Difference between revisions of "Thursday, April 17, 2014 1:00pm EDT"
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(New page: Previous meeting: Thursday, April 3, 2014 1:00pm EDT == Agenda == * Background radiation simulations == Minutes == <br><br> Return to Teleconferences <br> Return to [[MOLLER at...) |
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* Background radiation simulations | * Background radiation simulations | ||
+ | * Collaboration meeting talks | ||
== Minutes == | == Minutes == | ||
+ | |||
+ | * Talks | ||
+ | ** Seamus will give talk on Q^2/tracking and state of the software | ||
+ | ** Rupesh will be out of the country | ||
+ | ** Nickie can present the radiation background studies as well as the quick radiation results we have | ||
+ | |||
+ | * Background Radiation | ||
+ | ** Nickie can reproduce general energy deposited | ||
+ | ** Should look at hybrid coil next | ||
+ | ** Energy deposited on hall wall and near the detectors | ||
+ | ** Neutrons/background out of collimators | ||
+ | ** Net flux from concrete shielding | ||
+ | ** Nickie will contact Rakitha about this work done in PREX | ||
+ | |||
+ | * looked at [http://ace.phys.virginia.edu/MollerSpectrometer/306 | ||
+ | * We should put in lead donuts into the simulation, look at the new geometry | ||
<br><br> Return to [[Teleconferences]] | <br><br> Return to [[Teleconferences]] | ||
<br> Return to [[MOLLER at 11 GeV E09-005]] | <br> Return to [[MOLLER at 11 GeV E09-005]] |
Latest revision as of 13:28, 24 April 2014
Previous meeting: Thursday, April 3, 2014 1:00pm EDT
Agenda
- Background radiation simulations
- Collaboration meeting talks
Minutes
- Talks
- Seamus will give talk on Q^2/tracking and state of the software
- Rupesh will be out of the country
- Nickie can present the radiation background studies as well as the quick radiation results we have
- Background Radiation
- Nickie can reproduce general energy deposited
- Should look at hybrid coil next
- Energy deposited on hall wall and near the detectors
- Neutrons/background out of collimators
- Net flux from concrete shielding
- Nickie will contact Rakitha about this work done in PREX
- looked at [http://ace.phys.virginia.edu/MollerSpectrometer/306
- We should put in lead donuts into the simulation, look at the new geometry
Return to Teleconferences
Return to MOLLER at 11 GeV E09-005