Difference between revisions of "Minutes SHMS MC 1"
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| + | - Minutes of SHMS MC working group meeting 06/08/2011 - | ||
Participants: Mark, Howard, Peter, Tanja, Dave and Dipangkar | Participants: Mark, Howard, Peter, Tanja, Dave and Dipangkar | ||
Revision as of 08:54, 9 June 2011
- Minutes of SHMS MC working group meeting 06/08/2011 - Participants: Mark, Howard, Peter, Tanja, Dave and Dipangkar
1. Validation of single arm MC for the SHMS: It was felt that the existing single arm MC models of the SHMS neesd to be revalidated because there are discrepancies in the angle acceptance between various existing models. The validation will occur over the next two months with the goal of having a stable validated model by the Aug. Hall-C meeting. The following steps will be taken:
Mark will compare Dave Gaskell's COSY model agianst the Snake model Both models will be rationalized with the latest aperture numbers and other magnet parameters from Paul Brindza Dave will summarize the results of his model in a few slides, to be circulated to the group. Tanja will summarize the results of her earlier work in a few slides, to be circulated to the group. A wiki link will be created on the Hall-C wiki to organize all the validation work Once validated the code will be put in a CVS repository All work should be stored in the existing SHMS group disk space so that it is accessible to all in the group.
2. Once a validated model is available design of collimators and sieve slits can proceed
3. The validated model will be used to compare the 2 sieve slit option against the GEM tracker + 1 sieve slit option
4. The cosy reconstruction matrix elements will be optimzed using Mark's simplified fitter (sans PAW interface)
