9th LISA Symposium Paris, 22/05/2012 Optimization of the system calibration for LISA Pathfinder Giuseppe Congedo (for the LTPDA team)

Slides:



Advertisements
Similar presentations
BL OOS GG workshop, Pisa / S.Piero a Grado 2/26/2010, Thales Alenia Space Template reference : S-EN INTERNAL THALES ALENIA SPACE COMMERCIAL.
Advertisements

A synthetic noise generator M. Hueller LTPDA meeting, AEI Hannover 27/04/2007.
Lectures 12&13: Persistent Excitation for Off-line and On-line Parameter Estimation Dr Martin Brown Room: E1k Telephone:
Global longitudinal quad damping vs. local damping G v8 1.
Principal Component Analysis Based on L1-Norm Maximization Nojun Kwak IEEE Transactions on Pattern Analysis and Machine Intelligence, 2008.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Hubert HalloinScientific Committee 2013 WP Interface I3(APC/IPGP) : Fundamental Physics and Geophysics in Space Introduction and context  Fundamental.
PhD oral defense 26th March 2012 Spacetime metrology with LISA Pathfinder Giuseppe Congedo Advisors:Prof. Stefano Vitale Dr. Mauro Hueller.
DFT/FFT and Wavelets ● Additive Synthesis demonstration (wave addition) ● Standard Definitions ● Computing the DFT and FFT ● Sine and cosine wave multiplication.
The evaluation and optimisation of multiresolution FFT Parameters For use in automatic music transcription algorithms.
Nazgol Haghighat Supervisor: Prof. Dr. Ir. Daniel J. Rixen
Prénom Nom Document Analysis: Data Analysis and Clustering Prof. Rolf Ingold, University of Fribourg Master course, spring semester 2008.
EE311: Junior EE Lab Phase Locked Loop J. Carroll 9/3/02.
Pattern Recognition. Introduction. Definitions.. Recognition process. Recognition process relates input signal to the stored concepts about the object.
Maximum likelihood (ML)
Introduction To Signal Processing & Data Analysis
Doppler Radar From Josh Wurman Radar Meteorology M. D. Eastin.
On the Accuracy of Modal Parameters Identified from Exponentially Windowed, Noise Contaminated Impulse Responses for a System with a Large Range of Decay.
TeV Particle Astrophysics August 2006 Caltech Australian National University Universitat Hannover/AEI LIGO Scientific Collaboration MIT Corbitt, Goda,
LE 460 L Acoustics and Experimental Phonetics L-13
Lecture 1 Signals in the Time and Frequency Domains
1/25 Current results and future scenarios for gravitational wave’s stochastic background G. Cella – INFN sez. Pisa.
Sensitivity Analysis and Experimental Design - case study of an NF-  B signal pathway Hong Yue Manchester Interdisciplinary Biocentre (MIB) The University.
Part 5 Parameter Identification (Model Calibration/Updating)
Z B Zhou, Y Z Bai, L Liu, D Y Tan, H Yin Center for Gravitational Experiments, School of Physics, Huazhong University of Science.
LIGO- G Z August 19, 2004Penn State University 1 Extracting Signals via Blind Deconvolution Tiffany Summerscales Penn State University.
EEG Classification Using Maximum Noise Fractions and spectral classification Steve Grikschart and Hugo Shi EECS 559 Fall 2005.
Stochastic Linear Programming by Series of Monte-Carlo Estimators Leonidas SAKALAUSKAS Institute of Mathematics&Informatics Vilnius, Lithuania
Optimal Experimental Design Theory. Motivation To better understand the existing theory and learn from tools that exist out there in other fields To further.
John W. Conklin, 9 th International LISA Symposium, Paris, 23 May Estimation of the LISA TM-to-release tip adhesion force during dynamic separation.
LIGO-G Z Peter Shawhan, for the LIGO Scientific Collaboration APS Meeting April 25, 2006 Search for Gravitational Wave Bursts in Data from the.
Institute of Flight Mechanics and Control Barcelona, LISA7 Symposium, June 17th 2008 IFR – University of Stuttgart LISA Pathfinder.
Dusanka Zupanski And Scott Denning Colorado State University Fort Collins, CO CMDL Workshop on Modeling and Data Analysis of Atmospheric CO.
Structural Dynamics & Vibration Control Lab. 1 Kang-Min Choi, Ph.D. Candidate, KAIST, Korea Jung-Hyun Hong, Graduate Student, KAIST, Korea Ji-Seong Jo,
Progress in identification of damping: Energy-based method with incomplete and noisy data Marco Prandina University of Liverpool.
Center for Radiative Shock Hydrodynamics Fall 2011 Review Assessment of predictive capability Derek Bingham 1.
PeTeR: a hardware simulator for LISA PF TM-GRS system 23/05/ th LISA Symposium May 2012, BnF Paris L. Marconi and R. Stanga Università degli.
1SBPI 16/06/2009 Heterodyne detection with LISA for gravitational waves parameters estimation Nicolas Douillet.
Amaldi 9 Cardiff University July 2011 Parameter estimation for LISA Pathfinder Giuseppe Congedo University of Trento for the LTPDA team.
Noise and Sensitivity of RasClic 91
Possibility of tan  measurement with in CMS Majid Hashemi CERN, CMS IPM,Tehran,Iran QCD and Hadronic Interactions, March 2005, La Thuile, Italy.
July 11, 2006Bayesian Inference and Maximum Entropy Probing the covariance matrix Kenneth M. Hanson T-16, Nuclear Physics; Theoretical Division Los.
Robert Engle UCSD and NYU and Robert F. Engle, Econometric Services DYNAMIC CONDITIONAL CORRELATIONS.
NCAF Manchester July 2000 Graham Hesketh Information Engineering Group Rolls-Royce Strategic Research Centre.
Calibration in the Front End Controls Craig Cahillane LIGO Caltech SURF 2013 Mentors: Alan Weinstein, Jamie Rollins Presentation to Calibration Group 8/21/2013.
Monte-Carlo based Expertise A powerful Tool for System Evaluation & Optimization  Introduction  Features  System Performance.
Adaptive Control Loops for Advanced LIGO
Development of a Readout Scheme for High Frequency Gravitational Waves Jared Markowitz Mentors: Rick Savage Paul Schwinberg Paul Schwinberg.
Sensitivity Analysis and Experimental Design - case study of an NF-  B signal pathway Hong Yue Manchester Interdisciplinary Biocentre (MIB) The University.
Ultra-high dimensional feature selection Yun Li
Chance Constrained Robust Energy Efficiency in Cognitive Radio Networks with Channel Uncertainty Yongjun Xu and Xiaohui Zhao College of Communication Engineering,
Penn State, 20 th -24 th July TH INTERNATIONAL LISA S YMPOSIUM D. Bortoluzzi, M. Da Lio, S. Vitale1 LTP dynamics and control D. Bortoluzzi, M. Da.
Stochastic Background Data Analysis Giancarlo Cella I.N.F.N. Pisa first ENTApP - GWA joint meeting Paris, January 23rd and 24th, 2006 Institute d'Astrophysique.
1 Tom Edgar’s Contribution to Model Reduction as an introduction to Global Sensitivity Analysis Procedure Accounting for Effect of Available Experimental.
Tutorial 2, Part 2: Calibration of a damped oscillator.
Comparison of filters for burst detection M.-A. Bizouard on behalf of the LAL-Orsay group GWDAW 7 th IIAS-Kyoto 2002/12/19.
LTP Barcelona_26_27_06_2007 S. Vitale1 Master Plan Analyses DA#6.
ESA Living Planet - Begen – June B. Christophe, J-P. Marque, B. Foulon ESA LIVING PLANET SYMPOSIUM June 28 th -July 2 nd 2010 Bergen (Norway)
UTN synthetic noise generator M. Hueller LTPDA meeting, Barcelona 26/06/2007.
1 Chapter 5 Branch-and-bound Framework and Its Applications.
بسم الله الرحمن الرحيم Digital Signal Processing Lecture 2 Analog to Digital Conversion University of Khartoum Department of Electrical and Electronic.
Part 3: Estimation of Parameters. Estimation of Parameters Most of the time, we have random samples but not the densities given. If the parametric form.
Fundamentals of Data Analysis Lecture 11 Methods of parametric estimation.
Amplitude and time calibration of the gw detector AURIGA
MECH 373 Instrumentation and Measurements
OSE801 Engineering System Identification Spring 2010
MECH 373 Instrumentation and Measurements
CJT 765: Structural Equation Modeling
Title International Training Course, Rabat 2012 E. Wielandt:
LOCATION AND IDENTIFICATION OF DAMPING PARAMETERS
Presentation transcript:

9th LISA Symposium Paris, 22/05/2012 Optimization of the system calibration for LISA Pathfinder Giuseppe Congedo (for the LTPDA team)

Outline  Model of LPF dynamics: what are the system parameters? 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris2 Incidentally, we talk about:  Optimization method  System/experiment constraints  System calibration: how can we estimate them?  Optimization of the system calibration: how can we improve those estimates?

Motivation 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris3  The reconstructed acc. noise is parameter-dependent  For this, we need to calibrate the system  In the end, better precision in the measured parameters → better confidence in the reconstructued acc. noise Differential acceleration noise to appear in Phys. Rev. Uncertainties on the spectrum:  Parameter accuracy: system calibration  Parameter precision: optimization of calibration  Statistical uncertainty: PSD estimation stat. unc. of PSD estimation system calibration calibrated uncalibrated

Model of LPF dynamics 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris4 guidance signals: reference signals for the drag-free and elect. suspension loops  force gradients (~1x10 -6 s -2 )  sensing cross-talk (~1x10 -4 )  actuation gains (~1) direct forces on TMs and SC Science mode: TM 1 free along x, TM 2 /SC follow

Framework 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris5 sensed relative motion o 1, o 12 system calibration (system identification) parameters ω 1 2, ω 12 2, S 21, A df, A sus diff. operator Δ equivalent acceleration noise optimization of system calibration (optimal design)

System calibration 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris6 LPF system o i,1 o i,12... o1o1 o LPF is a multi-input/multi-output dynamical system. The determination of the system parameters can be performed with targeted experiments. We mainly focus on: Exp. 1: injection into the drag-free loop Exp. 2: injection into the elect. suspension loop

System calibration 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris7 residuals cross-PSD matrix  We build the joint (multi-experiment/multi-outputs) log-likelihood for the problem  The system response is simulated with a transfer matrix  The calibration is performed comparing the modeled response with both translational IFO readouts

Calibration experiment 1 Exp. 1: injection of sine waves into o i,1  injection into o i,1 produces thruster actuation  investigation of the drag-free loop 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris8 black: injection Standard design

Calibration experiment 2 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris9 Exp. 2: injection of sine waves into o i,12  injection into o i,12 produces capacitive actuation on TM 2  investigation of the elect. suspension loop black: injection Standard design

Optimization of system calibration 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris10 modeled transfer matrix evaluated after system calibration noise cross PSD matrix input signals being optimized estimated system parameters input parameters (injection frequencies) Question: how can we optimize the experiments, to get an improvement in parameter precision? gradient w.r.t. system parameters Answer: use the Fisher information matrix of the system (method already found in literature and named “theory of optimal design of experiments”)

Optimization strategy 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris11 practically speaking... Either way, the optimization seeks to minimize the “covariance volume” of the system parameters Perform a non-linear optimization (over a discrete space of design parameter values) of the scalar estimator 6 optimization criteria are possible:  information matrix, maximize: - the determinat - the minimum eigenvalue - the trace [better results, more robust]  covariance matrix, minimize: - the determinant - the maximum eigenvalue - the trace

Experiment constraints 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris12  Can inject a series of windowed sines  Fix the experiment total duration T ~ 2.5 h  For transitory decay, allow gaps of length δt gap = 150 s  Require that each injected sine must start and end at zero (null boudary conditions) → each sine wave has an integer number of cycles → all possible injection frequencies are integer multiples of the fundamental one → the optim. parameter space (space of all inj. frequencies) is intrinsically discrete → the optimization may be challenging  Divide the experiment in injection slots of duration δt = 1200 s each. This set the fundamental frequency, 1/1200 ~ 0.83 mHz.

System constraints 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris13  Capacitive authority, 10% of 2.5 nN  Thruster authority, 10% of 100 µN  Interferometer range, 1% of 100 µm → as the injection frequencies vary during the optimization, the injection amplitudes are adjusted according to the constraints above For safety reason, choose not to exceed:

System constraints 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris14  for almost the entire frequency band, the maximum amplitude is limited by the interferometer range  since the data are sampled at 1 Hz, we conservatively limit the frequency band to a 10th of Nyquist, so <0.05 Hz o i,12 inj. (Exp. 2)o i,1 inj. (Exp. 1) maximum injection amplitude (dashed) VS injection frequency interferometer

Optimization of calibration 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris15 initial-guess parameters ω 1 2, ω 12 2, S 21, A df, A sus best-fit parameters ω 1 2, ω 12 2, S 21, A df, A sus system calibration optimization of system calibration optimized experimental designs Discrete optimization may be an issue! Overcome the problem by: 1)overlapping a grid to a continuous variable space 2)rounding the variables (inj. freq.s) to the nearest grid node 3)using direct algorithms robust to discontinuities (i.e., patternsearch)

ParameterDescription Nominal value Standard design σ Optimal design σ ω 1 2 [s -2 ] Force (per unit mass) gradient on TM 1, “1st stiffness” -1.4x x x ω 12 2 [s -2 ] Force (per unit mass) gradient between TM 1 and TM 2, “differential stiffness” -0.7x x x S 21 Sensing cross-talk from x 1 to x 12 1x x x10 -7 A df Thruster actuation gain 17x x10 -4 A sus Elect. actuation gain 11x x10 -6 Optimization of exp. 1 & 2 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris16  Improvement of factor 2 through 7 in precision, especially for A df (important for the subtraction of thruster noise)  There are examples for which correlation is mitigated: Corr[S 21, ω 12 2 ]=-20%->-3%, Corr[ω 12 2, S 21 ]=9%->2%

Optimization of exp. 1 & 2 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris17 The optimization converged to:  Exp. 1: lowest (0.83 mHz) and highest (49 mHz) allowed frequencies  Exp. 2: highest (49 mHz) allowed frequency (plus a slot with 0.83 mHz)

Optimization of exp. 1 & 2 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris18 Optimized design: Exp. 1: mHz, 3 49 mHz Exp. 2: mHz, 6 49 mHz why is it so? the physical interpretation is within the system transfer matrix The optimization:  converges to the maxima of the transfer matrix  balances the information among them Exp. 1 Exp. 2

Effect of frequency-dependences 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris19 loss angle nominal stiffness, ~-1x10 -6 s -2 dielectric loss gas damping Simulation of the response of the system to a pessimistic range of values: δ 1, δ 2 = [1x10 -6,1x10 -3 ] s -2 τ 1, τ 2 = [1x10 5,1x10 7 ] s However, the biggest contribution is due to gas damping, Cavalleri A. et al., Phys. Rev. Lett. 103, (2009) (N 2, gas venting directly to space) (Ar)

Concluding remarks  The optimization of the system calibration shows: ‐improved parameter precision ‐improved parameter correlation  The optimization converges to only two relevant frequencies which corresponds to the maxima of the system transfer matrix; this leads to a simplification of the experimental designs  Possible frequency-dependences in the stiffness constants do not impact the optimization of the system calibration  However, we must be open to possible frequency-dependences in the actuation gains [to be investigated]  The optimization of the system calibration is model-dependent, so it must be performed once we have good confidence on the model 22/05/2012Giuseppe Congedo - 9th LISA Symposium, Paris20

Thanks for your attention! Giuseppe Congedo - 9th LISA Symposium, Paris22/05/ and to the Trento team for the laser pointer (the present for my graduation)!