Difference between revisions of "Thursday, April 24, 2014 1:00pm EDT"
From Hall A Wiki
(→Agenda) |
(→Minutes) |
||
(2 intermediate revisions by the same user not shown) | |||
Line 9: | Line 9: | ||
== Minutes == | == Minutes == | ||
+ | |||
+ | * Talks | ||
+ | ** Rakitha - PREX background overview | ||
+ | ** Seamus - State of Software | ||
+ | ** Seamus - Tracking, collimation | ||
+ | ** Juliette - Spectrometer | ||
+ | ** Kent - Polarimetry | ||
+ | ** Nilanga - GEMs | ||
+ | ** Mark - Beam monitoring | ||
+ | ** Kent or Mark - Qweak experience, beam haloing | ||
+ | ** Bob - DAQ | ||
+ | ** Gordon - Source? | ||
+ | ** Nickie - Background and shielding simulations, ideas for present design (Tyler's work) | ||
+ | ** Ernie - Engineering | ||
+ | ** Javier - Project Managment | ||
+ | ** Michael - Detector work | ||
+ | ** Rupesh - Positioning systematics | ||
+ | ** Dustin - Showermaxing | ||
+ | ** Robin - Project integration | ||
+ | ** Accelerator - Coming back up and parity quality beam? | ||
+ | |||
<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 13:58, 24 April 2014
Previous meeting: Thursday, April 17, 2014 1:00pm EDT
Agenda
- Background radiation simulations - review geometry such as lead placement
- Collaboration meeting talks
- Nickie [1]
- Rakitha [2]
Minutes
- Talks
- Rakitha - PREX background overview
- Seamus - State of Software
- Seamus - Tracking, collimation
- Juliette - Spectrometer
- Kent - Polarimetry
- Nilanga - GEMs
- Mark - Beam monitoring
- Kent or Mark - Qweak experience, beam haloing
- Bob - DAQ
- Gordon - Source?
- Nickie - Background and shielding simulations, ideas for present design (Tyler's work)
- Ernie - Engineering
- Javier - Project Managment
- Michael - Detector work
- Rupesh - Positioning systematics
- Dustin - Showermaxing
- Robin - Project integration
- Accelerator - Coming back up and parity quality beam?
Return to Teleconferences
Return to MOLLER at 11 GeV E09-005