summarizes results from this configuration.
    • "side wall" detector uses a 1/2 meter radius cut at the beam dump entrance.
    • results for LH2 only: used magnetic fields, but no other material than target.
  2. Kent's notes on Rakitha's slides
  3. Cameron MOLLER log entry elog:376 (no shielding) elog:377 (with full shielding)

Attendance:

Attendance: Rakitha, Cameron, Cip, Kent, KK




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