Detector Characterization Status. K. Hayama (ICRR), KAGRA detchar subsystem
|
|
- Roy Dean
- 5 years ago
- Views:
Transcription
1 Detector Characterization Status K. Hayama (ICRR), KAGRA detchar subsystem
2 Scope Detector diagnostics system Data quality Veto analysis
3 Tasks Support to understand what is happening in KAGRA DetChar tools Environmental monitor sensors and PEM injection Study of environmental issues Data quality Information for operation, data analysis To define DQ using DetChar tools Practice : ikagra data characterization Selection of channels to use for DQ Distribution of DQ flag to collaborators Veto Information for data analysis Multi-channel analysis Safe, unsafe channel analysis
4 Tasks Support to understand what is happening in KAGRA DetChar tools Environmental monitor sensors and PEM injection Study of environmental issues Data quality Information for operation, data analysis To define DQ using DetChar tools Practice : ikagra data characterization Selection of channels to use for DQ Distribution of DQ flag to collaborators Veto Information for data analysis Multi-channel analysis Safe, unsafe channel analysis
5 command line tools for characterization, web daily summary, monitoring etc. Non Stationary Line User Interface command line webbased Monitoring Pages Gaussianity Summary Pages Time Series Spectrum Environmental Monitors Data Categorization DQ flag Sensors Preparation Arm mapping ikagra Paper DQ application Connection PEM Injection GW range Correlation System Health etc. ChirpletMon Site Study magnetic field water gravity Logistics support DetChar Shifts
6 command line tools for characterization, web daily summary, monitoring etc. Non Stationary Line User Interface command line webbased Monitoring Pages Gaussianity Summary Pages Time Series Spectrum >60 command line tools are developed and updating for using NDS tools Environmental Monitors Data Categorization DQ flag Sensors Preparation Arm mapping Connection DQ application ikagra data characterization PEM Injection GW range Correlation System Health etc. ChirpletMon Site Study magnetic field water gravity Logistics support DetChar Shifts
7
8 DetChar Tools Glitch Monitor Line Finder Line Tracking Line Removal Rayleigh Monitor Non-Stationarity Line Gaussianity Coherence Finder Multiple-channel coherence finder (BruCo) Pearson correlation Finder NonLinear correlation Finder Realtime Quick look webpage Daily summary webpage GUI Interface Web-Base Interface Command-line Interface Health monitor File Finder (New) Globally Correlated magnetic noise Violin mode Non-Gaussianity Monitor RMS Monitor Noise Floor Monitor Time-Series Monitor Spectrum Monitor Spectrogram Monitor Sensitivity Monitor Range Monitor Time-Series Spectrum GW Range Correlation Inspiral Inspiral-Merger-Ringdown Multi-channel analysis Ringdown Newtonian noise Stochastic User Interface System Health Effect of water inside the mountain
9 Web based diagnostics tools
10 Daily Summary Monitors
11 Env. sensor locations Y end table IMC TRANS EY3 BS, X,Y Front MC MCF PSL IMMT2T IFI IO IMC REFL Seis PRM IMM EYC EYA Y EY4 rack MCE TRY EY2 chamber Temp Therm Baro Mag EYT IYA 1F 2F Temp Temp Therm Therm Baro Baro Seis Seis PR2 Mag Mag PR3 arm (Temp,therm,Ba ro)x2,... X arm PCY1 IYC IY1 IX1 PCX1 BS 1F Temp Therm Baro Seis Mag 2F Temp Therm Baro Seis Mag IXC (Temp,therm,Ba ro)x2,... IXA EXA EXC EXT IMMT1T REFL MMTPRM POY LSC ASC1ASC2AUX EX2 EX3 EX4 POP SR2 PR2 BS SR2 SR3 OMM POS POX AS? AS Server room 2F Temp Therm Baro Seis Mag 1F Temp Therm Baro Seis Mag X end 11
12 On-Going Magnetometer Thermometer, Barometer, Hygrometer cabling, making amps, for the connection to rack 2 start test operation at the X arms (GIF DAQ) cabling, making amps, for the connection to rack Seismometer 2 is running around BS, at Xfront 1 is tested for the Type-A experiment 12
13 Water gravity noise 13
14 14
15 Water Newtonian Noise Estimation Nishizawa(Nagoya) water flow along an open channel O Sn ~ function of b^(-1/2) O Sn ~ function of v sensitive to velocity (assuming a smooth surface for a water pipe and negligible transverse velocity)
16 CDF X Model Z ow fl r e t Wa Result Y Kasuya (Titech) Conditions Material: Water Initial Velocity: 1000 mm/s Initial water surface height: mm Boundary flow velocity:1000 mm/s Analysis time: 10 sec Φ443 mm L=1024 mm Groove width: 20 mm Groove height: 38 mm (30,0,-700) Time vs Vz Flow Velocity at(30,0,-700)
17 Measurement of magnetic fields with LI GO and Virgo Test of filtering correlated magnetic field noise at KAGRA Virgo S. Atsuta, K. Hayama, S.Kataoka, T. Ogawa, K.Somiya, Nelson Christensen, Michael Coughlin, Rosario Derosa, Irene Fiori, Mark Golkowski, Melissa Guidry, Jan harms, Jerzy Kubisz, Andrzej Kulakm, Janusz Mlynarczyk, Federico Paoletti, Tristan Shoemaker, Eric Thrane
18 Filter to mitigate the Schumann resonance
19 Measurement Magnetometers (fromeri, U. tokyo) GPS time stamps for studying coherence between the sites KAGRA Villa Cristina
20 Coherence KAGRA-Villa Cristina (North-South direction)
21 Filter performance
22 Schedule Update of tools, web-based summary page, quick look page (CRY) Environmental sensors prepared sensors initially will be running ~July, 2017 Unknown environmental noise Dec, 2017 effect of water gravity noise ~June, 2017 DQ study November, 2017
23 Interface
Status of KAGRA Detector Characterization. Kazuhiro Hayama (Osaka City Univ.) on behalf of the detector characterization group
Status of KAGRA Detector Characterization Kazuhiro Hayama (Osaka City Univ.) on behalf of the detector characterization group Interface of the detector characterization Two Direction : To provide system,
More informationDownselection of observation bandwidth for KAGRA
Downselection of observation bandwidth for KAGRA MG13, Stockholm Jul. 2012 K.Somiya, K.Agatsuma, M.Ando, Y.Aso, K.Hayama, N.Kanda, K.Kuroda, H.Tagoshi, R.Takahashi, K.Yamamoto, and the KAGRA collaboration
More informationKAGRA Large-scale Cryogenic Gravitational wave Telescope Project in Japan
KAGRA Large-scale Cryogenic Gravitational wave Telescope Project in Japan KAGRA Collaborators ICRR, Univ. of Tokyo National Astronomical Observatory of Japan, High Energy Accelerator Research Organization,
More informationPossibility of Upgrading KAGRA
The 3 rd KAGRA International Workshop @ Academia Sinica May 22, 2017 Possibility of Upgrading KAGRA Yuta Michimura Department of Physics, University of Tokyo with much help from Kentaro Komori, Yutaro
More informationCommissioning of Advanced Virgo
Commissioning of Advanced Virgo VSR1 VSR4 VSR5/6/7? Bas Swinkels, European Gravitational Observatory on behalf of the Virgo Collaboration GWADW Takayama, 26/05/2014 B. Swinkels Adv. Virgo Commissioning
More informationCONTROLS CONSIDERATIONS FOR NEXT GENERATION GW DETECTORS
CONTROLS CONSIDERATIONS FOR NEXT GENERATION GW DETECTORS CONTROLS WORKSHOP GWADW 26 MAY 2016 AGENDA Introduction (
More informationISC RF Photodetector Design: LSC & WFS
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY LIGO Laboratory / LIGO Scientific Collaboration LIGO 7 August 2014 ISC RF Photodetector Design: LSC & WFS Rich Abbott, Rana Adhikari, Peter Fritschel.
More informationADVANCED VIRGO at the DAWN WORKSHOP
Giovanni Losurdo Advanced Virgo Project Leader for the Virgo Collaboration and EGO ADVANCED VIRGO at the DAWN WORKSHOP DAWN Workshop, May 8, 2015 G Losurdo - AdV Project Leader 1 ADVANCED VIRGO! Participated
More informationOptical lever for KAGRA
Optical lever for KAGRA Kazuhiro Agatsuma 2014/May/16 2014/May/16 GW monthly seminar at Tokyo 1 Contents Optical lever (OpLev) development for KAGRA What is the optical lever? Review of OpLev in TAMA-SAS
More informationStatus of GEO600. Harald Lück. for the GEO Team LIGO-G Z. GWADW May06, H. Lück
Status of GEO600 Harald Lück for the GEO Team LIGO-G060279-00-Z Tube / Trench Triple Pendulum + Reaction Pendulum GEO600 Optical Layout 53 W 0.09 2.3 74 kw 3 5 kw 10 6 W Tunable optical transfer function
More informationImproving seismic isolation in Advanced LIGO using a ground rotation sensor
Improving seismic isolation in Advanced LIGO using a ground rotation sensor 04/16/2016 Krishna Venkateswara for UW- Michael Ross, Charlie Hagedorn, and Jens Gundlach aligo SEI team LIGO-G1600083 1 Contents
More informationDigital Communications over Fading Channel s
over Fading Channel s Instructor: Prof. Dr. Noor M Khan Department of Electronic Engineering, Muhammad Ali Jinnah University, Islamabad Campus, Islamabad, PAKISTAN Ph: +9 (51) 111-878787, Ext. 19 (Office),
More informationIntroduction to laser interferometric gravitational wave telescope
Introduction to laser interferometric gravitational wave telescope KAGRA summer school 013 July 31, 013 Tokyo Inst of Technology Kentaro Somiya Interferometric GW detector Far Galaxy Supernova explosion,
More informationMuhammad Ali Jinnah University, Islamabad Campus, Pakistan. Fading Channel. Base Station
Fading Lecturer: Assoc. Prof. Dr. Noor M Khan Department of Electronic Engineering, Muhammad Ali Jinnah University, Islamabad Campus, Islamabad, PAKISTAN Ph: +9 (51) 111-878787, Ext. 19 (Office), 186 (ARWiC
More informationThe Virgo detector. L. Rolland LAPP-Annecy GraSPA summer school L. Rolland GraSPA2013 Annecy le Vieux
The Virgo detector The Virgo detector L. Rolland LAPP-Annecy GraSPA summer school 2013 1 Table of contents Principles Effect of GW on free fall masses Basic detection principle overview Are the Virgo mirrors
More informationReal-Time Spectrum Monitoring System Provides Superior Detection And Location Of Suspicious RF Traffic
Real-Time Spectrum Monitoring System Provides Superior Detection And Location Of Suspicious RF Traffic By Malcolm Levy, Vice President, Americas, CRFS Inc., California INTRODUCTION TO RF SPECTRUM MONITORING
More informationTHE FUTURE OF VIRGO BEYOND ADVANCED DETECTORS. Gianluca Gemme INFN Genova for the Virgo Collaboration
THE FUTURE OF VIRGO BEYOND ADVANCED DETECTORS Gianluca Gemme INFN Genova for the Virgo Collaboration GW150914 2 Post Newtonian formalism DEVIATION OF PN COEFFICIENTS FROM GR Phase of the inspiral waveform
More informationUnderstanding Initial LIGO and Possible Influences on Enhanced LIGO. Sam Waldman and Rai Weiss February 2008
Understanding Initial LIGO and Possible Influences on Enhanced LIGO Sam Waldman and Rai Weiss February 2008 Motivations Outline Improve understanding of initial LIGO, f < 200Hz Improve chance of detections
More informationInterferometer for LCGT 1st Korea Japan Workshop on Korea University Jan. 13, 2012 Seiji Kawamura (ICRR, Univ. of Tokyo)
Interferometer for LCGT 1st Korea Japan Workshop on LCGT @ Korea University Jan. 13, 2012 Seiji Kawamura (ICRR, Univ. of Tokyo) JGW G1200781 v01 Outline Resonant Sideband Extraction interferometer Length
More informationJGW-G ikagra calibration offline h(t) of ikagra
JGW-G1706731 ikagra calibration offline h(t) of ikagra Observation summary of ikagra ikagra observation 1st run: Mar. 25, 9:00(JST) - Mar. 31, 17:00(JST) GPS: 1142899217-1143446417 2nd run: Apr. 11, 9:00(JST)
More informationACOUSTIC MITIGATION POST-S3 UPDATE
ACOUSTIC MITIGATION POST-S3 UPDATE Robert Schofield, University of Oregon AND MANY OTHERS 1 REDUCTION IN ACOUSTIC COUPLING SINCE S2 Red: AS_Q normal; Black: AS_Q with noise; Yellow & Orange: BSC7 mic March
More informationParametric signal amplification
Parametric signal amplification ET meeting @ Birmingham Mar 27, 2017 K.Somiya Observation of high freq GW sources [Kiuchi, 2010] BNS merger with different models D=100Mpc BNS merger appears above the cavity
More informationKAGRA Actuator Noise Modeling Report
KAGRA Actuator Noise Modeling Report Yuta Michimura June 12, 2017 1 Introduction This report is to summarize the results of actuator noise modeling for the KA- GRA suspensions. The modeling was done by
More information5 Advanced Virgo: interferometer configuration
5 Advanced Virgo: interferometer configuration 5.1 Introduction This section describes the optical parameters and configuration of the AdV interferometer. The optical layout and the main parameters of
More informationCharacterization of High Q Spherical Resonators
Characterization of High Q Spherical Resonators Kenneth Bader, Jason Raymond, Joel Mobley University of Mississippi Felipe Gaitan, Ross Tessien, Robert Hiller Impulse Devices, Inc. Grass Valley, CA Physics
More informationReview of 40m upgrade goals ffl The primary goal of the 40 m upgrade is to demonstrate a scheme for using resonant sideband extraction (RSE), in eithe
40m Upgrade Plans ffl Review of 40m upgrade goals ffl 40m infrastructure upgrade ffl RSE configuration - design considerations ffl IFO optical configuration ffl RSE control scheme ffl people, money, schedule
More informationSystem Integration of the TPS. J.R. Chen NSRRC, Hsinchu
System Integration of the TPS J.R. Chen NSRRC, Hsinchu OUTLINE I. Main features of the TPS II. Major concerns and intersystem effects of an advanced synchrotron light source III. Subsystems and intersystem
More informationEmbedded Surface Mount Triaxial Accelerometer
Embedded Surface Mount Triaxial Accelerometer Robert D. Sill Senior Scientist PCB Piezotronics Inc. 951 Calle Negocio, Suite A San Clemente CA, 92673 (877) 679 0002 x2954 rsill@pcb.com Abstract 18566 59
More informationTexas Components - Data Sheet. The TX53G1 is an extremely rugged, low distortion, wide dynamic range sensor. suspending Fluid.
Texas Components - Data Sheet AN004 REV A 08/30/99 DESCRIPTION and CHARACTERISTICS of the TX53G1 HIGH PERFORMANCE GEOPHONE The TX53G1 is an extremely rugged, low distortion, wide dynamic range sensor.
More informationEHE Physics and ARIANNA
EHE Physics and ARIANNA http://arianna.ps.uci.edu Steve Barwick, UCI for the ARIANNA collaboration US Sweden New Zealand From OC Register 2012 Cosmogenic neutrino flux IC08-09 IC10-12(prel.) Proto ARIANNA
More informationChapter 2 Channel Equalization
Chapter 2 Channel Equalization 2.1 Introduction In wireless communication systems signal experiences distortion due to fading [17]. As signal propagates, it follows multiple paths between transmitter and
More informationMulti-Path Fading Channel
Instructor: Prof. Dr. Noor M. Khan Department of Electronic Engineering, Muhammad Ali Jinnah University, Islamabad Campus, Islamabad, PAKISTAN Ph: +9 (51) 111-878787, Ext. 19 (Office), 186 (Lab) Fax: +9
More informationEMI/EMC. GLAST Large Area Telescope. LAT Pre-Shipment Review. Gamma-ray Large Area Space Telescope. Neil Johnson NRL. Michael Lovellette NRL
GLAST Large Area Telescope Gamma-ray Large Area Space Telescope LAT Pre-Shipment Review EMI/EMC EMI/EMC 1 Neil Johnson NRL Michael Lovellette NRL Stanford Linear Accelerator Center Purpose / Contents Demonstrate
More informationStudy of the HD target spin rotations during G14
Study of the HD target spin rotations during G14 A. Deur, deurpam@jlab.org April 18, 2013 1 Introduction During the G14 run, the target spin was reversed using either magnetic field rotations or RF spin
More informationStable Recycling Cavities for Advanced LIGO
Stable Recycling Cavities for Advanced LIGO Guido Mueller University of Florida 08/16/2005 Table of Contents Stable vs. unstable recycling cavities Design of stable recycling cavity Design drivers Spot
More informationInertial Doppler Radio Locator (IDRL) for DoD Test Range Applications
INNOVATIONS IN ENGINEERING Inertial Doppler Radio Locator (IDRL) for DoD Test Range Applications This project is funded by the Test Resource Management Center (TRMC) Test and Evaluation/Science and Technology
More informationChannel. Muhammad Ali Jinnah University, Islamabad Campus, Pakistan. Multi-Path Fading. Dr. Noor M Khan EE, MAJU
Instructor: Prof. Dr. Noor M. Khan Department of Electronic Engineering, Muhammad Ali Jinnah University, Islamabad Campus, Islamabad, PAKISTAN Ph: +9 (51) 111-878787, Ext. 19 (Office), 186 (Lab) Fax: +9
More informationA DISCUSSION ON QAM SNARE SENSITIVITY
ADVANCED TECHNOLOGY A DISCUSSION ON QAM SNARE SENSITIVITY HOW PROCESSING GAIN DELIVERS BEST SENSITIVITY IN THE CATEGORY 185 AINSLEY DRIVE SYRACUSE, NY 13210 800.448.1655 / WWW.ARCOMDIGITAL.COM ADVANCED
More informationProgress on Burst Upper Limits simulation development. AJW, 4/3/01. Here s my overview of the task at hand:
Progress on Burst Upper Limits simulation development. AJW, 4/3/1 Here s my overview of the task at hand: Milestones for the simulation subgroup: Exercise LDAS user application code / pipeline - Become
More informationPractical Use of the Accuraspray Plume Sensor
Practical Use of the Accuraspray Plume Sensor Sauer Engineering www.sauerengineering.com John P. Sauer jopsauer@fuse.net 513-290-3617 Accuraspray Usage in a Quick Summary Accuraspray must be considered
More informationLIGO seminar Jul. 20, 2015 Caltech, Pasadena, USA. Status of KAGRA. Seiji Kawamura (ICRR, UTokyo) JGW G v1
LIGO seminar Jul. 20, 2015 Caltech, Pasadena, USA Status of KAGRA JGW G1503846 v1 1 Seiji Kawamura (ICRR, UTokyo) Outline: Review of KAGRA Current status Schedule, Organization, Collaboration Summary 2
More informationMag Lev Train 1. By: Paul Friend. Project Advisor: Dr. Anakwa. Date:
Mag Lev Train 1 By: Paul Friend Project Advisor: Dr. Anakwa Date: October 28, 2003 The Mag Lev Train 1 project is to design and implement an active levitation, guidance, and propulsion system for a model
More informationVibration studies of a superconducting accelerating
Vibration studies of a superconducting accelerating module at room temperature and at 4.5 K Ramila Amirikas, Alessandro Bertolini, Wilhelm Bialowons Vibration studies on a Type III cryomodule at room temperature
More informationApplication of Non-Harmonic Analysis for Gravitational Wave Detection
Application of Non-Harmonic Analysis for Gravitational Wave Detection Masaya Nakano University of Toyama Collaborate with S. Hirobayashi(Univ. Toyama), H. Tagoshi(Osaka Univ.), K. Ueno(Osaka Univ.), T.
More informationPerformance Characterization of the Dual- Recycled Michelson Subsystem in Advanced LIGO
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 2014 Performance Characterization of the Dual- Recycled Michelson Subsystem in Advanced LIGO Anamaria Effler Louisiana
More informationApplication Note. Monitoring the Release of Radioactive Noble Gases Through the Stack of a Nuclear Power Plant (NPP): Stack Monitor System
Application Note Monitoring the Release of Radioactive Noble Gases Through the Stack of a Nuclear Power Plant (NPP): Stack Monitor System Based on the German KTA 1503.1 and respective international regulations,
More informationDevelopment of the accelerometer for cryogenic experiments II
Development of the accelerometer for cryogenic experiments II ICRR Univ. of Tokyo, KEK A, Dept. of advanced materials science Univ. of Tokyo B K. Yamamoto, H. Hayakawa, T. Uchiyama, S. Miyoki, H. Ishitsuka,
More informationA Courseware about Microwave Antenna Pattern
Forum for Electromagnetic Research Methods and Application Technologies (FERMAT) A Courseware about Microwave Antenna Pattern Shih-Cheng Lin, Chi-Wen Hsieh*, Yi-Ting Tzeng, Lin-Chuen Hsu, and Chih-Yu Cheng
More informationFLCS V2.1. AHRS, Autopilot, Gyro Stabilized Gimbals Control, Ground Control Station
AHRS, Autopilot, Gyro Stabilized Gimbals Control, Ground Control Station The platform provides a high performance basis for electromechanical system control. Originally designed for autonomous aerial vehicle
More informationStable recycling cavities for Advanced LIGO
Stable recycling cavities for Advanced LIGO Guido Mueller LIGO-G070691-00-D with input/material from Hiro Yamamoto, Bill Kells, David Ottaway, Muzammil Arain, Yi Pan, Peter Fritschel, and many others Stable
More informationPSL - Power Sensors Ltd
PSL - Power Sensors Ltd a Division of Power Standards > Founded in 2000 - Alameda CA, USA > Power Quality Experts - IEC standards > Manufacturer of leading Power Quality monitors We Capture All Bad Power
More informationStatus of the untriggered burst search in S3 LIGO data
Status of the untriggered burst search in S3 LIGO data Igor Yakushin (LIGO Livingston Observatory) For the LIGO Scientific Collaboration GWDAW-9, December 15-18, 2004, Annecy, France Overview Differences
More informationSqueezing with long (100 m scale) filter cavities
23-28 May 2016, Isola d Elba Squeezing with long (100 m scale) filter cavities Eleonora Capocasa, Matteo Barsuglia, Raffaele Flaminio APC - Université Paris Diderot Why using long filter cavities in enhanced
More informationACOUSTIC MITIGATION STATUS FOR S3
ACOUSTIC MITIGATION STATUS FOR S3 Robert Schofield, University of Oregon Doug Cook, Akiteru Takamori, Daniel Sigg, LHO Jonathan Kern, Joe Kovalik, LLO Peter Fritschel, Ken Mason, MIT AND MANY OTHERS PROBLEM
More informationProposed Vibration Measurement Program In A Parallel Tunnel
Proposed Vibration Measurement Program In A Parallel Tunnel 1 of 14- Fred Asiri Introduction Next Linear Collider U.S. Collaboration NLC Site Investigation Plan for Next Year Prepare an accurate and consistent
More informationMC-370CE - Soco Cold Saw, Includes Stand 100 x 100mm Rectangle Capacity Dual Speed 22 / 44rpm & Self Centring Vice & CE Approved Guarding
MC-370CE - Soco Cold Saw, Includes Stand 100 x 100mm Rectangle Capacity Dual Speed 22 / 44rpm & Self Centring Vice & CE Approved Guarding Ex GST Inc GST $5,590.00 $5,290.00 $6,149.00 $5,819.00 Special
More informationThe VIRGO detection system
LIGO-G050017-00-R Paolo La Penna European Gravitational Observatory INPUT R =35 R=0.9 curv =35 0m 95 MOD CLEAN ER (14m )) WI N d:yag plar=0 ne.8 =1λ 064nm 3km 20W 6m 66.4m M odulat or PR BS N I sing lefrequ
More informationStretched Wire Test Setup 1)
LCLS-TN-05-7 First Measurements and Results With a Stretched Wire Test Setup 1) Franz Peters, Georg Gassner, Robert Ruland February 2005 SLAC Abstract A stretched wire test setup 2) has been implemented
More informationBeamforming for IPS and Pulsar Observations
Beamforming for IPS and Pulsar Observations Divya Oberoi MIT Haystack Observatory Sunrise at Mileura P. Walsh Function, Inputs and Outputs Function - combine the voltage signal from each of the 512 tiles
More informationLASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY -LIGO- CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSSETTS INSTITUTE OF TECHNOLOGY
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY -LIGO- CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSSETTS INSTITUTE OF TECHNOLOGY Technical Note LIGO-T38- - Z 3/2/ E2 Correlations Nelson Christensen,
More informationLIGO. Advanced LIGO. Keita KAWABE, LIGO Hanford, Caltech LIGO-G
Advanced Keita KAWABE, Hanford, Caltech Introduction Current status Future TOC Why a What is a Introduction Why a: i was not that bad S6 (peak, average) NSNS ~(21, 16) Mpc (H1) and ~(20, 14) Mpc (L1),
More informationResilient and Accurate Autonomous Vehicle Navigation via Signals of Opportunity
Resilient and Accurate Autonomous Vehicle Navigation via Signals of Opportunity Zak M. Kassas Autonomous Systems Perception, Intelligence, and Navigation (ASPIN) Laboratory University of California, Riverside
More informationDRAFT Expected performance of type-bp SAS in bkagra
DRAFT Expected performance of type-bp SAS in bkagra December 27, 216 Yoshinori Fujii Table of Contents 1 Expected performance of type-bp SAS in bkagra 2 1.1 Overview.................................................
More informationHow to Build a Gravitational Wave Detector. Sean Leavey
How to Build a Gravitational Wave Detector Sean Leavey Supervisors: Dr Stefan Hild and Prof Ken Strain Institute for Gravitational Research, University of Glasgow 6th May 2015 Gravitational Wave Interferometry
More informationSignal segmentation and waveform characterization. Biosignal processing, S Autumn 2012
Signal segmentation and waveform characterization Biosignal processing, 5173S Autumn 01 Short-time analysis of signals Signal statistics may vary in time: nonstationary how to compute signal characterizations?
More informationSIGNAL DETECTION IN NON-GAUSSIAN NOISE BY A KURTOSIS-BASED PROBABILITY DENSITY FUNCTION MODEL
SIGNAL DETECTION IN NON-GAUSSIAN NOISE BY A KURTOSIS-BASED PROBABILITY DENSITY FUNCTION MODEL A. Tesei, and C.S. Regazzoni Department of Biophysical and Electronic Engineering (DIBE), University of Genoa
More informationServo Drives SPECIFICATIONS Model DA-XDA DA-XDA DA-XDA Continuous Current 4 A peak / 2.8 A RMS 8 A peak / 5.6 A RMS 16 A peak
Allied Motion s new xdrive servo drives are precision, all-digital DSPbased servo drive amplifiers capable of supplying up to 16 A peak continuous, 32 A peak current at up to 230 VAC. The xdrive is designed
More informationActivities in the Homestake mine
Activities in the Homestake mine 07-20-2008/09-19-2008 LIGO-G080475-00-R Angelo Sajeva Jan Harms Riccardo De Salvo Vuk Mandic The three minesketeers! and D Artagnan Jan Riccardo Angelo Vuk Who? Jan Harms,
More informationPrecision RF Beam Position Monitors for Measuring Beam Position and Tilt Progress Report
Precision RF Beam Position Monitors for Measuring Beam Position and Tilt Progress Report UC Berkeley Senior Personnel Yury G. Kolomensky Collaborating Institutions Stanford Linear Accelerator Center: Marc
More informationVirgo status and commissioning results
Virgo status and commissioning results L. Di Fiore for the Virgo Collaboration 5th LISA Symposium 13 july 2004 VIRGO is an French-Italian collaboration for Gravitational Wave research with a 3 km long
More informationD1.17B VDES Channel Model - Review of VDES terrestrial test results Recent Updates and Work In Progress
D1.17B VDES Channel Model - Review of VDES terrestrial test results Recent Updates and Work In Progress Arunas Macikunas 1, Jan Šafář 2, Ronald Raulefs 3, Wei Wang 3 1 Waves in Space Corp., Canada 2 General
More informationAdvanced LIGO optical configuration investigated in 40meter prototype
Advanced LIGO optical configuration investigated in 4meter prototype LSC meeting at LLO Mar. 22, 25 O. Miyakawa, Caltech and the 4m collaboration LIGO- G5195--R LSC meeting at LLO, March 25 1 Caltech 4
More informationionospheric satellite cluster scientific premises and proposed configuration
ionospheric satellite cluster scientific premises and proposed configuration O. Fedorov, Institute of Space Research, Kyiv, Ukraine V. Korepanov, Lviv Centre of Institute of Space Research, Lviv, Ukraine
More informationPolarisation properties of [SQUID] 2 horizontal components at the LSBB (Laboratoire Souterrain à Bas Bruit)
Polarisation properties of [SQUID] 2 horizontal components at the LSBB (Laboratoire Souterrain à Bas Bruit) Christian Kwisanga a Department of Physics, College of Science and Technology, University of
More informationExperiment on signal filter combinations for the analysis of information from inertial measurement units in AOCS
Journal of Physics: Conference Series PAPER OPEN ACCESS Experiment on signal filter combinations for the analysis of information from inertial measurement units in AOCS To cite this article: Maurício N
More informationUnit 5 - Week 4 - Multipath Fading Environment
2/29/207 Introduction to ireless and Cellular Communications - - Unit 5 - eek 4 - Multipath Fading Environment X Courses Unit 5 - eek 4 - Multipath Fading Environment Course outline How to access the portal
More informationMeasuring Noise; Low Noise Model
Noise in data Specifying noise Measuring noise How to quantify seismic noise Karlsruhe Institute of Technology (KIT) Black Forest Observatory (BFO) September 2011 Noise in data Specifying noise Measuring
More informationMETEOROLOGICAL INSTRUMENTS
METEOROLOGICAL INSTRUMENTS INSTRUCTIONS ELECTRONIC COMPASS W/ SERIAL INTERFACE MODEL 32500 R.M. YOUNG COMPANY 2801 AERO PARK DRIVE, TRAVERSE CITY, MICHIGAN 49686, USA TEL: (231) 946-3980 FAX: (231) 946-4772
More informationECE 695 Numerical Simulations Lecture 28: Finite-Difference Time Domain in MEEP. Prof. Peter Bermel March 27, 2017
ECE 695 Numerical Simulations Lecture 28: Finite-Difference Time Domain in MEEP Prof. Peter Bermel March 27, 2017 Recap: Special Features of MEEP jdj.mit.edu/meep nanohub.org/tools/meep Arbitrary dimensionality,
More informationEMC review for Belle II (Grounding & shielding plans) PXD DEPFET system
EMC review for Belle II (Grounding & shielding plans) PXD DEPFET system Outline 1. Introduction 2. Grounding strategy Implementation aspects 3. Noise emission issues Test plans 4. Noise immunity issues
More informationThe Signature VM package delivers vessel-mounted AD2CP capabilities based on present-day technology
The package delivers vessel-mounted AD2CP capabilities based on present-day technology Until now, ADCP current surveys have been complex and time-consuming processes. A successful current survey depends
More informationKey-Words: - Fuzzy Behaviour Controls, Multiple Target Tracking, Obstacle Avoidance, Ultrasonic Range Finders
Fuzzy Behaviour Based Navigation of a Mobile Robot for Tracking Multiple Targets in an Unstructured Environment NASIR RAHMAN, ALI RAZA JAFRI, M. USMAN KEERIO School of Mechatronics Engineering Beijing
More informationThe X-arm interferometer test of HEPI at LIGO Livingston
The X-arm interferometer test of HEPI at LIGO Livingston J. Giaime, Louisiana State University & LIGO Livingston. 1 G040358-00-D, LSC meeting, LIGO Hanford, 18 August 2004. Development history Decades
More informationA LARGE COMBINATION HORIZONTAL AND VERTICAL NEAR FIELD MEASUREMENT FACILITY FOR SATELLITE ANTENNA CHARACTERIZATION
A LARGE COMBINATION HORIZONTAL AND VERTICAL NEAR FIELD MEASUREMENT FACILITY FOR SATELLITE ANTENNA CHARACTERIZATION John Demas Nearfield Systems Inc. 1330 E. 223rd Street Bldg. 524 Carson, CA 90745 USA
More informationExperimentswithaunSQUIDbasedintegrated magnetometer.
ExperimentswithaunSQUIDbasedintegrated magnetometer. Heikki Seppä, Mikko Kiviranta and Vesa Virkki, VTT Automation, Measurement Technology, P.O. Box 1304, 02044 VTT, Finland Leif Grönberg, Jaakko Salonen,
More informationEconomic Solutions for Spectrum Monitoring. 2 MAR Re 08/00 1
Economic Solutions for Spectrum Monitoring 2 MAR Re 08/00 1 Everybody needs to communicate 8SPM/Kr 06-2004 2 8SPM/Kr 06-2004 3 Secure and reliable communication is essential for modern society But! The
More informationGeneral Specifications
General Specifications FN510 Field Wireless Multi-Function Module GENERAL This General Specification (GS) describes the specifications for Field Wireless Multi-Function Module. Combined with Field Wireless
More informationGROUND MOTION IN THE INTERACTION. ensured that the final focus quadrupoles on both. rms amplitudes higher than some fraction of the
GROUND MOTION IN THE INTERACTION REGION C.Montag, DESY Abstract Ground motion and according quadrupole vibration is of great importance for all Linear Collider schemes currently under study, since these
More informationIntelligent Monitoring Analysis System
Wireless RH503 & RH550 Software MOS2000 Intelligent Monitoring Analysis System Remark: RH503 is the updated version of RH501 1. Product Introduction RH503 wireless transducer and RH550 wireless communication
More informationAdvanced Digital Motion Control Using SERCOS-based Torque Drives
Advanced Digital Motion Using SERCOS-based Torque Drives Ying-Yu Tzou, Andes Yang, Cheng-Chang Hsieh, and Po-Ching Chen Power Electronics & Motion Lab. Dept. of Electrical and Engineering National Chiao
More informationDiamond sensors as beam conditions monitors in CMS and LHC
Diamond sensors as beam conditions monitors in CMS and LHC Maria Hempel DESY Zeuthen & BTU Cottbus on behalf of the BRM-CMS and CMS-DESY groups GSI Darmstadt, 11th - 13th December 2011 Outline 1. Description
More informationVIRGO. The status of VIRGO. & INFN - Sezione di Roma 1. 1 / 6/ 2004 Fulvio Ricci
The status of VIRGO Fulvio Ricci Dipartimento di Fisica - Università di Roma La Sapienza & INFN - Sezione di Roma 1 The geometrical effect of Gravitational Waves The signal the metric tensor perturbation
More informationAdvanced Virgo Technical Design Report
Advanced Virgo Technical Design Report VIR xxxa 12 Issue 1 The Virgo Collaboration March 21, 2012 Contents 1 ISC 1 1.1 General description of the sub-system........................ 1 1.2 Input from other
More informationIntegrated Navigation System
Integrated Navigation System Adhika Lie adhika@aem.umn.edu AEM 5333: Design, Build, Model, Simulate, Test and Fly Small Uninhabited Aerial Vehicles Feb 14, 2013 1 Navigation System Where am I? Position,
More informationEL6483: Sensors and Actuators
EL6483: Sensors and Actuators EL6483 Spring 2016 EL6483 EL6483: Sensors and Actuators Spring 2016 1 / 15 Sensors Sensors measure signals from the external environment. Various types of sensors Variety
More informationExternal seismic pre-isolation retrofit design
External seismic pre-isolation retrofit design J. Giaime, B. Lantz, C. Hardham, R. Adhikari, E. Daw, D. DeBra, M. Hammond, K. Mason, D. Coyne, D. Shoemaker April 3, 2002 T020040-00-D Contents 1 Introduction
More informationSTPA FOR LINAC4 AVAILABILITY REQUIREMENTS. A. Apollonio, R. Schmidt 4 th European STAMP Workshop, Zurich, 2016
STPA FOR LINAC4 AVAILABILITY REQUIREMENTS A. Apollonio, R. Schmidt 4 th European STAMP Workshop, Zurich, 2016 LHC colliding particle beams at very high energy 26.8 km Circumference LHC Accelerator (100
More informationMulti-Function Fuze Capability Against High Speed Mobile Water Attack Craft
Multi-Function Fuze Capability Against High Speed Mobile Water Attack Craft 55th Annual NDIA Fuze Conference Presenter: James Ring ATK Propulsion & Controls 1 Presentation Agenda Functional Overview Design
More informationHow to introduce LORD Sensing s newest inertial sensors into your application
LORD TECHNICAL NOTE Migrating from the 3DM-GX4 to the 3DM-GX5 How to introduce LORD Sensing s newest inertial sensors into your application Introduction The 3DM-GX5 is the latest generation of the very
More informationINTERFEROMETRIC SENSING AND CONTROL
INTERFEROMETRIC SENSING AND CONTROL IN LIGO Nergis Mavalvala October 1998 Introduction to control systems Length and alignment sensing Noise Sensitivity Length control system Noise suppression More tricks?
More information