monalisa david urner paul coe matthew warden armin reichold oxford university

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MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

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Page 1: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

MONALISA

David UrnerPaul Coe

Matthew WardenArmin Reichold

Oxford University

Page 2: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

STATUS: New Design

• More traditional Michelson setup leads to nice results.

• Integration of many interferometer into one node more difficult –

• A compact version is ready and shows promise.

Page 3: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Parallel Michelson

Originalconcept

Inputbeam

PZT

Mechanical design

PZT

Page 4: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Michelson : realised in the lab

Stationarymirror

Beam-splitter

PZT sweptmirror

Camera

Launchcollimator

Page 5: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Michelson :Camera view of mirror sweeping

Page 6: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Replaced camera with MT connector used 4 nearest neighbour fibres to read out

0 5000 10000 15000

0.0

0.2

0.4

0.6

0.8

1.0

No

rma

lise

d in

ten

sity

/ a

.u.

Time / DAQ cycles

ch 1 ch 2 ch 3 ch 4

Page 7: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Use modified Carré algorithm to extract4 channel average wrapped phase

0 5000 10000 15000

-3

-2

-1

0

1

2

Ph

ase

/ ra

d

Time / DAQ cycles

UnwrappedWrapped

Page 8: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

9000 10000 11000

-1.0

-0.5

0.0

0.5

1.0

Ext

ract

ph

ase

/

rad

Time / DAQ cycles

Extract independentlyfrom each channelusing 4 points separated equally in time

Here 320 cycles apart

Use modified Carré algorithm to extract

wrapped phase for each channel fit a line

Fit a line to eachstraight sectionaround cycle 10 000and extract residuals

1 ~ 40 mradequivalent 10 nm

Page 9: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

STATUS: New Design

• More traditional Michelson setup leads to nice results.

• Integration of many interferometer into one node more difficult –

• A compact version is ready and shows promise.

Page 10: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Compact Interferometer head

• Shown here using 2cm optics• 1cm optics likely to work. According to

Zemax simulation diffraction should not be a problem. (tests underway)

5cm

4cm

Collimator

Beam splitter

Readout fibres

Input fibre

Retro Reflector

Page 11: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Status of Subsystems

• Electronics ready for mass production (in use by LiCAS, DC mode integrated for us)

• Temperature measurement system ready for mass production (24 channels built and tested)

• Readout software:– ADC Readout needs adaptation from LiCAS– Binary storage format ready

• FSI data analysis code:– Simple version working and used– In collaboration with LiCAS group implementing advanced object

oriented analysis framework.• Evaluation of Laser to buy for ATF setup finished by end

of January.– New laser available by end of February

Page 12: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Mass Production of Interferometer

• Full test of present system in air.• Test vacuum system for laboratory:

– Design ready to build vacuum test system– Available in February– Test present setup in vacuum

• Vacuum fibre feedthrough:– Commercial feedthrough too expensive:

• Build own feedtroughs• Jig in production now• First workable feedthroughs by February to be used in test vacuum

system

• Build Jig to place/glue components (beamsplitter and collimator) precisely onto base.– Build first model by March

Page 13: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

• Setup at ATF• Need Scaffolding to hold vacuum tubes• Triangle Nodes Concept

– Drawings ready for base plate – Construction by March

Vacuum system at ATF

Page 14: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

• Triangle Nodes Concept– Drawings ready for base plate – Construction of base plateby March– Construction of instrument platform and dome by May

Vacuum system at ATF

Page 15: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

KEK BPM nodes

• Concept allowing for considerable angle play. • Fixed (or single bellow) attachment to KEK aluminum bar. • Installation early summer 2007

Page 16: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Move to ATF2

• If 2 nano-BPM setups at ATF2 beam line available:– Within reasonable distance between each other.– Moving experiment to ATF2 beam line can be considered.

• Requirements:– New scaffolding and floor plate– New “flowerpots”

Page 17: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

SLAC/LLBL BPM Node

Here attach vacuum tube for interferometerAttached to BPM.

Holds retro reflector.

Firmconnection

Strain Gauge• Needs bellow to allow

motion of BPM– Vacuum causes a force

order of 100N!

• Develop small force vacuum mount using double bellow system.

• Allows small motion (~1 mm) of BPM-system (we still can measure)

• Large motion (5-10mm) are possible but we cannot measure anymore

• Test stand to measure remaining (perpendicular) force on BPM frame.

-1mm-3mm 1mm 3mm

1N

2N

-1N

0N

-2N

-3N

-3N

Force exerted on carbon frame (BPM)±1mm: < 0.5N/mm±3mm: < 0.8N/mm

Force exerted by perpendicular motion

Page 18: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

SLAC/LLBL BPM Node• Needs bellow to allow

motion of BPM– Vacuum causes a force

order of 100N!

• Develop small force vacuum mount using double bellow system.

• Allows small motion (~1 mm) of BPM-system (we still can measure)

• Large motion (5-10mm) are possible but we cannot measure anymore

• Test stand to measure remaining (perpendicular) force on BPM frame.

• Next item to design is retro holder object: a small tube with vacuum flanges for both bellows at the end.

• Plan to mount in March

• “Flower pot” design needed by March; built in May– Flower pot attached to

scaffolding not carbon fibre tube!

RetroReflector

Retro Holder

Page 19: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

SLAC/LLBL BPM Node• Needs bellow to allow

motion of BPM– Vacuum causes a force

order of 100N!

• Develop small force vacuum mount using double bellow system.

• Allows small motion (~1 mm) of BPM-system (we still can measure)

• Large motion (5-10mm) are possible but we cannot measure anymore

• Test stand to measure remaining (perpendicular) force on BPM frame.

• Next item to design is retro holder object: a small tube with vacuum flanges for both bellows at the end.

• Plan to mount in March

• Allow for true non-touching setup– More difficult analysis

RetroReflector

Retro Holder

NanoGrid

Page 20: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Combining all Measurement

• Three systems have to be operated simultaniously:– 3 SLAC-BPMs define beam direction– 1 KEK Q-BPM measures motion with respect to that direction.

This BPM is still present on the original motion stage. It can be correlated to the aluminium bar via a Michelson interferometer.

– MONALISA measures relative motion of two BPM systems.

• Isues to be solved:– Read KEK BPM with SLAC readout system– Align two BPM system that both get optimal measurements

We would like to ask if this can be demonstrate before we install MONALISA.

Page 21: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

ATF2: Measuring Motion of Shintake Monitor with Respect to

Final Doublet • Idea of Compact Straightness Monitor (CSM)

presented in May:

Pointsource

Retro

Mirror

Collimator

Fibre launchand readout

Long arm

Use reflection from fibreend as short arm

Distancemeter

Page 22: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Binocular Michelson

PZTdrivenmirror

Fibre launchcollimator

Pelliclebeam-splitter

Pelliclebeam-splitter

Photodetector

Photodetector

Target retroreflector

Setup takes shape on our optical table.

Page 23: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Attaching CSM: Shintake Monitor

Monitor and scanner location

IP(on-axis)

Beam sampler

off-axismonitor(ch1)

Phase scanner

off-axismonitor(ch2)

• What do we want to monitor:• Monitor motion (angular

vibrations) of “intersection mirrors”– Its already a mirror– Has to be done in air (Requires

close distance monitor)– Needs to correlate the motion

measurements of the two mirrors.

• Monitor off-axis camera– Easier setup– Mor indirect measurement

Page 24: MONALISA David Urner Paul Coe Matthew Warden Armin Reichold Oxford University

Attaching CSM: Focusing Magnet

• Unsolved Problem on how to monitor magnetic centre of focusing magnet.– Attach CSM to one point of

magnet– Use several distance metres

to monitor breathing of magnet

– Correlate with temperature measurements Retro Reflectors

CSM