sct endcap module initial alignments using survey data
DESCRIPTION
SCT Endcap Module Initial Alignments Using Survey Data. Paul S Miyagawa University of Manchester. Outline. Objectives Available survey data Calculation of alignment constants Comparison with CSC constants Summary and future work. Objectives. - PowerPoint PPT PresentationTRANSCRIPT
SCT Endcap Module Initial Alignments Using Survey Data
Paul S MiyagawaUniversity of Manchester
11 December 2006 ATLAS Software & Computing Workshop 2/13
Outline
• Objectives• Available survey data• Calculation of alignment constants• Comparison with CSC constants• Summary and future work
11 December 2006 ATLAS Software & Computing Workshop 3/13
Objectives
• Extensive survey data available for SCT endcap modules and discs
• Combine the survey data to produce “as-built” module-on-disc (level-3) alignments
• Compare with the distributions used for CSC production
• Use alignments as initial step in alignment algorithms
11 December 2006 ATLAS Software & Computing Workshop 4/13
Module Survey Data (1)• Modules consist of two (or
four) wafers mounted at an angle of 40 mrad– (For outer and middle
modules, each wafer is split into two parts)
• Hole and slot used to mount the module on disc
Nominal values
Parameter Tolerance Outer Middle Short Middle Inner
mhx (mm) 0.020 -78.136 71.708 41.764 45.060
mhy (mm) 0.020 0.000 0.000 0.000 0.000
msx (mm) 0.100 62.244 -66.672 -96.616 -34.320
msy (mm) 0.020 0.000 0.000 0.000 0.000
midxf (mm) 0.010 0.000 0.000 0.000 0.000
midyf (mm) 0.005 -0.040 -0.053 -0.652 0.000
stereo (mrad) 0.130 -20.000 -20.000 -20.000 -20.000
11 December 2006 ATLAS Software & Computing Workshop 5/13
Module Survey Data (2)• Modules surveyed
during assembly at Manchester, NIKHEF and Geneva
• Survey information on positions of wafers, hole + slot, angle between wafers
• Uncertainties in module construction < O(10 μm)
11 December 2006 ATLAS Software & Computing Workshop 6/13
Disc Survey Data (1)• Modules mounted on disc
in three rings– 40 modules each in inner
and middle rings, 52 in outer ring
– Outer and inner rings mounted on front face of disc, middle ring on rear face
• At each position on disc, main/secondary pins insert into hole/slot on module
• 2 reference holes define survey coordinates– Holes also used to align
discs within the endcap
11 December 2006 ATLAS Software & Computing Workshop 7/13
Disc Survey Data (2)• Discs surveyed during
assembly at Liverpool and NIKHEF
• Positions of pins and reference holes surveyed on disc
• Uncertainties in pin positions O(60 μm)– Should be dominant
over module uncertainties
11 December 2006 ATLAS Software & Computing Workshop 8/13
Athena Conventions• Level-3 AlignableTrans-
forms define translations and rotations of modules in local frame
• Centre of rotations taken to be stereo centre on rφ face of module– Strips of rφ face point
along radial direction– Strips of stereo face
rotated 40 mrad• Transforms are for entire
module; not available separately for each face of a module– Cannot reflect shift of
stereo centre or non-nominal angle between wafers
rφ
y
stereo
x
X
Y
Z
y
x
z
11 December 2006 ATLAS Software & Computing Workshop 9/13
Stereo Centre of Module• Stereo centre defined to be
intersection of central strips of each wafer
• Shift in wafer positions relative to each other causes shift in stereo centre– Positions of overlaps
relative to stereo centre are unaffected
– Endpoints of strips relative to stereo centre are changed
• Leads to inefficiency at one end of strips
• Cannot be reflected by AlignableTransforms
11 December 2006 ATLAS Software & Computing Workshop 10/13
Angle Between Wafers• Central axis of module
chosen such that angle between wafers is symmetric about nominal angle
• Non-nominal angle affects positions of overlaps– Cannot be reflected by
AlignableTransforms
nominal
actual
11 December 2006 ATLAS Software & Computing Workshop 11/13
Alignment Parameters• Calculated in-plane
translations and rotations for modules– Translations < O(100 μm)– Rotations O(400 mrad)– Distributions are (vaguely)
Gaussian– Largely determined by
positions of pins on disc• Still need to complete
verification of data– Using Michal Dwuznik’s
viewer– Running alignment
algorithm on this set of misalignments
11 December 2006 ATLAS Software & Computing Workshop 12/13
Comparison with CSC Numbers• CSC misalignment set
used flat distributions• estimates for CSC
misalignments were slightly pessimistic
• CSC misalignments are random; survey misalignments are correlated– Relative alignment
between modules could be used as a constraint
type of misalignment
half-width
dx 100 μm
dy 100 μm
dγ 1 mrad
11 December 2006 ATLAS Software & Computing Workshop 13/13
Summary and Future Work• Extensive survey data available for SCT endcap modules and discs
– Uncertainties in module construction < O(10 μm)– Uncertainties in disc construction
• Combined survey data to produce “as-built” in-plane level-3 alignments– Translations < O(100 μm)– Rotations O(400 mrad)– Roughly Gaussian distributions– Numbers used for CSC misalignments were slightly pessimistic
• AlignableTransforms not available separately for each face of a module– Cannot reflect shift of stereo centre or non-nominal angle between
wafers
• Work to come– Complete verification of data– Compare reconstruction performance on real data with survey
misalignments versus nominal geometry