Vibration Isolation Group

Slides:



Advertisements
Similar presentations
Extra Large Telescope Wind Engineering. Wind and Large Optical Telescopes Wind is a key factor in the design of large telescopes: larger wind-induced.
Advertisements

Vibration Isolation Group R. Takahashi (ICRR)Chief T. Uchiyama (ICRR)Payload design H. Ishizaki (NAOJ)Prototype test R. DeSalvo (Caltech)SAS design A.
Participants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage.
CLIO Current Status of Japanese Detectors Daisuke Tatsumi National Astronomical Observatory of Japan.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
Control strategy in the vibrtion isolation system for KAGRA Ryutaro Takahashi (Institute for Cosmic Ray Research, Univ. of Tokyo / National Astronomical.
Seismic attenuation chains concept, design and advancement status Riccardo DeSalvo for the KAGRA Seismic group JGW-G September 10, 20121JGW-G
LCGT seismic Attenuation System DRADF DRAFT DRAFT DRAFT.
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.
Vibration and isolation. Seismic isolation Use very low spring constant (soft) springs Tripod arrangement used for mounting early AFM’s Had long period.
ICRR M2 Takanori Sekiguchi ICRR, NAOJ A, ERI B, Sannio Univ. C, INFN Roma D, NIKHEF E, AEI F Ryutaro Takahashi, Kazuhiro Yamamoto, Takashi Uchiyama, Hideharu.
DX Upper Tree-House & Fan 12 June, 2010 Esguerra.
Vibration Isolation R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR), H. Ishizaki (NAOJ), A. Takamori (ERI), R. DeSalvo.
SEO report _SAITO 1. Overall schedule of iKAGRA installation/commissioning change to Michelson Interferometer 2. Scheduling of daily works for installation.
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
Status of LCGT and CLIO Masatake Ohashi (ICRR, The University of TOKYO) and LCGT, CLIO collaborators TAUP2007 Sendai, Japan 2007/9/12.
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
IFE Plant Structural Concepts Including Shielding and Optical Stability Requirements Thomas Kozub, Charles Gentile, Irving Zatz - PPPL.
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.
CLIC MDI Working Group Vibration attenuation via passive pre- isolation of the FF quads A. Gaddi, H. Gerwig, A. Hervé, N. Siegrist, F. Ramos.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
Simulation for KAGRA cryogenic payload: vibration via heat links and thermal noise Univ. Tokyo, D1 Takanori Sekiguchi.
G. Barber Sci-Fi Tracker Progress Ral 28 Oct Progress On The Design Of The Full Tracker Contents:- Recap of New Station Layout Version 2.5 Version.
Behavior of an inverted pendulum in the Kamioka mine R. Takahashi (NAOJ), A. Takamori (ERI), E. Majorana (INFN) GWADW 2010 We are investigating behavior.
LCGT Technical Review Suspension Point Interferometer for Parasitic Noise Reduction and an Additional IFO S.Miyoki (ICRR, Univ. of TOKYO)
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi GWADW in Hawaii.
Steel Honeycomb Vibration Isolation Tables
LIGO-G Z Guido Mueller University of Florida For the LIGO Scientific Collaboration ESF Exploratory Workshop Perugia, Italy September 21 st –23.
Understanding Cabling Noise in LIGO Chihyu Chen Lafayette College Mentors: Mark Barton Norna Robertson Helpful Researcher:Calum Torrie Co-SURF:Julian Freed-Brown.
New in-air seismic attenuation system for the next generation gravitational wave detector M.R. Blom, A. Bertolini, E. Hennes, A. Schimmel, H.J. Bulten,
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
ACIGA High Optical Power Test Facility
Low frequency anti-vibration system of LCGT Vibration Isolation Group R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
Two Layers SAS: Damping of Torsion Mode Feb. 5th, 2011 F2F Meeting Takanori Sekiguchi, Riccardo DeSalvo, Ryutaro Takahashi 1/8.
LIGO-G R Inverted pendulum studies for seismic attenuation Ilaria Taurasi University of Sannio at Benevento, Italy September 20, 2005 Supervisor.
External forces from heat links in cryogenic suspensions D1, ICRR, Univ. Tokyo Takanori Sekiguchi.
Vibration Isolation Subsystem KAGRA face to face meeting (31 July, 2012) R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
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.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The University of Tokyo KAGRA external review (Cryogenic payload) 18 April 2012.
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,
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research The university of Tokyo LCGT internal review (Cryogenic payload) 30 January 2012.
Active Vibration Isolation using a Suspension Point Interferometer Youichi Aso Dept. Physics, University of Tokyo ASPEN Winter Conference on Gravitational.
E. Majorana (INFN – Rome) ELiTES 3 rd General Meeting Hongo Campus – Tokyo – 9-10 Feb., 2015 Cryogenic platform with vertical suspension: a practical approach.
Yoichi Aso Columbia University, New York, NY, USA University of Tokyo, Tokyo, Japan July 14th th Edoardo Amaldi Conference on Gravitational Waves.
Short or Tall?. Short Tall Short Tall Short Tall. 3
Overview of the 20K configuration
Type-A SAS Local Control Simulation (Current Status)
Pros and cons of cryogenics for Einstein Telescope and Cosmic Explorer
Kazuhiro Yamamoto on behalf of KAGRA collaboration
KAGRA用防振装置の開発 VIII Configuration Sensors and Actuators
LCGT Seismic Attenuation System LCGT-SAS
Kazuaki Kuroda On behalf of LCGT Collaboration
Control of the KAGRA Cryogenic Vibration Isolation System
External forces from heat links in cryogenic suspensions
Vibration Isolation Systems
Superattenuator for LF and HF interferometers
Cryogenic Payload Modeling: Vibration via Heat Links
The Superattenuator upgrades and the SAFE Project
Fishing Rod Design for KAGRA GAS Filters
HAM-SAS Mechanics Status of modeling V.Boschi, V. Sannibale.
Development of vibration isolation systems for LCGT VII
Cryogenic Suspension for KAGRA and Suspension Thermal Noise Issues
Cryogenic Payload Modeling: Vibration via Heat Links
Presentation transcript:

Vibration Isolation Group Two-layer configuration Budget → tunnel group Schedule Installation and Maintenance Short Inverted Pendulum LCGT A-review of VIS (20 Dec., 2010) 1

Generalities 4m φ (→8m x 12m) x 4m h (→7m) upper tunnel containing pre-attenuator 1.2m diameter 5m tall bore-hole with SAS chain 5.5m (→8m) tall containing main beam and cryostat

(2) Schedule

(3) Installation and Maintenance Ease of installation No need of large, expensive rigid structures Much lighter crane (1t) requirements

Disposition of GAS filters Case (1): 4 filers are placed every 2m. Eddy current damping to the Filter1 works effectively (<10min). Careful wiring between filters is necessary. One long wire (in TAMA) → Short wire chain with anchored connector. Case (2): 3 filters are inside the upper chamber. It is difficult to damp the torsion mode (>1h). If thick 7-m wire is used, a frequency of the wire resonance becomes too low (~10Hz). Maintenance of filters is easer.

Damping of torsion mode Case (1) Case (2) Filter0 3.74mm x 2.1m 3.42mm x 0.8m Filter1 3.44mm x 2.1m Filter2 3.11mm x 2.1m 3.98mm x 7.0m Filter3 2.74mm x 2.1m CB 2.45mm x 1.0m 2.44mm x 1.0m by T. Sekiguchi

(4) Short Inverted Pendulum Pre-isolator footed on solid rock It was found that small size = better performance Easy of access for pre-isolator tuning

Performance of IP Short IP is sensitive to the load. Performance by H. Ishizaki Short IP is sensitive to the load. Performance Long IP (NIM A582, 683) ~50dB Short IP (NIM A598, 737) ~80dB

Disadvantages Need new bore-holes to re-position any optical element Need to know where to locate all mirrors ! Will need 1200 mm diameter or oval boreholes to allow for ±100 mm tuning of PR, SR, ITM mirrors

In the case of one layer. External rigid structure Base for IP on bottom of the chamber like TAMA-SAS → It is difficult to apply to Type-A system.