Difference between revisions of "Optics Meeting Dec 13 2022 230PM ET"
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=Attendance= | =Attendance= | ||
| + | David Kate, Zuhal, Bill | ||
=Minutes= | =Minutes= | ||
| + | # (David) Final Design review (Internal) went well. | ||
| + | # (Kate) Noticed that Jason B's slides for FDR said that the sieve/blockers would be 100% W; we should check, since we believe the plan is 90%W/10%Cu. Not a problem for us, of course, 100%W has even shorter radiation length. | ||
| + | # (Bill) Working in getting the GEM frames into remoll, and defining a detector numbering scheme for GEMs | ||
| + | # (Kate) Some evidence that the problem with the low-energy Livermore libraries is when low-energy particles are in magnetic fields, they don't propagate properly. Has implemented (with help from Zuhal) and is now testing a two-step simulation that should be able to bypass this problem. | ||
| + | # probably will have meeting next week, last one before holiday break. | ||
=Meeting link information= | =Meeting link information= | ||
Latest revision as of 19:57, 16 December 2022
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Contents
[hide]Agenda
Attendance
David Kate, Zuhal, Bill
Minutes
- (David) Final Design review (Internal) went well.
- (Kate) Noticed that Jason B's slides for FDR said that the sieve/blockers would be 100% W; we should check, since we believe the plan is 90%W/10%Cu. Not a problem for us, of course, 100%W has even shorter radiation length.
- (Bill) Working in getting the GEM frames into remoll, and defining a detector numbering scheme for GEMs
- (Kate) Some evidence that the problem with the low-energy Livermore libraries is when low-energy particles are in magnetic fields, they don't propagate properly. Has implemented (with help from Zuhal) and is now testing a two-step simulation that should be able to bypass this problem.
- probably will have meeting next week, last one before holiday break.
Meeting link information
Meeting URL
https://cwm.zoom.us/j/97259755403?pwd=WTRqVHJnZ3RQa1IwNHdMQjJuQm9FZz09
Meeting ID: 972 5975 5403
Passcode: 4937
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