Difference between revisions of "Optics Meeting May 23 2023 200PM ET"
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| + | # Kate fixed the oddities related to symmetry hole hit locations in GEM plane for default (ideal) magnetic field, by using the simple mean of the data rather then the centroid of Gaussian fits - now the results all make sense. | ||
| + | # The Technical Board approved the sieve design, but subsequently Kent had a number of additional questions. We discussed many of them | ||
| + | and came up with some additional plots to generate: [https://moller.jlab.org/cgi-bin/DocDB/private/ShowDocument?docid=1124]. Transmission of the sieve design to MIT engineering will await completion of these tasks. | ||
=Meeting link information= | =Meeting link information= | ||
Revision as of 15:13, 24 May 2023
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Contents
[hide]Agenda
- questions about optics calibration [Kent]
- short update on sieve hole symmetry using raw data instead of gaussian fits [Kate] [1]
Attendance
David, Kate, Vassu, Bill, Tyler, Ryan, Michael D, Ciprian, Kent, Sayak, Andrew, Juliette.
Minutes
- Kate fixed the oddities related to symmetry hole hit locations in GEM plane for default (ideal) magnetic field, by using the simple mean of the data rather then the centroid of Gaussian fits - now the results all make sense.
- The Technical Board approved the sieve design, but subsequently Kent had a number of additional questions. We discussed many of them
and came up with some additional plots to generate: [2]. Transmission of the sieve design to MIT engineering will await completion of these tasks.
Meeting link information
Meeting URL
https://cwm.zoom.us/j/97259755403?pwd=WTRqVHJnZ3RQa1IwNHdMQjJuQm9FZz09
Meeting ID: 972 5975 5403
Passcode: 4937
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