Difference between revisions of "More information can be found here"
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= Current (optimized) matrices = | = Current (optimized) matrices = | ||
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| + | == LHRS == | ||
Replace in matrix [4] the line: | Replace in matrix [4] the line: | ||
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This is the coefficient that relates delta with theta (xptar) fp linearly. We did this to get rid of a slope we saw in Emiss vs. xptar. | This is the coefficient that relates delta with theta (xptar) fp linearly. We did this to get rid of a slope we saw in Emiss vs. xptar. | ||
| − | [ | + | [6] [http://web.mit.edu/reynier/www/Tritium_optics_matrices/LHRS_current_optics.html current LHRS matrix] |
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| + | == RHRS == | ||
| − | [ | + | [7] [http://web.mit.edu/reynier/www/Tritium_optics_matrices/RHRS_current_optics.html current RHRS matrix] |
Revision as of 15:03, 26 July 2018
The following are the matrices that we used during the online analysis of the experiment:
[HERE] [1]
[HERE] [2]
The following is the LHRS matrix optimized by GMp
[HERE] [3]
The following is an optimization that Shujie did on the GMp LHRS matrix [3] using the standard procedure for optimizing the angles and the sieve runs taken during MARATHON
[HERE] [4]
The following is the RHRS matrix optimized by GMp
[HERE] [5]
Current (optimized) matrices
LHRS
Replace in matrix [4] the line:
D 1 0 0 -6.863500E-02 2.633700E-01 1.096600E-02 -7.253300E-02
with:
D 1 0 0 4.932426E-03 2.633700E-01 1.096600E-02 -7.253300E-02
This is the coefficient that relates delta with theta (xptar) fp linearly. We did this to get rid of a slope we saw in Emiss vs. xptar.
