Difference between revisions of "Thursday, November 10, 4:00pm ETD"
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*** the GDML write from GEANT4 did NOT create tesselated volumes, but the parameterization is lost | *** 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 | ||
+ | * Changing code to write volume numbers of sensitive volumes to root file - need a better way of identifying them? | ||
+ | ** using 0-999 for actual detectors (possibly 0-99 for plane detectors and 100-999 for pieces quartz?, tracking?) | ||
+ | ** using 1000-1999 for collimators | ||
+ | ** using 2000-???? for coils | ||
<br> | <br> | ||
* Collimator/field configuration comparison update (Sereres) | * Collimator/field configuration comparison update (Sereres) |
Revision as of 10:53, 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
- Changing code to write volume numbers of sensitive volumes to root file - need a better way of identifying them?
- using 0-999 for actual detectors (possibly 0-99 for plane detectors and 100-999 for pieces quartz?, tracking?)
- using 1000-1999 for collimators
- using 2000-???? for coils
- Collimator/field configuration comparison update (Sereres)
- Plots of asymmetries
- Plots of ee/ep separation and peak widths
Minutes
Return to Teleconferences
Return to MOLLER at 11 GeV E09-005