Minutes SHMS MC 7

Minutes of SHMS MC working group meeting 11/15/2011

Participants: Dave, Dipangkar, Mark and Peter

1. Mark showed plots that demonstrated why the delta acceptance of the SNAKE and COSY models were looking different as observed during the previous meeting. The reason was the difference were the cuts in the detector HUT which were not being applied in the SNAKE model. Once those cuts are in place, the COSY and SNAKE distributions agree very well. The x at the focal plane agree remarkably well, although at different intermediate apertures in the dipole they can look somewhat different. The y distribution at the FP agree but have an small offset.

2.