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The Linear Collider Alignment and Survey (LiCAS) Project

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But water only follows local geoid...some parts of TESLA don't ....while NLC does not at all ... TESLA follows Earth's geoid. So cannot be used for TESLA. 7 March 2003 ... – PowerPoint PPT presentation

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Title: The Linear Collider Alignment and Survey (LiCAS) Project


1
The Linear Collider Alignment and Survey (LiCAS)
Project
  • Richard Bingham, Edward Botcherby, Paul Coe, John
    Green,
  • Grzegorz Grzelak, Ankush Mitra, John Nixon, Armin
    Reichold
  • University of Oxford
  • Andreas Herty, Wolfgang Liebl, Johannes Prenting
  • Applied Geodesy Group, DESY

2
Contents
  • Introduction
  • Survey and Alignment of a Linear Collider
  • Survey Concept
  • LiCAS System Overview
  • Frequency Scanning Interferometry (FSI)
  • Straightness Monitors (SM)
  • Simulation of LiCAS performance
  • Summary

3
Why do we need another collider ?
  • Whats wrong with the LHC ?
  • Its a high energy, high luminosity hadron
    collider
  • Good as a discovery machine eg Higgs Hunting
  • But hadron colliders are messy
  • Difficult to make precision measurements
  • Cannot determine quantum numbers of initial state

NEED A LEPTON COLLIDER
4
Physics with a (Linear) Lepton Collider
MH 120 GeV, 3104 pb-1 S/?B3.6 (5.0 105 pb-1)
  • LHC Can see 120 GeV Higgs
  • LC Can see 120 GeV Higgs more clearly

5
Why do we need a Linear Collider ?
  • Cant we build a Super-LEP ?
  • Synchrotron Radiation
  • For 1 Synchrotron radiation loss

LEP II Super-LEP
Energy 180 GeV 500 GeV
DE / Rev 1.5 GeV 5 GeV
Radius 4.3 km 255.8 km
6
The Super-LEP
LEP
Synchrotron radiation loss sets the size of a
Super-LEP Lets try a Linear Particle Accelerator
7
Requirements for a Linear Collider
  • To study interesting physics, LC must be
  • High Energy to create massive particles
  • High Luminosity to create large numbers of
    particles
  • LC must have
  • Large accelerating gradients
  • VERY small beam cross-sections at IP O(nm)

8
Proposed Linear Collider TESLA
X-FEL
  • Collider Length 33km
  • Beam Energy 500 GeV
  • Beam Luminosity 1034 cm-2 s-1
  • Beam Alignment at IP O(nm)
  • Collider Alignment Survey

200mm over 600m
9
Why is this hard ?
200mm over 600m
  • Temperature pressure gradients inside collider
    tunnel affect open-air measurements
  • A 600m line of sight can be bent by 4.5mm for
    0.1oC/m temperature gradient
  • Ground motion will misalign collider so survey
    must be quick

Light gets bent by air refraction
T
10
Ground Motion Effect on Luminosity
Time to reset collider
1week
2s
20s
11
Extra Survey Constraints
  • Confined space (also used as emergency escape)
  • Collider has mixture of straight and curved
    sections
  • Electrically noisy environment

12
When to Survey Accelerator
  • Tunnel Construction
  • Check tunnel has stopped settling
  • Accelerator Installation
  • Check component positions ( correct them)
  • Accelerator Maintenance
  • If a component is replaced the accelerator will
    be re-surveyed
  • Each step has to achieve 200mm over 600m
    precision
  • Accelerator Diagnostics
  • Check accelerator maintains alignment ( correct
    it)
  • Find out what went wrong

13
Traditional Accelerator Surveys
  • A team of surveyors using theodolites, laser
    trackers, etc
  • Make precision measurements of accelerator site
    and accelerator
  • A survey takes months to complete and requires a
    large team of people.
  • But this approach is not suited to LC because
  • Cannot achieve required accuracy
  • Slow
  • Manual
  • Large space required

14
Solutions Hydrostatic Levelling Systems
  • Traditional method to measure vertical alignment
  • But water only follows local geoidsome parts of
    TESLA dont
  • .while NLC does not at all

NLC
15
Other Solutions
  • Use a long stretched wire
  • The wire will sag under gravity Only good for
    horizontal alignment
  • Use a laser to align accelerator
  • In open-air, it will be refracted by temperature
    gradients
  • TESLA follows Earths geoid. So cannot be used
    for TESLA

16
Survey Procedure
  • Two-step Survey procedure
  • Survey equidistant tunnel wall markers via
    multiple overlapping measurements LiCAS Job
  • Measure collider components against wall makers
  • Advantage
  • The same procedure is employed during tunnel
    construction, collider installation, operation
    and maintenance

Accelerator wall
Survey Train
Accelerator
17
Survey Train
  • A survey train is used to perform the first step
  • Mechanical concept developed by DESY Geodesy
    Group
  • LiCAS provides an optical metrology for the train
  • Survey Train carries two systems
  • Frequency Scanning Interferometry
  • Makes 1D Length Measurements
  • Laser Straightness Monitors
  • Measures transverse displacements and rotations

18
Survey Train External Measurements
  • Each carriage measures the position of a
    reference marker in its own co-ordinates
  • Q How to tie reference marker co-ordinates
    together

Marker 1 at (x1,y1)
Marker 2 at (x2,y2)
1D FSI Length Measurements
Carriage 2
Carriage 1
19
Survey Train Internal Measurements
  • Use internal system to relative positions of
    carriages
  • Internal systems ties the external measurements
    together

Marker 1 at (x1,y1)
Marker 2 at (x2,y2)
1D FSI Length Measurements
SM Measurements
Carriage 1
Carriage 2 (xc2,yc2)
20
Survey Train LiCAS Systems
  • An Optical metrology system for survey of a
    linear Collider
  • Fast, automated high precision system
  • Can operate in tight spaces

Vacuum tube
21
Survey Implementation
Tunnel Wall
Reconstructed tunnel shapes (relative
co-ordinates)
22
Frequency Scanning Interferometry
  • Interferometric length measurement technique
  • Require precision of 1mm over 5m
  • Originally developed for online alignment of the
    ATLAS SCT tracker

Tunable Laser
Reference Interferometer L
Measurement Interferometer D
(Grid Line Interferometer (GLI))
Change of phase DFGLI
23
FSI Length Measurement
DFGLI
DFRef
24
FSI Thermal Drift Cancellation
  • Thermal effects add subtle systematic errors to
    FSI
  • Nanometre movements can contribute micron errors
    (µ (n/Dn) )
  • Use two lasers tuning in opposite directions to
    cancel thermal drift

25
FSI Thermal Drift Cancellation
DFGLI
DQ()
True Gradient
DQ(-)
Measured Gradient with Laser Tuning Up
Measured Gradient with Laser Tuning Down
DFRef
26
FSI 2-Laser Thermal Drift Cancellation
27
FSI ATLAS Implementation
28
FSI ATLAS Test Grid
  • 6 simultaneous length measurements made between
    four corners of the square.
  • 7th interferometer to measure stage position.
  • Displacements of one corner of the square can
    then be reconstructed.

29
FSI ATLAS Resolution
30
FSI ATLAS Resolution
  • Stage is kept stationary
  • RMS 3D Scatter
  • lt 1 mm

31
LiCAS FSI System
ATLAS FSI System
Laser 1
Laser 2
Reference Interferometer
Splitter Tree
piezo
detector
Uncollimated Quill
Collimated Quill
1m GLI
5m GLI
32
Erbium Doped Fibre Amplifiers
  • EDFA are optical power amplifiers
  • Used to amplify low power tunable laser
  • Standard equipment for Telecoms
  • but will it work for FSI ?

4I11/2
Pump 980nm
Decay
Single Telecoms Channel
4I13/2
Signal 1550nm
fluorescence
4I15/2
1610
Wavelength / nm
1530
33
Quill Collimation
  • Refractive
  • Reflective

Quill
Retroreflector
Reflective, off-axis paraboloid
34
Two Laser AM Demodulation
  • Need 2 lasers for drift cancellation
  • Have both lasers present use AM demodulation to
    electronically separate signals

M1
t0
t1
M2
Laser 1
Laser 2
Detector
t0
t1
35
Two Laser AM Demodulation
  • Amplitude Modulation on FSI fringe
  • _at_ 40 80 kHz (now) 0.5 1MHz (later)
  • High Pass Filter
  • FSI fringe stored as amplitude on
  • Carrier (à la AM radio)
  • Demodulation reproduces FSI Fringes

36
Results of Demodulation
Both signals have same frequency !!
Demodulation of modulated laser does not effect
interferometer signal
37
Reference Interferometer Phase Extraction
  • Reference Interferometer is FSIs yard-stick
  • Must measure interferometer phase precisely
  • Uses standard technique of Phase-Stepping

Step1 I(ftrue-1.5Df) Step2 I(ftrue-0.5Df) Step3
I(ftrue0.5Df) Step4 I(ftrue1.5Df)
Reference Interferometer mirror moved in 4 equal
sized steps
ftrue
38
Software Phase Extraction
  • Telecoms laser tunes linearly
  • Extract phase with software phase-stepping

39
FSI Extensions for LiCAS
  • Collimation optics for quill outputs
  • Move to Telecoms wavelength (1510nm 1640nm)
  • Telecoms fibres and equipment are cheaper
  • Exploit cheap, high quality lasers
  • Reduce drift errors
  • x300 increase in continuous tuning range (0.24nm
    130nm)
  • x3000 increase in tuning rate (100 GHz/min
    5THz/sec)
  • New features such as Amplitude Modulation (AM)
  • Use Erbium Doped Fibre Amplifiers (EDFA)
  • Modular power distribution

40
Straightness Monitors
  • Used to measure carriage transverse translations
    and rotations
  • Require 1mm precision over length of train

Rotation Spots move opposite directions
Translation Spots move same direction
CCD Camera
41
SM Rotations about Z
  • Use two parallel beams to measure rotation about
    z-axis

SM beams coming out of the screen
Image of beam spots observed on CCD Camera
42
SM Splitter Configurations
  • Single Beam Splitter End carriage
    retroreflector
  • Double Beam Splitter per carriage
  • Pro Measurements independent of splitter angle
  • Con Retroreflector introduces unknown
  • transverse walk to all carriages
  • Pro No retroreflector No unknown walks
  • Con The angle of each beam-splitter in each has
  • to be determined 12 extra
    calibration
  • constants

43
SM Low Coherence Beams
  • Low coherence length diode lasers are used to
    avoid CCD interference
  • Stray reflections off surfaces can interfere if
    coherent

The two reflected rays can interfere if coherent
The two reflected rays can interfere if coherent
Beam- Splitters
CCD Chip
CCD Glass Face-plate
44
SM Interference Rings
  • Laser with long coherence length.
  • Interference rings observed on CCD
  • Laser with low coherence length
  • No interference structure is observed

45
SM Demagnification Lenses
  • CCD cameras are ½ square.
  • A long collimated beam Þ large beam
  • This can be larger than the CCD
  • Use of demagnification lenses increase dynamic
    range
  • Lenses must be high quality to prevent beam
    distortion

46
SM Results
47
SM Stability Results
48
SM Extensions for LiCAS
  • Use of two parallel beam to measure rotations
    about z-axis
  • Two beam-splitter configurations are under
    investigation
  • Simple SM under test
  • Low coherence length laser under test
  • Demagnification lenses are being designed

49
Simulations (of single car)
  • FSI resolution 1mm, SM resolution 1 mm
  • Weak measurement of rotation around z-axis due to
    small separation between two beams on CCD
  • Tilt meters resolution 1mrad

Without tilt meters
With 1-Axis tilt meters
50
Simulations of Train over 600m
Error on positions lt 200mm after 600m
51
Summary
  • Future linear colliders require precision survey
    and alignment
  • The LiCAS group is developing optical metrology
    techniques to address this in collaboration with
    DESY
  • Proposed solution is being developed for TESLA
    but can be applied to any collider
  • Preliminary results have been encouraging
  • LiCAS is now PPRP approved ?
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