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University of Wisconsin-Madison

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Presentation on theme: "University of Wisconsin-Madison"— Presentation transcript:

1 University of Wisconsin-Madison
Transfer Line Studies James N. Bellinger University of Wisconsin-Madison 12 December 2008

2 Summary No Cocoa yet Hand fits show relative rotation among Endcap disks Can identify backwards DCOPS James N. Bellinger 12-December-2008

3 Description 6 Transfer lines at 60 degree intervals around the outside of the detector 12 DCOPS on each Transfer line 4 on each Endcap 4 on selected MABs 2 Lasers on each Transfer line Call them the Plus and Minus lasers 72 DCOPS in all, with 144 readings Oriented so the 1/3 CCD pair measure Rφ, 2/4 pair measures radius James N. Bellinger 12-December-2008

4 Problems A few DCOPS were unreadable
Sometimes LV to Barrel DCOPS was off Lasers were shadowed in places: no signal Laser direction not always adjustable James N. Bellinger 12-December-2008

5 Layout YB-2 YB-0 YB+0 YB+2 Laser Laser ME-4 ME-3 ME-1 ME+1 ME+2 ME+3
James N. Bellinger 12-December-2008

6 Cocoa Model of Transfer Lines
Is not ready yet. James N. Bellinger 12-December-2008

7 Data Selection From CRAFT run
Select interval with field at 3.8T in which laser directions don’t drift much Select interval with field off ditto (CRAFT data taking was two runs: would have been a single run if the power hadn’t failed) Plot the distribution of mean values subject to quality cuts Background area < pixel x counts Signal area>0 and <500000 Sigma >39 pixels and < 220 Mean>0 pixels and < 2048 James N. Bellinger 12-December-2008

8 Endcap-only study For each magnetic field state
For each Endcap, use the laser at that end For each Transfer line, use the 4 DCOPS Reorient the CCD information to match DCOPS mounting For each CCD, fit the means at the 4 DCOPS and find the residuals Average the residuals of opposite pairs of CCDs Interpret these residuals as displacements of the DCOPS and plot them James N. Bellinger 12-December-2008

9 Plus Endcap DCOPS displacements
Vectors plotted to show dX Ring diameter is not relevant Largest vector has length given in the title Vectors at center average of rest, to estimate disk displacement James N. Bellinger 12-December-2008

10 Minus Endcap DCOPS displacements
ME-1 and ME-2 show relative rotation about .5 mrad ME-1 and ME-2 show relative dislocation of about 3mm James N. Bellinger 12-December-2008

11 Change with field Change in relative displacement with field is mostly
radial ME+3 and ME+2 move oppositely (EXPECTED!) The disk YE+2 bends, and the DCOPS positions are cantilevered James N. Bellinger 12-December-2008

12 Change of Raw Beam Positions
ME-4 ME-3 Difference between field on and off for Minus endcap at each station, as a function of position (φ) around the disk. ME-4 next to laser: little change ME-3: about 3mm ME-2: about 3mm ME-1: about 8mm ME-2 ME-1 James N. Bellinger 12-December-2008

13 Connecting Across Select data from 16-August
Not all profiles are usable For Transfer Line 1, only connect with Up/Down CCD data (Rφ) Both lasers reach across for Line 1, so I can compare their results directly James N. Bellinger 12-December-2008

14 Example of Transfer Line Profiles
CCD0 CCD0 data reaches across, but CCD1 gets blocked somewhere CCD1 James N. Bellinger 12-December-2008

15 DCOPS orientations This one is odd: DCOPS directions data suggests
other direction DCOPS directions aren’t the same along a line James N. Bellinger 12-December-2008

16 Deviations from Linear Fit
10 Stations had data for Up/Down CCDs (not always both of the pair) for both laser beams Estimated laser tilt Averaged CCD values if both present Corrected for laser tilt if not Fit for each laser and plotted the deviations from the fits James N. Bellinger 12-December-2008

17 Oddity RMS=3.3mm Difference is huge at this point. If I assume the
DCOPS is backwards, the points fit very well. RMS=1.0mm Difference in deviations found using Plus and Minus laser fits James N. Bellinger 12-December-2008

18 Conclusions When the beam is unobstructed we can get useful information out of the system Once mounting variations are understood we’ll have a better measure of the resolution of the system James N. Bellinger 12-December-2008


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