The Autoalignment System of GEO 600 Hartmut Grote and the GEO 600 team Max-Planck Institute for Gravitational Physics Amaldi, Perth 12-07-2001.

Slides:



Advertisements
Similar presentations
Factor each trinomial:
Advertisements

By D. Fisher Geometric Transformations. Reflection, Rotation, or Translation 1.
0 - 0.
Addition Facts
Stefan Hild for the GEO600 team October 2007 LSC-Virgo meeting Hannover Homodyne readout of an interferometer with Signal Recycling.
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) HOMODYNE AND HETERODYNE READOUT OF A SIGNAL- RECYCLED GRAVITATIONAL WAVE DETECTOR.
Stefan Hild (for the GEO-team) January 2008 GEO simulation meeting Attempts to measure the Optical Spring in GEO600.
Gravitational Wave Astronomy Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow Universität Jena, August 2010.
School Shop. Welcome to my shop. You have 10p How much change will you get? 7p 3p change.
19. October 2004 A. Freise Automatic Alignment using the Anderson Technique A. Freise European Gravitational Observatory Roma
The GEO 600 Detector Andreas Freise and the GEO 600 Team University of Hannover May 20, 2002.
Dual Recycling for GEO 600 Andreas Freise, Hartmut Grote Institut für Atom- und Molekülphysik Universität Hannover Max-Planck-Institut für Gravitationsphysik.
Addition 1’s to 20.
Doubles Facts Doubles with Pictures Doubles without Pictures Pictures Only.
1 LA general training session, Cascina Virgo alignment - overview - Nonlinear alignment = prealignment Linear alignment = autoalignment.
MAX-PLANCK-INSTITUT FÜR GRAVITATIONSPHYSIK ALBERT-EINSTEIN-INSTITUT Karsten Kötter1 Detector Characterization of GEO600 4th Edoardo Amaldi Conference.
Week 1.
Bottoms Up Factoring. Start with the X-box 3-9 Product Sum
Stefan Hild S4 Data Workshop, Hannover, May 2005 Title 1 kHz Glitches in S4 Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Status of the Virgo Commissioning G.Losurdo – INFN Firenze/Urbino for the Virgo Collaboration.
September 21, 2005Virgo Status – ESF Workshop1 Status of Virgo B. Mours.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Present status of the laser system for KAGRA Univ. of Tokyo Mio Lab. Photon Science Center SUZUKI, Ken-ichiro.
Cascina, January 24, 2005 Status of GEO600 Joshua Smith for the GEO600 team.
Status of the LIGO Project
LGS diagnostics Results (so far) Anna Moore, Hal Petrie LGS facility meeting 30 th Jan 2007.
Q09/2001 The GEO 600 Laser System LIGO-G Z V. Quetschke°, M. Kirchner°, I.Zawischa*, M. Brendel*, C. Fallnich*, S. Nagano +, B. Willke° +, K.
Towards dual recycling with the aid of time and frequency domain simulations M. Malec for the GEO 600 team Max-Planck-Institut für Gravitationsphysik Albert-Einstein-Institut.
G D Tasks After S3 Commissioning Meeting, Oct 6., 2003 Peter Fritschel, Daniel Sigg.
GEO600 Harald Lück Ruthe, Worldwide Interferometer Network.
Virgo Control Noise Reduction
Katrin Dahl for the AEI 10 m Prototype team March 2010 – DPG Hannover Q29.1 Stabilising the distance of 10 m separated.
Stefan Hild 1Ilias WG1 meeting, Sep 2005, Perugia Title GEO 600 Commissioning progress Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) Institut für Atom- und Molekülphysik Detector Characterization of GEO 600 during.
Joshua Smith December 2003 Detector Characterization of Dual-Recycled GEO600 Joshua Smith for the GEO600 team.
The GEO 600 Detector Andreas Freise for the GEO 600 Team Max-Planck-Institute for Gravitational Physics University of Hannover May 20, 2002.
Interferometer Control Matt Evans …talk mostly taken from…
04. November 2004 A. Freise A. Freise, M. Loupias Collaboration Meeting November 04, 2004 Alignment Status.
GEO600 Detector Status Harald Lück Max-Planck Institut für Gravitationsphysik Institut für Atom- und Molekülphysik, Uni Hannover.
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
Squeezed light and GEO600 Simon Chelkowski LSC Meeting, Hannover.
1 Virgo commissioning: Next steps December 12 st 2005 Hannover, ILIAS-GWA WG1 Matteo Barsuglia, LAL/CNRS.
1/30 Challenge the future Auto-alignment of the SPARC mirror W.S. Krul.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
LIGO-G D Commissioning, Part II PAC 12, June 2002 Peter Fritschel, LIGO MIT.
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 August G Z Gingin High Optical Power Test Facility (AIGO) 1 High Optical Power Test Facility - Status First lock, auto-alignment and.
Status of the Advanced LIGO PSL development LSC Virgo meeting, Caltech, March 2008 LIGO G Z Benno Willke for the PSL team.
Abstract The Hannover Thermal Noise Experiment V. Leonhardt, L. Ribichini, H. Lück and K. Danzmann Max-Planck- Institut für Gravitationsphysik We measure.
Perugia, Italy Reducing the Noise in GEO600 Joshua Smith for the GEO 600 team.
Dual Recycling in GEO 600 H. Grote, A. Freise, M. Malec for the GEO600 team Institut für Atom- und Molekülphysik University of Hannover Max-Planck-Institut.
1 Virgo Commissioning Status WG1 meeting Potsdam, 21 st July 2006.
Modeling of the Effects of Beam Fluctuations from LIGO’s Input Optics Nafis Jamal Shivanand Sanichiro Yoshida Biplab Bhawal LSC Conference Aug ’05 LIGO-G Z.
Alexander Khalaidovski, Henning Vahlbruch, Hartmut Grote, Harald Lück, Benno Willke, Karsten Danzmann and Roman Schnabel STATUS OF THE GEO HF SQUEEZED.
G D LIGO Commissioning Update LSC Meeting, Nov. 11, 2003 Daniel Sigg.
Status of GEO600 Benno Willke for the GEO600 team ESF Exploratory Workshop Perugia, September 2005.
Sensitivity of Virgo E. Tournefier (LAPP-CNRS) LSC-Virgo week May 23 rd,2007 LIGO-G Z.
1 ILIAS WG1 meeting, Hannover The 2 nd modulation frequency project.
GEO600 – The output mode cleaner Mirko Prijatelj for the GEO600-Team Institute for Gravitational Physics Albert-Einstein-Institute Hannover / Germany.
EFC Media Center Training
GEO600 Control aspects where do the error signal come from?
Signal recycling R&D at LAL: Influence in Virgo
Calibration of data in the time domain (or how to generate 1800s long SFTs from time domain data) XS, Bruce Allen, Mike Landry, Soumya Mohanty, Malik.
Commissioning Update PAC 15, Dec. 11, 2003 Daniel Sigg.
Commissioning progress Stefan Hild Ilias WG1 meeting, Sep 2005
Workshop on Gravitational Wave Detectors, IEEE, Rome, October 21, 2004
Virgo Update – LSC meeting
LIGO Interferometry CLEO/QELS Joint Symposium on Gravitational Wave Detection, Baltimore, May 24, 2005 Daniel Sigg.
Optimal on-line time-domain calibration of the
Presentation transcript:

The Autoalignment System of GEO 600 Hartmut Grote and the GEO 600 team Max-Planck Institute for Gravitational Physics Amaldi, Perth

Autoalignment - Purposes Superimpose cavity axes with incoming beam - Differential wavefront sensing (analog feedback for 14 DOF) Center beam spot positions on mirrors - Spot position sensing (digital feedback for 20 DOF)

Autoalignment Experimental setup for 1 cavity

Autoalignment Experimental setup for 1 cavity

Autoalignment Experimental setup for 1 cavity

Autoalignment Experimental setup for 1 cavity Differential wavefront sensing Orthogonalization < 1/10 Bandwith 0.2 or 6 Hz Sensitivity typ. 10 p rad / sqrt(Hz)

Autoalignment Experimental setup for 1 cavity Local beam centering servos Bandwith ~ 1kHz

Autoalignment Experimental setup for 1 cavity Spot position control

Autoalignment - Switching On and Off

Modecleaner Alignment Drift Over 1 Day

Autoalignment setup PR + MI cavity

PR Mirror Rotation Autoalignment Errorsignal