MSC recent activities COMM Cascina 5 Feb 2007. EM-MSC-0502072 Commissioning-oriented running activity Operation and interface updates Hardware checkup.

Slides:



Advertisements
Similar presentations
MSC recent activities virgoweek Cascina 4 Dec 2006.
Advertisements

Global longitudinal quad damping vs. local damping G v8 1.
Status of the Virgo Commissioning G.Losurdo – INFN Firenze/Urbino for the Virgo Collaboration.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
Payload design methods versus modeling E. Majorana.
Virgo commissioning update - VSR1 first month summary E. Tournefier WG1 meeting, Cascina June 20 th,2007.
Suspended Mirror control: Learning through Virgo Experience E. Majorana - I.N.F.N. Pisa Aspen GWAD February 16, 2004.
1 Virgo Commissioning progress and plans ILIAS, Jan 23 rd 2007 Matteo Barsuglia on behalf of the Commissioning Team.
rd ILIAS-GW annual general meeting 1 VIRGO Commissioning progress J. Marque (EGO)
Use ofSiesta in VIRGO commissioning Lisa Barsotti University of Pisa – INFN Pisa For the Virgo collaboration Caltech, December 19th 2003.
Present Superatttenuator performance vs. AdV & ET Requirements S.Braccini for Virgo Suspension group.
Virgo Control Noise Reduction
Stefan Hild 1ILIAS WG1 meeting, Cascina, November 2006 Comparison of tuned and detuned Signal-Recycling Stefan Hild for the GEO-team.
1 Ist Virgo+ review Cascina H. Heitmann Alignment: Virgo+ changes.
Thoughts on short term improvements for Mirror Suspension Control G.Losurdo - P.Ruggi.
Takanori Sekiguchi ALPS Report, Dec. 26th, 2013 Prototype Test of Type-B 1 Takanori Sekiguchi KAGRA F2F MEETING Feb
March 17, 2008LSC-Virgo meeting1/12 Virgo Status B. Mours.
EM-MSC MSC Columbus’ eggs VW EM-MSC outline EQG  SFR Note Actuation Noise: still under study, a framework of actions is being.
Virgo Commissioning update Gabriele Vajente for the Virgo Collaboration LSC/VIRGO Meeting – MIT 2007, July LIGO-G Z.
ILIAS – WG1 Hierarchical suspension control G.Losurdo INFN Firenze.
Takanori Sekiguchi External Review Alignment control servo for type-B/type-Bp (OpLev/WFS) 1 T. Sekiguchi.
MSC recent activities Commissioning Cascina 2 Apr 2007.
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.
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.
EM-MSC MSC staus & plans Commissioning meeting
Minimizing the Resonant Frequency of MGAS Springs for Seismic Attenuation System in Low Frequency Gravitational Waves Interferometers Maddalena Mantovani,
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.
MSC - 18 Oct 071 LOW FREQUENCY SEISMIC NOISE: LOCKING AND SENSITIVITY ISSUE Paolo Ruggi noise meeting.
ILIAS Geneva 29 March 2007 Virgo suspension control progress E. Majorana INFN Mirror Suspension Control workgroup.
Lecture 25: Implementation Complicating factors Control design without a model Implementation of control algorithms ME 431, Lecture 25.
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.
ILIAS WG1 meeting Han/Ruthe Harald Lück ILIAS WG1 meeting, Sep. 2004, Hannover/Ruthe GEO Status (Update)
Mirror Suspension Control commissioning learning
Adaptive Control Loops for Advanced LIGO
1 Commissioning meeting, Cascina, LA electronics noise budget ● Sources of electronic noise ● C7 electronic noise ● Electronic noise for optimized.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
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.
M. Mantovani ILIAS Cascina March 2008 Automatic Alignment system Improvements after the VSR1 M. Mantovani for the Alignment team.
Status of Virgo GWDAW12 Status of Virgo GWDAW Dec Leone B. Bosi INFN and University of Perugia (Italy) On behalf of the Virgo Collaboration.
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.
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.
20-22 July 2006 Maddalena Mantovani Automatic Alignment Noise Improvement M. Mantovani, H. Heitmann, J. Marque, P. Ruggi.
MSC, focus on: WI ghost noise. 1 “Recent” history and effect July 11 July 22 Aug 1 Jul 28 Aug 1 The disturbance, with us since Dec , had disappeared.
Filter #7 control April 18, 2016 –, Cascina Paolo Ruggi.
ALIGO HSTS Damping Loops Design Comparison J. Kissel, for the SUS and ISC Teams.
Advanced SA Specifications & Scientific Motivations S.Braccini, Cascina 21 Settembre 2007.
20/09/2006 EM MSC September /09/2006 EM MSC “activities” (from the web page, by Giovanni) are: - Inertial damping - Local control - Tide control.
Last stage SA F7 monitor/control
Type-A SAS Local Control Simulation (Current Status)
VIRGO–KAGRA Meeting about bottom filter damping
Present Superattenuator performance vs. ET Requirements S
Status of Virgo GWDAW Dec 13-16
Alignment status & plans
Control of the KAGRA Cryogenic Vibration Isolation System
Superattenuator for LF and HF interferometers
The Superattenuator upgrades and the SAFE Project
MSC report September weekly meeting EM-MSC
Frequency Noise in Virgo
Weekly meeting Cascina 9 Jan 2007
SUSPENSION CONTROL: a joint Virgo/LSC workshop
HAM-SAS Mechanics Status of modeling V.Boschi, V. Sannibale.
5/10/2019 MSC briefing Cascina 11-Dec 2006 wwwwwww.
weekly meeting Cascina 28 Nov 2006
Presentation transcript:

MSC recent activities COMM Cascina 5 Feb 2007

EM-MSC Commissioning-oriented running activity Operation and interface updates Hardware checkup and specific tests MSC performance VS disturbance

EM-MSC Main topic of this report: MSC disturbance rejection strategies Global Inverted Pendulum Control Vertical Damping implementation Sensor blending and Hybrid filters suspended done

EM-MSC Winter issues: STD scheme and blending used until Dec 2006 ACC LVDT + HP LP cross IP f crossover = 50 mHz Compromise between: 30 mHz (wind disturbance through ACC) and 70 mHz (  seism disturbance through LVDT) Note: since 2005 we have much larger margin on number of digital filter coefficients in the DSP and speed.

EM-MSC Winter issues: hybrid filters (W2S tuning with no download) ACC LVDT + HP  LP  IP + HPw LPw mix cross mix =0.5 : “medium” attenuation of  seism noise oldnew mix =0 (wind): not worse than old filters against  seism + tilt noise attenuation below 50 mHz oldnew mix =1 (  seism) : “strong” attenuation of  seism noise with slightly worsened tilt noise attenuation. oldnew How much is it enough ?

EM-MSC Winter issues: test of hybrid filters in use versus ITFstep12 Calm period mix= Hz, (IP notch) Pitch excitation (payload mode) yaw bump (due to large zM correction) Large zM due to tilt disturbance through accelerometers 3 mechanisms (at least): F0_z zCorr, F0_z  x, F0_z  y

EM-MSC Winter issues: WSR7, heuristic threshold for mix adjustment wind (mix 0)sea (mix 1)hic sunt leones

EM-MSC Winter issues: trend data: wind, no-sea Affordable situation using mix tuning ( 0) or GIPC mm mm mm mm mm mm

EM-MSC Winter issues: trend data: sea, no-wind Affordable situation using mix tuning ( 1) mm mm mm mm mm mm

EM-MSC Winter issues: trend data: 200 mHz bump uneasy situation using mix tuning only ( 0.5), GIPC to be studied mm mm mm mm mm mm

EM-MSC Winter issues: trend data: All, problems ! Need to assess more quantitative specs for HP/LP features VS weather conditions exploiting the mixing range (0-1). mm mm mm mm mm mm

EM-MSC F0_z zCorr : towards a more detailed model based upon measurements - Mechanism of zCorr contamination through LVDT noise re-injection. result: reconstructed zCorr matches observed zCorr We can consistently trust zCorr noise re-injection model (closed loop TF with different blending shapes and mix) V/sqrt(Hz) Hz

EM-MSC Winter issues: IP legs TF have to be properly considered to obtain consistent model Hz,Q=0.5). ACC LVDT HPLP mix cross IP seism In order to work-out a specs for LVDT cutoff we have to separate direct effect of microseism at the IP top level with respect to LVDT sensing. CL TF reconstruction versus measurement helps to attain a trustable model.

EM-MSC F0_z  x : towards a more detailed model based upon measurements Calibrated  x disturbance due to z mirror (and then to F0_z).

EM-MSC LP/HP optimization, given the standard actual corrector (cross) CL TF ACC LVDT HPLP mix cross IP seism mix=0.70 mix=0.90 mix=0.95 mix=1 LP/HP ratio versus CL TF Hz Two regions can be distinguished: A) LP/HP ratio plays a role attenuating LVDT sensor disturbance (  seism) B) No effect of LP/HP attenuation LVDT noise projection into zCorr 1) Hz V/sqrt(Hz) HPLP performance and mix optimized, limited-band gain enhancer tested.

EM-MSC WSR7 => WSR8 optimization under test Hz  ms -2 LP: anti-  seism previousWSR7 WSR8 accel. comparison

EM-MSC WSR7 => WSR8 optimization under test Hz  ms -2 HP: anti-wind (  previousWSR7 WSR8 LP: accel. comparison note: cleaner blending allows to re-tune HP to improve tilt re-injection

EM-MSC WSR7 => WSR8 overall tuning (mix 0-1) LP/HP mix 0 => 1 wind => sea mix 1 => 0 sea => wind A) assessing how much it is enough to enhance LP/HP to beat tilt re- injection is not easy. B) more data needed in windy-only conditions… C) no significant role played around the crossing frequency.

EM-MSC F0_z  y : Non-linear (quadratic) effect Three solutions : - zCorr reduction (mix 0); - digital compensation (not done yet),; - re-allocation of zCorr to input mirrors marionette (tested).

EM-MSC Hierarchical: zCorr reallocation to input mirror A reallocation mix option is available for WSR8 in case of wind (reduction large zM by a factor 2 lightens gain request to AA).

EM-MSC Hierarchical: zCorr reallocation to input mirrors (0.5, step1)

EM-MSC Conclusions: Provided that vertical damping is enabled and high gain AA filters are running and significantly improving the overall sensitivity. A more quantitative criterium to improve sensor blending and hybrid filters has been developed. We are close to “alpize” the mix parameter. More data and experience in windy conditions will help to design tilt noise reduction. It is not easy to work out a universal strategy valid if wind and  seism appear together are very strong. In order to limit anti-wind noise re-injection and request to AA marionette re-allocation has been enabled. Times are reasonably mature to restart GIPC studies. In parallel Siesta simulation of tilts is starting (G.L.).

EM-MSC V-damp ON/OFF one-by-one and OFF/ON All ALL OFF ALL ON O-B-O OFF O-B-O OFF No crucial Improvement during OBO Test. Clear Improvement All OFF/ON Relationship with Angular fluctuations