A Mole for warm magnetic and optical measurements

  • Slides: 35
Download presentation
A Mole for warm magnetic and optical measurements of LHC dipoles 1 L Bottura

A Mole for warm magnetic and optical measurements of LHC dipoles 1 L Bottura 1, M Buzio 1, G Deferne 1, H Jansen 2, C Glöckner 2, A Köster 2, P Legrand 1, A Rijllart 1, P Sievers 1 , F Villar 1 1 CERN, European Organization for Nuclear Research - 1211 Geneva 23, Switzerland 2 Frauenhofer Institut IPT, Aachen, Germany Eleventh International Magnet Measurement Workshop September 21 - 24, 1999 Brookhaven National Laboratory, Upton, New York, USA Thursday, 23 Sept. 1999 Berkner B 10: 50 -11: 20 1 Also published in the proceedings of the 16 th International Conference on Magnet Technology, Ponte Vedra Beach, IL, 26 Sept- 2 Oct 1999 A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

A Mole for Warm Magnetic and Optical Measurements of LHC Dipoles ¨ ¨ ¨

A Mole for Warm Magnetic and Optical Measurements of LHC Dipoles ¨ ¨ ¨ Introduction Mechanical layout VR Demo 1 Magnetic performance Optical performance Conclusions 1 http: //home. cern. ch/m/mtauser/www/applications/mole/virtualmole. wrl A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Introduction ¨ Why use a mole ? ¾ Purpose: measure magnetic axis ¾ Cold

Introduction ¨ Why use a mole ? ¾ Purpose: measure magnetic axis ¾ Cold measurements done for max. efficiency with 15 m long coil shaft, obstructing line-of-sight to the coil center Þ travelling probe is needed ¾ Additional duties: warm field quality of all dipoles, cold field of samples ¨ Requirements for series measurements ¾ ¾ Coil center position: precision better than 0. 1 mm Warm measurements: 50 mm, B 25 m. T Rugged, quick and simple to setup and operate As many off-the-shelf components as possible A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Mole test bench overview magnet front reference bench (telescope) rear reference bench (transport motor,

Mole test bench overview magnet front reference bench (telescope) rear reference bench (transport motor, cable connections) A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Front reference bench Telescope CCD camera mole support shell (closed) focusing system Sliding support

Front reference bench Telescope CCD camera mole support shell (closed) focusing system Sliding support A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Rear reference bench Axis transfer jig Mole Cable receptacle Transport motor A mole for

Rear reference bench Axis transfer jig Mole Cable receptacle Transport motor A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Front reference bench optical alignment targets ( 4) Laser for alignment measurement axis transfer

Front reference bench optical alignment targets ( 4) Laser for alignment measurement axis transfer carbon fiber jig Telescope/CCD/DSP unit granite table transport belt A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Status ¨ Warm Mole ¾ First unit accepted and under commissioning ¾ Two more

Status ¨ Warm Mole ¾ First unit accepted and under commissioning ¾ Two more units to come, will perform warm test of all LHC dipoles ¾ Can be readily adapted to warm quadrupole tests ¨ Cold Mole ¾ Order started, last design details now being finalized ¾ Will perform cold tests for a sample populations of LHC dipoles to get warm-cold axis correlation ¾ Further units may be slightly modified for cold quadrupole tests A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Mechanical layout ¨ Main features ¾ ¾ ¾ three 750 mm long radial coils

Mechanical layout ¨ Main features ¾ ¾ ¾ three 750 mm long radial coils coil drive: Shinsei travelling-wave ultrasonic piezo motor 4096 CPR Heidenhein angular encoder On-board feedback auto-leveling system Spring-loaded roller system Motorized traction belt drive Two granite benches to establish reference positions LED+lens system to create virtual light-spot in the coil centre Telescope + CCD camera + DSP to measure light-spot position All functions remotely controlled via RS 232 Auxiliary optical system to transfer axis to magnet fiducials A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Main components Piezo motor 3: 1 reduction gearbox Wyler encoder Coil Potentiometer Elastic coupling

Main components Piezo motor 3: 1 reduction gearbox Wyler encoder Coil Potentiometer Elastic coupling (with helical groove for the cable) Ball-bearing support flange A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Longitudinal transport · closed-loop pre-tensioned Inconel transport belt · feedback-controlled DC motor drive ·

Longitudinal transport · closed-loop pre-tensioned Inconel transport belt · feedback-controlled DC motor drive · referencing given by optical barriers at both ends of the magnet (selfcalibration at the end of each trip) · max. velocity about 1 m/s · precision of positioning better than 0. 5 mm · mole must be switched manually between apertures A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Longitudinal reference position spring-loaded roller LED viewing aperture Optical barrier (receptor) lower half-shell support

Longitudinal reference position spring-loaded roller LED viewing aperture Optical barrier (receptor) lower half-shell support front transport belt attachment A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Safety · interlock system: mole will stop if covers are removed, transport cable gets

Safety · interlock system: mole will stop if covers are removed, transport cable gets tangled, transport motor drains overcurrent · reduced velocity close to the edges · longitudinal position cross-checked with two independent measurements (angular encoder + linear potentiometer) A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Autoleveling ¨ Why autoleveling ? ¾ ¾ ¨ imperfections of beam pipe/rollers rotation of

Autoleveling ¨ Why autoleveling ? ¾ ¾ ¨ imperfections of beam pipe/rollers rotation of container during travel observed rotation up to 2~3°/m transport belt & cable may be twisted coil must be level prior to measurement How does it work ? ¾ ¾ ¾ DC motor engaged in container to rotate coil+encoder+piezo motor feedback system using wide-range level meter precision achieved better than 4 mrad time needed less than 5 s autoleveling done at the end of each longitudinal movement A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Auto-leveling mechanism Inner gear (linked with container) Wide-range level meter Motor shaft gear Roller

Auto-leveling mechanism Inner gear (linked with container) Wide-range level meter Motor shaft gear Roller (fixed tangentially by friction) A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Auto-leveling mechanism travel Start autolevel End of travelling Final configuration A mole for warm

Auto-leveling mechanism travel Start autolevel End of travelling Final configuration A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Optical measurement 1. Telescope ¾ accurately leveled and aligned wrt magnet ¾ mounted on

Optical measurement 1. Telescope ¾ accurately leveled and aligned wrt magnet ¾ mounted on rails to serve both apertures 2. CCD camera ¾ 752 582 pixel, 6. 00 4. 96 mm size ¾ self-aligned to telescope via reference marks 3. DSP image processor ¾ threshold filtering + center of gravity calculation ¾ measurements internally averaged over multiple takes ¾ software calibration map A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Virtual lightspot the virtual image remains in the coil center even when the mole

Virtual lightspot the virtual image remains in the coil center even when the mole rotates LED Magnifying lens Virtual lightspot A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Optical measurement ¨ Performance ¾ 4 mm 14 mm 20 m range ¾ total

Optical measurement ¨ Performance ¾ 4 mm 14 mm 20 m range ¾ total error 60 m ¾ measurement time 4 s at closest range A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Optical system calibration A mole for warm magnetic and optical measurements of LHC dipoles

Optical system calibration A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Optical system calibration A mole for warm magnetic and optical measurements of LHC dipoles

Optical system calibration A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Example: optical measurement A mole for warm magnetic and optical measurements of LHC dipoles

Example: optical measurement A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Focusing system ¨ How does it work ¾ ¾ no autofocus needed longitudinal position

Focusing system ¨ How does it work ¾ ¾ no autofocus needed longitudinal position sent to the camera at the end of each movement focusing motor follows a software calibration table total error if out-of-focus 1 m/mm A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Magnetic performance ¨ Harmonic Coils ¾ 41 750 mm fiberglass/epoxy coil support ¾ 3

Magnetic performance ¨ Harmonic Coils ¾ 41 750 mm fiberglass/epoxy coil support ¾ 3 radial coils with 400 turns, 3. 4 m 2 area ¾ 1 coil for main dipole, 1 for dipole compensation + 1 spare ¨ System precision ¾ ¾ Main dipole: better than 10 -4 Dipole angle: better than 0. 2 mrad Multipoles: generally better than 2· 10 -6 relative to B 1 bucking factor 2000 A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Example: multipoles A mole for warm magnetic and optical measurements of LHC dipoles IMMW

Example: multipoles A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Example: calibrated dipole angle A mole for warm magnetic and optical measurements of LHC

Example: calibrated dipole angle A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Axis Transfer ¨ Why transfer the magnetic axis ? ¾ harmonics, and hence magnetic

Axis Transfer ¨ Why transfer the magnetic axis ? ¾ harmonics, and hence magnetic axis, are measured in the coil reference frame ¾ the center of the coil is measured in the telescope reference frame ¾ the magnetic axis is needed in the reference frame of the magnet fiducials ¨ How the transfer will be done ¾ the granite tables establish two reference positions per aperture, vertically and laterally reproducible within 20 m ¾ reference positions are measured by the telescope ¾ relative position of magnet fiducials and granite tables is measured by means of an auxiliary laser system ¾ relative position of coil center wrt magnet fiducials can thus be computed A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Axis Transfer Granite jig reference line Granite table reference line Mole coil position along

Axis Transfer Granite jig reference line Granite table reference line Mole coil position along magnet Magnet fiducial line Auxiliary alignment laser beam Granite table jig Telescope frame A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Axis Transfer Z Magnetic center (z) Magnet fiducial line Mole coil position Marble table

Axis Transfer Z Magnetic center (z) Magnet fiducial line Mole coil position Marble table jigs line Marble table reference line Y Telescope reference frame A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Problems encountered ¨ ¨ Unsteady velocity of piezo-motor, getting worse with motor heating Micro

Problems encountered ¨ ¨ Unsteady velocity of piezo-motor, getting worse with motor heating Micro cables and connectors delicate and difficult to handle Fine alignment of the lens Image distortion due to thermal gradients in the magnet A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Piezo motor rotation speed ¨ Rotation speed quality ¾ encoder detects low-frequency rotation speed

Piezo motor rotation speed ¨ Rotation speed quality ¾ encoder detects low-frequency rotation speed oscillations up to 8% ¾ oscillation amplitude gets larger as motor heats up ¾ oscillations interfere with measured harmonics (errors in b 2 up to 0. 5 units observed) ¨ Improvements under way ¾ optimization of stiffness and damping of the coil/motor link to minimize response ¾ fine tuning of motor speed map (t) to minimize excitation ¾ enhanced motor cooling ¾ automatic off-line filtering of spurious harmonics A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Piezo motor rotation quality Forward run Backward run average A mole for warm magnetic

Piezo motor rotation quality Forward run Backward run average A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Piezo motor rotation quality A mole for warm magnetic and optical measurements of LHC

Piezo motor rotation quality A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Piezo motor rotation quality A mole for warm magnetic and optical measurements of LHC

Piezo motor rotation quality A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch

Conclusions 1. 2. 3. 4. 5. Magnetic and optical performance generally exceeding specifications Well

Conclusions 1. 2. 3. 4. 5. Magnetic and optical performance generally exceeding specifications Well suited for industrial-type test environment Test bed for further technological improvements (piezo-motor, remote encoders, etc. ) Software integration under way Minor improvements under way: smoother velocity control, better optics alignment A mole for warm magnetic and optical measurements of LHC dipoles IMMW XI, Brookhaven National Laboratory, 21 -24 Sept. 1999 marco. buzio@cern. ch