Last stage SA F7 monitor/control

Slides:



Advertisements
Similar presentations
Vibration Isolation Group R. Takahashi (ICRR)Chief T. Uchiyama (ICRR)Payload design H. Ishizaki (NAOJ)Prototype test R. DeSalvo (Caltech)SAS design A.
Advertisements

Status of the Virgo Commissioning G.Losurdo – INFN Firenze/Urbino for the Virgo Collaboration.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.
Payload design methods versus modeling E. Majorana.
1 Virgo commissioning status M.Barsuglia LAL Orsay.
LCGT seismic Attenuation System DRADF DRAFT DRAFT DRAFT.
Virgo commissioning update - VSR1 first month summary E. Tournefier WG1 meeting, Cascina June 20 th,2007.
F. Frasconi I.N.F.N. Pisa for the Virgo Collaboration TAUP2007 Sendai, September 11-15, 2007 VIRGO EXPERIMENT VIRGO: a large interferometer for Gravitational.
Suspended Mirror control: Learning through Virgo Experience E. Majorana - I.N.F.N. Pisa Aspen GWAD February 16, 2004.
Thursday, 18 March 2004 Andrea Viceré, Urbino University 1/34 Issues in the Virgo mechanical simulation Why a mechanical simulation How the simulation.
Use ofSiesta in VIRGO commissioning Lisa Barsotti University of Pisa – INFN Pisa For the Virgo collaboration Caltech, December 19th 2003.
SIESTA for Virgo locking experience L. Barsotti University of Pisa – INFN Pisa on behalf of the Virgo Locking Group Cascina, March 16th 2004 Simulation.
Present Superatttenuator performance vs. AdV & ET Requirements S.Braccini for Virgo Suspension group.
Thoughts on short term improvements for Mirror Suspension Control G.Losurdo - P.Ruggi.
Prototype Test of Vibration Isolation System Current Status & Schedule
Takanori Sekiguchi Anual Meeting of Physics Society of Japan Sep. 22nd, 2013) Prototype Test of Vibration Isolation System Current Status & Schedule 1.
Takanori Sekiguchi ALPS Report, Dec. 26th, 2013 Prototype Test of Type-B 1 Takanori Sekiguchi KAGRA F2F MEETING Feb
1 1.ISC scope and activities 2.Initial Virgo status 3.Design requirements 4.Reference solution and design status 5.Plans toward completion 6.Technical.
ILIAS – WG1 Hierarchical suspension control G.Losurdo INFN Firenze.
Experimental tests of SA simulation Irene Fiori – Simulation Workshop – March 18, 2004 Virgo dataSiesta simulation 1. Inertial Damping simulation  test.
Seismic Attenuation System (SAS) for LCGT Inverted pendulum: 30mHz 3 cascaded GAS filter: 500mHz Test mass suspension: triple pendulum Transfer functions.
Ryutaro Takahashi (National Astronomical Observatory of Japan) Vibrtion isolation system for KAGRA The 6th Korea-Japan workshop on KAGRA NAOJ, June,
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
SUSPENSIONS Pisa S.Braccini C.Bradaschia R.Cavalieri G.Cella V.Dattilo A.Di Virgilio F.Fidecaro F.Frasconi A.Gennai G.Gennaro A.Giazotto L.Holloway F.Paoletti.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
SUSPENSION Performance vs. Specs PASSIVE ATTENUATION IN BAND: OK for AdV MIRROR HOR. SWING DAMPING “IN VELOCITY”: Ok for Locking in Adv MIRROR HOR. SWING.
Behavior of an inverted pendulum in the Kamioka mine R. Takahashi (NAOJ), A. Takamori (ERI), E. Majorana (INFN) GWADW 2010 We are investigating behavior.
1 The Virgo noise budget Romain Gouaty For the Virgo collaboration GWADW 2006, Isola d’Elba.
STREGA-C3 Cryogenic Seismic Isolation Roberto Passaquieti Dipartimento di Fisica “E. Fermi” Università di Pisa INFN sezione di Pisa ILIAS-GW Annual General.
MSC - 18 Oct 071 LOW FREQUENCY SEISMIC NOISE: LOCKING AND SENSITIVITY ISSUE Paolo Ruggi noise meeting.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
LIGO-G Z The Status of VIRGO E. Tournefier for the Virgo Collaboration GWADW 2004, Aspen From the CITF to VIRGO Commissioning of the Fabry-Perot.
1 PAY Review Meeting 1 18/3/2009 Piero Rapagnani 18/03/2009.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
GWADW - La Biodola 20061/20 Underground reduction of Gravity Gradient Noise. Giancarlo Cella INFN sez. Pisa/Virgo GWADW – La Biodola 2006.
MSC winter, short-term schedule Commissioning meeting Cascina 2 Oct 2006.
The control of the Virgo Superattenuator: present and future Giovanni Losurdo - INFN Firenze/Urbino on behalf of the Virgo Collaboration.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
Two Layers SAS: Damping of Torsion Mode Feb. 5th, 2011 F2F Meeting Takanori Sekiguchi, Riccardo DeSalvo, Ryutaro Takahashi 1/8.
MSC recent activities COMM Cascina 5 Feb EM-MSC Commissioning-oriented running activity Operation and interface updates Hardware checkup.
LIGO-G R Inverted pendulum studies for seismic attenuation Ilaria Taurasi University of Sannio at Benevento, Italy September 20, 2005 Supervisor.
LIGO-G R 1 HAM Passive Seismic Attenuation System (SAS) System Performance, Fabrication, Assembly, Installation Riccardo DeSalvo, Valerio Boschi,
SAT Plans for System R&D Signal Recycling Construction and A&I Short Suspension Upgrade Roberto Passaquieti Università di Pisa and INFN-Pisa AdV Review.
Advanced Advanced Virgo BASELINE DESIGN advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration.
Advanced Coll. Meeting – Cascina, Sept 11th, 2007 G.Losurdo – INFN Firenze/Urbino 1 SUPERATTENUATOR - IP BASELINE: VIRGO DESIGN with STIFFER IP LEGS TILTMETER.
LSC Meeting Baton Rouge, LA, V.Boschi for the HAM-SAS team Ben Abbott, Valerio Boschi, Dennis Coyne, Michael Forte, Jay Heefner, Yu-mei Huang,
CERN –GSI/CEA MM preparation meeting, Magnetic Measurements WP.
New Coil Drivers Time Line Alberto Gennai I.N.F.N. Pisa.
Displacement, Location or Position Sensor Muhajir Ab. Rahim School of Mechatronic Engineering, KUKUM.
Filter #7 control April 18, 2016 –, Cascina Paolo Ruggi.
1 Advanced Virgo Monolithic Payloads P.Rapagnani Thermal Noise Workshop 2012_02_24-25.
Advanced SA Specifications & Scientific Motivations S.Braccini, Cascina 21 Settembre 2007.
Paola Puppo INFN – Rome Thermal Noise Meeting – “Sapienza”-Rome - February 26 th 2008.
VIRGO Superattenuator performance and its evolution in the SAFE Project F. Frasconi – INFN Pisa (ET-WP2 Workshop – Roma – February 27, 2009)
Type-A SAS Local Control Simulation (Current Status)
First clues on ET payload sensing and control
CLIC magnets precise positioning
Calorimeter Mu2e Development electronics Front-end Review
VIRGO–KAGRA Meeting about bottom filter damping
LCGT Seismic Attenuation System LCGT-SAS
Present Superattenuator performance vs. ET Requirements S
Advanced VIRGO Experiment
Control of the KAGRA Cryogenic Vibration Isolation System
External forces from heat links in cryogenic suspensions
Superattenuator for LF and HF interferometers
Magnetic Coupling to Test Mass Suspensions
Background With new accelerators delivering beams always smaller and more energetic, requirements for very precise beam alignment become more and more.
The Superattenuator upgrades and the SAFE Project
HAM-SAS Mechanics Status of modeling V.Boschi, V. Sannibale.
Presentation transcript:

Last stage SA F7 monitor/control Passaquieti Roberto University of Pisa & INFN-Pisa KAGRA-VIRGO Joint Meeting 18th Apr. 2016

SA Filter-7 monitor/control: origin/specs The Filter-7 (F7) monitor/control was first introduced in Virgo in 2003 after the Superattenuators (SA) installation/integration (initially not foreseen) Initial Virgo commissioning experienced serious problems with the SA setup monitor and control Tight constraints with frequent mechanical contacts Hard damping of the LF SA modes ( 16-30 mHz) excited by the Locking action forces The Virgo monitor/control architecture Specs: Operation in HV Precision (~ 0.1 mm, ~ 0.1 mrad), long term efficiency and reliability Longitudinal X, Z and yaw (ThY) d.o.f. monitor/control 3 horiz. LVDTs (Sens. ~ 130 mV / mm, noise spectr. 10 -8 m / Hz) sharing the secondary winding with a collocoted constant gradient Maxwell magnet-coil actuators Vertical Z d.of. On board LVDT measuring the vertical displ.of the floating filter “crossbar” (sum of all 6 SA filter LVDT s) (Sens. ~ 570 mV / mm, noise spectr.10 -7 m /  Hz) Angulat pitch (ThX) and roll (ThZ) High precision and HV campatible bi-axial ball tiltmeter (Res.= 0.1 microrad)

Virgo F7: mecanical constraints z x y Virgo F7 working point constraints: longitudinal X, Z d.o.f.: < ± 4 mm vertical Y : < ± 7 mm angular x< 3mrad, z < 8 mrad,y <10 mrad

Virgo F7: damping scheme  dashpot (F7ground) M  = -  d /d t 1 2 5 6 27 35 Virgo Marionette-Mirror TF Marionette-Mirror TF without damp. Marionette-Mirror Transfer Function with damping (F7-ground) =0.5 16 mHz 32 mHz

Virgo F7: actuator/sensor device Primary coil Magnet Secondary coils voltage/displacement: 0.20 mV/mm force/current:  = 73 mN/A Wide ±20 mm linear range dynamics to limit seism. noise

Virgo F7: monitor/control installation

AdV F7 monitor/control upgrade In AdV w.r.t. Virgo most of the F7 mechanical constraints have disappeared: the old IVC was removed from the test-masses towers Still the increased complexity of the F7-payload system required the upgrade of the F7 monitor/control. the actuation on the F7 body was extended to all 6 d.o.f. (Virgo x,z,thy) Following our experience we merged the requiered 6 sensors (3 hor.+3 vert.) and 6 actuators into 6 Virgo-like collocated Maxwell pairs of magnet-coils systems maximum force: 50mN; max noise ~ 1 nN/sqrt(Hz) @ 10Hz; low force gradient: < 1%/mm (to not reintroduce seismic noise);

AdV: New F7 monitor/control prototyping Space constraints induced a little re-scaling of the coil dimensions but still keeping a consistent dinamical range: axial clearance: 12 mm; radial clearance: a few cm; operating volume: 10x10x10 mm3; maximum force: 50mN; max noise ~ 1 nN/sqrt(Hz) @ 10Hz; low force gradient: < 1%/mm (to not reintroduce seismic noise). During the prototyping phase we tested new LVDT devices with a moving ferrite core in place of the moving primary coil: experienced a better sensing but with a much reduced linearity range. For the final set-up we came back to the Virgo F7 LVDT scheme: secondary Maxwell coils pairs fixed to groungd, with a the primary coil fixed on the F7 body, free to move inside the operating volume of the secondary windings. F7 monitor/control prototypes with ferrites

From prototype to final AdV design

Rendering of the AdV F7-payload system New IVC vessel F7 mon./contr. system