Difference between revisions of "Thursday, November 10, 4:00pm ETD"

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(Agenda)
Line 5: Line 5:
 
** modified field determination code to be somewhat general - can rotate the field easily now
 
** modified field determination code to be somewhat general - can rotate the field easily now
 
** coded the upstream torus in GDML (see [http://ace.phys.virginia.edu/MollerSpectrometer/202 elog 202])
 
** coded the upstream torus in GDML (see [http://ace.phys.virginia.edu/MollerSpectrometer/202 elog 202])
*** plan to also hard-code to maintain the ability to use hard-coded geometry
+
*** plan to also hard-code to maintain the ability to continue to use it - but I REALLY like the GDML
 
*** will compare the results for hard-coded vs. GDML defined  
 
*** will compare the results for hard-coded vs. GDML defined  
 +
*** the GDML write from GEANT4 did NOT create tesselated volumes, but the parameterization is lost
 
*** if we code directly in GDML it is really easy to parameterize things AND to modularize things   
 
*** if we code directly in GDML it is really easy to parameterize things AND to modularize things   
 +
 
* Collimator/field configuration comparison update (Sereres)
 
* Collimator/field configuration comparison update (Sereres)
 
** Plots of asymmetries
 
** Plots of asymmetries
** Plots of ee/ep separation and peak widths  
+
** Plots of ee/ep separation and peak widths
  
 
== Minutes ==
 
== Minutes ==

Revision as of 10:49, 9 November 2011

Agenda

Presentations:

  • Updates to mollersim (geometry)
    • rotated the phi-defining collimator so that there is a closed section to beam left
    • modified field determination code to be somewhat general - can rotate the field easily now
    • coded the upstream torus in GDML (see elog 202)
      • plan to also hard-code to maintain the ability to continue to use it - but I REALLY like the GDML
      • will compare the results for hard-coded vs. GDML defined
      • the GDML write from GEANT4 did NOT create tesselated volumes, but the parameterization is lost
      • if we code directly in GDML it is really easy to parameterize things AND to modularize things
  • Collimator/field configuration comparison update (Sereres)
    • Plots of asymmetries
    • Plots of ee/ep separation and peak widths

Minutes



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