Optics Meeting Mar 13 2024 1100AM ET

From Moller Wiki
Revision as of 18:48, 24 March 2024 by Armd (Talk | contribs) (Minutes)

Jump to: navigation, search

Back to Main Page >> Optics Meetings

>> following meeting

>> previous meeting

Agenda

  1. database update [Bill [[1]]]
  2. Optics Fit Update [Vassu][2]

Attendance

  1. David, Kate, Bill, Vassu, Sayak, Tyler, Zuhal, Buddhika, Ciprian, Andrew, Juliette

Minutes

  1. (Bill) Discussion on detector numbering scheme (important for MYSQL database as well as remoll). Decide to adopt a GEM numbering scheme that tracks the magnet coil numbering: detectors start with 1 (not 0), increase as one goes clockwise when looking downstream. The first GEM number (and first Trigger Scintillator number) would be in its "open sector" measurement position (starting location) between toroid magnet coil 1 (which is the first one in the clockwise direction from beam left, i.e. it is at a small +x and a small positive y location) and coil 2. Call this the "zero degree" rotation angle for the GEM rotator. The 28-fold pion detectors also start in the same azimuthal location. We don't know about the Main Detector numbering scheme. The ShowerMax detectors are not matched the pion detectors at present in remoll, but we can plan on asking for that to be changed.
  2. (Bill) Discussed ideas for information for the database. In the run-by-run part of the database want 4 angular positions to be defined - the 0 degree, two intermediate positions, and then one position which is a complete sector (2pi/7) rotation from the original. Perhaps they can just be labeled as "A", "B","C","D" rotations. Vassu notes that the intermediate positions may not be at exactly steps of (2pi/21), as we want to enure that all relevant sieve hole images will be clearly seen in each rotation (each sieve hole's image must be clearly seen in active GEM area for at least one rotation angle). We don't need to specify exact rotation angles now, but we should look at this again now that we have the final sieve hole pattern defined. Will probably eventually host the database at JLab behind the gateway after construction of the GEMs, so it can be easily used and updated during the experiment. Would want a mirror site off-site from Jlab.
  3. (Vassu) new simulation runs with mew 12C foil locations are done.

Meeting link information

See email invitation, or contact David Armstrong, Kate Evans, or Jennifer McAllister for Zoom link