Cavity Work at LASTI LSC-VIRGO Meeting, Hannover - 24 th October 2007 Lisa Barsotti and Matthew Evans for the LASTI group G070694-00-D.

Slides:



Advertisements
Similar presentations
Hierarchical Control Notes – Blending Style Follows quad example Note: coil drivers and ESD are LASTI style; seismic noise is outdated 1G v3.
Advertisements

Global longitudinal quad damping vs. local damping G v8 1.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
LIGO - G R 1 HAM SAS Test Plan at LASTI David Ottaway November 2005 LIGO-G Z.
Global longitudinal quad damping vs. local damping Brett Shapiro Stanford University 1/32G v13 LIGO.
One Arm Cavity M0 L1 L2 TM M0 L1 L2 TRIPLE QUAD 16m R = 20m, T=1% R = ∞, T=1%  Optimally coupled cavity (no mode matched light reflected back)  Finesse.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
Optical Waveguide and Resonator
An Introduction to Electrostatic Actuator
Current-Mode Multi-Channel Integrating ADC Electrical Engineering and Computer Science Advisor: Dr. Benjamin J. Blalock Neena Nambiar 16 st April 2009.
Matthew Evans, Ph237 April Application of Simulation to LIGO Interferometers  Who am I? »Matthew Evans, Ph.D. from Caltech on Lock Acquisition 
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
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.
Stefan Hild, Andreas Freise, Simon Chelkowski University of Birmingham Roland Schilling, Jerome Degallaix AEI Hannover Maddalena Mantovani EGO, Cascina.
Present Superatttenuator performance vs. AdV & ET Requirements S.Braccini for Virgo Suspension group.
Refractive index dispersion and Drude model Optics, Eugene Hecht, Chpt. 3.
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
Stefan Hild 1Ilias WG1 meeting, Sep 2005, Perugia Title GEO 600 Commissioning progress Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Interferometer Control Matt Evans …talk mostly taken from…
1 © Unitec New Zealand DE4401 AC PHASORS BASICS. AC Resistors 2 © Unitec New Zealand.
Stefan Hild October 2007 LSC-Virgo meeting Hannover Interferometers with detuned arm cavaties.
Conceptual Design for Advanced LIGO Suspensions Norna A Robertson University of Glasgow and Stanford University for the GEO suspension team +contribution.
Lecture 5 Method of images Energy stored in an electric field Principle of virtual work 1.
GEO‘s experience with Signal Recycling Harald Lück Perugia,
Experimental tests of SA simulation Irene Fiori – Simulation Workshop – March 18, 2004 Virgo dataSiesta simulation 1. Inertial Damping simulation  test.
European Gravitational Observatory12/12/2005 WG1 Hannover 1 Mode Matching of the Fabry-Perrot cavities Julien Marque.
Electrostatic actuators: from the GEO experience to the 2 nd generation requirements Harald Lück Perugia,
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
System Identification for LIGO Seismic Isolation Brett Shapiro GWADW – 19 May G v1.
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: Next steps December 12 st 2005 Hannover, ILIAS-GWA WG1 Matteo Barsuglia, LAL/CNRS.
Matt Evans, LSC March 2003 (G E)1 Lock Acquisition in LIGO  Who am I? »Matt Evans »Caltech graduate  What is Lock Acquisition? »The process.
Vistas in Axion Physics April 2012 ADMX Cavities at higher and lower frequencies C. Hagmann, J. Hoskins, I. Stern, A.A. Chisholm, P. Sikivie, N.S. Sullivan,
Analysis and Design of Multi-Wave Dilectrometer (MWD) for Characterization of Planetary Subsurface Using Finite Element Method Manohar D. Deshpande and.
Arm Length Stabilisation for Advanced Gravitational Wave Detectors Adam Mullavey, Bram Slagmolen, Daniel Shaddock, David McClelland Peter Fritschel, Matt.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
LSC-VIRGO joint meeting - Pisa1 Input mirrors thermal lensing effect Frequency modulation PRCL length in Virgo Some results from a Finesse simulation.
Harald Lückfor the GEO600 Comissioning team 1ILIAS Meeting, Palma, Oct Title GEO 600 Commissioning Status Based on a talk of Stefan Hild for the.
LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.
1 The Virgo noise budget Romain Gouaty For the Virgo collaboration GWADW 2006, Isola d’Elba.
Abstract The Hannover Thermal Noise Experiment V. Leonhardt, L. Ribichini, H. Lück and K. Danzmann Max-Planck- Institut für Gravitationsphysik We measure.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
M. Mantovani, ILIAS Meeting 7 April 2005 Hannover Linear Alignment System for the VIRGO Interferometer M. Mantovani, A. Freise, J. Marque, G. Vajente.
Adaptive Control Loops for Advanced LIGO
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
Chapter 11 Vibrations and Waves.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
Aligning Advanced Detectors L. Barsotti, M. Evans, P. Fritschel LIGO/MIT Understanding Detector Performance and Ground-Based Detector Designs LIGO-G
Mechanical Mode Damping for Parametric Instability Control
1 Locking in Virgo Matteo Barsuglia ILIAS, Cascina, July 7 th 2004.
Optical Spring Experiments With The Glasgow 10m Prototype Interferometer Matt Edgar.
LIGO-G Z March 2007, LSC meeting, Osamu Miyakawa 1 Osamu Miyakawa Hiroaki Yamamoto March 21, 2006 LSC meeting Modeling of AdLIGO arm lock acquisition.
1 DC readout for Virgo+? E. Tournefier WG1 meeting, Hannover January 23 rd,2007 DC vs AC readout: technical noises Output mode cleaner for DC readout.
1 Frequency Noise in Virgo by Matt Evans. 2 The Actors  Noise Sources  Input Mode Cleaner length noise  Sensing noise on IMC lock  Frequency Servo.
Sensitivity of Virgo E. Tournefier (LAPP-CNRS) LSC-Virgo week May 23 rd,2007 LIGO-G Z.
Yoichi Aso Columbia University, New York, NY, USA University of Tokyo, Tokyo, Japan July 14th th Edoardo Amaldi Conference on Gravitational Waves.
Calibration and the status of the photon calibrators Evan Goetz University of Michigan with Peter Kalmus (Columbia U.) & Rick Savage (LHO) 17 October 2006.
LV Meeting – 22 September 2009 Brett Shapiro G v1
ESD Force Noise and Range for Various Modes of Operation
Progress on Acoustic Mode Damper design
Violin mode amplitude glitch monitor for the presence of excess noise: from GEO 600 to aLIGO Borja Sorazu, Alan Cumming, Giles Hammond, Siong Heng, Rahul.
Update on aLIGO Charging Issues
Commissioning progress Stefan Hild Ilias WG1 meeting, Sep 2005
Lock Acquisition Real and Simulated
HAM SAS Test Plan at LASTI
Lessons Learned from Commissioning of Advanced Detectors
Talk prepared by Stefan Hild AEI Hannover for the GEO-team
Measurement of radiation pressure induced dynamics
Understanding Network Analysis
Presentation transcript:

Cavity Work at LASTI LSC-VIRGO Meeting, Hannover - 24 th October 2007 Lisa Barsotti and Matthew Evans for the LASTI group G D

2 One Arm Cavity M0 L1 L2 TM QUAD (control prototype) 16m R = 20m, T=1% R = ∞, T=1% TRIPLE Optimally coupled cavity (no mode matched light reflected back) Finesse ~ 625 M0 L1 L2

3 Goals Test of the QUAD : Electrostatic Drive (ESD) Hierarchical Control Lock Acquisition ✯ ✯ TF and resonance frequencies: T , by Brett and Richard

4 QUAD performance  Real Seismic Noise (MODEL)

5 QUAD performance Real Data (as measured by the optical lever) (MODEL)  Real Seismic Noise

6 ESD: Principle Goal: get rid of coil-magnet actuators (reduce noise coupling due to magnets) 4 pairs of electrodes, coated onto the reaction mass Each pair of electrodes forms a capacitor, whose fringe field attracts the mirror surface (dielectric) placed in front of it F =  (  r, d,a)( ΔV)² distance between test mass and reaction mass Constant geometry factor depending on the electrode pattern design The attractive force F is proportional to the square of the difference in the applied voltage ΔV to the electrodes:  Coupling coefficient [N/V²]

7 Design for Advanced LIGO  = 7e-10 N/ V² * Based on the GEO measurement (4.9e-10 N/V²); for Advanced LIGO estimate of 35% more force produced for a given voltage Electrostatic drive (ESD) results from GEO and application in Advanced LIGO T K, K. Strain (Feb 2006) F MAX = 7e-10 * (800)² = 450  Optimized electrode pattern for AdvLIGO Coupling coefficient expected* to be: Maximum force available for lock acquisition (with a difference of 800 V between the two channels):

8 ESD at LASTI (QUAD Controls Prototype) Coupling coefficient expected to be as in GEO:  = 4.9e-10 N/V² (not optimized electrode pattern yet) Maximum difference voltage currently available at LASTI: 600 V Maximum force expected: F MAX = 4.9 e-10 * (600)² ~ 180  Bias, Control Q2 Q3 Q4 Q1

9 LASTI Measurement - I With a 7Hz line we expect the  component (2π*7Hz) to be twice as big as the 2  (2 π* 14 Hz)…. …but  component not measured at all.. 2  component  component F =  (V bias - V con )² F =  V² +  V² sin²(ωt) - 2  V²sin(ωt) V bias = V V con = Vsin(ωt) Bias, Control Q2 Q3 Q4 Q1 Cavity locked by acting on the triple (OSEM) ESD Drive:

10 LASTI Measurement - II   SINE on controls + OFFSET on BIAS SINE + OFFSET on a single electrode By driving a single electrode with an OFFSET plus a SINE, we get the fundamental (similar results for all of the 8 electrodes): By driving the 8 electrodes with an OFFSET plus a SINE: No significant difference measured in the amplitude of the  component by inverting the sign of the drive on the BIAS relative to CONTROL!

11 LASTI Numbers F MAX = 2.15e-9 * (300)² ~ 180  The same as if the ESD behaved correctly, about 2.5 times less than the Advanced LIGO design  V² = 52  N   2.15e-9 N/ V² Cavity error signal calibration: 2e6 counts/ mm  610 V/mm Coupling coefficient a measured by driving ALL the electrodes with V = *sin(wt): Maximum force available for lock acquisition

12 What’s the problem?  the metallic part standing in for the QUAD mirror changes the behavior of the electric field between the ESD electrodes and the test mass TEST MASS It looks like each electrode driven by itself gives some response, but it doesn’t “see” the one next to it Possible explanation: Metallic structure ~1 inch glass plate metallic part ESD TEST MASS REFERENCE MASS

13 Finite Element Model (by Matt) Matlab model which solves electrostatic problems Given the potential on the conductors, it deduces the charge distribution on the conductors, the electric field and the potential everywhere in the space Example: Simple Capacitor

14 ESD Model for AdvLIGO Dielectric (Test Mass) Section perpendicular to the ESD plane Electrodes driven with +V, -V

15 ESD Model for AdvLIGO  Measured coupling coefficient about a factor 3 bigger than the expected one for Advanced LIGO, but maximum voltage difference available about 2.5 smaller (300V instead of 800V) Maximum force available for lock acquisition Section perpendicular to the ESD plane Fringe field Coupling coefficient in agreement with the expected one (within 50%)

16 ESD Model for LASTI - I Electrodes driven by +V, -V Negligible force on the ground plane Force on the dielectric due to the ESD fringe field, coupling coefficient  diff Electrodes driven by +V, +V Negligible force on the dielectric (no fringe field) Force on the ground due to the gradient of the potential, coupling coefficient  comm According to the model,  diff and  comm, are the same (bad luck??) and their value is compatible with the measured value (within 50%)

17 V con = V bias  F ~ 8V²  comm sin(ωt) V con = - V bias  F ~ 8V²  diff sin(ωt) ESD Model for LASTI - II F =  diff (V bias – V con )² +  comm (V bias + V con )² Ground plane which modifies the behaviour of the ESD V bias = V, V con = Vsin(ωt): F ~ 2V² (  comm -  diff ) sin(ωt) No fundamental if  comm =  diff V bias = V + Vsin(ωt) Same result if  comm =  diff Model explains the experimental results

18 +V 0 b d b << d ESD Model for LASTI - III Further cross check by analytically computing the coupling coefficient assuming the electrodes as a plane at the potential V rr x y 00 Computed coupling coefficient in agreement with the measured one (within 50%) and the one derived from the model

19 ESD Linearization Code FORCE VOLTAGE

20 ESD Linearization - Efficiency ESD 7 Hz  Reduction by about a factor 10 of the first harmonic

21 ESD Drive Cavity locked by acting on the triple (OSEM) Correction signals moved from the triple to the quad ESD: saturation due to frequency noise ( ~ Hz ) Phase lock loop: down to ~ Hz Frequency noise still too high! Cavity locked using the quad ESD above 20Hz and the triple OSEM below: only 25% change in the open loop TF of the longitudinal loop measured with the “right” (blue) and “wrong” (red) sign of the ESD loop “WRONG” SIGN “RIGHT” SIGN

22 Hierarchical Control Reallocation of the low frequency component of the mirror locking force to higher stages of the chain Less dynamic range needed for the mirror actuators  low noise state Sort of Hierarchical Control present in LIGO I (tidal control) More complex for multi-stage suspensions (VIRGO,..) M0 L1 L2 TM Main concern: couplings between the dofs of the different stages Never tested on the QUAD before

23 QUAD “Hierachical Control” ESD not able to be used to keep the lock (saturated by frequency noise) Test done by splitting the locking force between the TRIPLE (above 10 Hz) and the penultimate mass (L2) on the QUAD (below 10 Hz) Correction Signal Error Signal

24 Test Mass Charge: ESD as Sensor Top Mass (M0) driven at 2.5 Hz 4 electrodes of the ESD used as sensors, connected as input signal to an SR560 BSC ground connected to the SR560 ground M0 L1 L2 TM If the charge on the TM is not null, you expect to get a signal on the ESD at the driving frequency

25 Test Mass Charge: ESD as Sensor Signal measured by ESD

26 Test Mass Charge: ESD as Sensor Top Mass (M0) driven at 2.5 Hz 4 electrodes of the ESD used as sensors, connected as input signal to an SR560 BSC ground connected to the SR560 ground M0 L1 L2 TM If the charge on the TM is not null, you expect to get a signal on the ESD at the driving frequency Work function difference between Aluminium and Gold might be the cause for the signal that we measure The principle may still be valid without the metallic part

27 Summary ESD not behaving as designed, reasons understood Frequency noise in the present set-up too high Linearization code works properly Hierarchical Control: Cavity controlled below 10Hz acting on the penultimate mass of the QUAD

28 Plans Improve frequency stabilization (new input bench needed) Repeat tests (ESD, Lock Acquisition, Hierarchical Control) on QUAD Noise Prototype (test mass in glass)

The End

30 Frequency Noise Reduction Phase-lock loop: frequency noise reduced by about a factor 10

31 QUAD “Hierachical Control”