Title: The Linear Collider Alignment and Survey (LiCAS) Project
1The 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
2Contents
- 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
3Why 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
4Physics 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
5Why 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
6The Super-LEP
LEP
Synchrotron radiation loss sets the size of a
Super-LEP Lets try a Linear Particle Accelerator
7Requirements 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)
8Proposed 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
10Ground Motion Effect on Luminosity
Time to reset collider
1week
2s
20s
11Extra Survey Constraints
- Confined space (also used as emergency escape)
- Collider has mixture of straight and curved
sections - Electrically noisy environment
12When 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
13Traditional 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
14Solutions 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
15Other 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
16Survey 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
17Survey 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
21Survey Implementation
Tunnel Wall
Reconstructed tunnel shapes (relative
co-ordinates)
22Frequency 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
23FSI Length Measurement
DFGLI
DFRef
24FSI 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
25FSI Thermal Drift Cancellation
DFGLI
DQ()
True Gradient
DQ(-)
Measured Gradient with Laser Tuning Up
Measured Gradient with Laser Tuning Down
DFRef
26FSI 2-Laser Thermal Drift Cancellation
27FSI ATLAS Implementation
28FSI 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.
29FSI ATLAS Resolution
30FSI ATLAS Resolution
- Stage is kept stationary
- RMS 3D Scatter
- lt 1 mm
31LiCAS FSI System
ATLAS FSI System
Laser 1
Laser 2
Reference Interferometer
Splitter Tree
piezo
detector
Uncollimated Quill
Collimated Quill
1m GLI
5m GLI
32Erbium 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
33Quill Collimation
Quill
Retroreflector
Reflective, off-axis paraboloid
34Two 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
35Two Laser AM Demodulation
- Amplitude Modulation on FSI fringe
- _at_ 40 80 kHz (now) 0.5 1MHz (later)
- FSI fringe stored as amplitude on
- Carrier (à la AM radio)
- Demodulation reproduces FSI Fringes
36Results 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
38Software Phase Extraction
- Telecoms laser tunes linearly
- Extract phase with software phase-stepping
39FSI 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
40Straightness 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
41SM 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
42SM 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
43SM 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
44SM Interference Rings
- Laser with long coherence length.
- Interference rings observed on CCD
- Laser with low coherence length
- No interference structure is observed
45SM 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
46SM Results
47SM Stability Results
48SM 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
49Simulations (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
50Simulations of Train over 600m
Error on positions lt 200mm after 600m
51Summary
- 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 ?