1|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements NAOJ GW Meeting, May 8 th,

Slides:



Advertisements
Similar presentations
Chapter 29 Magnetic Fields.
Advertisements

Gravitational Wave Astronomy Dr. Giles Hammond Institute for Gravitational Research SUPA, University of Glasgow Universität Jena, August 2010.
Global longitudinal quad damping vs. local damping G v8 1.
Participants: C-1:Cryogenic last-stage suspensions (interferometers) (F.Ricci-G.Frossati) Objectives: -Design new suspension elements for the last stage.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.
Global longitudinal quad damping vs. local damping Brett Shapiro Stanford University 1/32G v13 LIGO.
One Arm Cavity M0 L1 L2 TM M0 L1 L2 TRIPLE QUAD 16m R = 20m, T=1% R = ∞, T=1%  Optimally coupled cavity (no mode matched light reflected back)  Finesse.
Takanori Sekiguchi Italy-Japan Workshop (19 April, 2013) Inverted Pendulum Control for KAGRA Seismic Attenuation System 1 D2, Institute for Cosmic Ray.
LIGO-G D Suspensions Update: the View from Caltech Phil Willems LIGO/Caltech Livingston LSC Meeting March 17-20, 2003.
Pore Detection in Small Diameter Bores The University of Michigan, Ann Arbor NSF Engineering Research Center for Reconfigurable Manufacturing Systems.
Nature of light Ray or geometrical optics Wave or physical optics Quantum theory: W p =hf.
40m Suspension Electronics Benjamin Abbott California Institute of Technology 10/18/01 G R.
M. Ellis - 11th February 2004 Sci Fi Cosmic Light Yield 2 views 3 views.
MERIT Primary Containment Inspection – HandySurf Review Van Graves MERIT Video Conference November 24, 2010.
Use ofSiesta in VIRGO commissioning Lisa Barsotti University of Pisa – INFN Pisa For the Virgo collaboration Caltech, December 19th 2003.
Definition: A circle is the set of all points on a plane that is a fixed distance from the center.
Vibration Isolation R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR), H. Ishizaki (NAOJ), A. Takamori (ERI), R. DeSalvo.
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
1 Ist Virgo+ review Cascina H. Heitmann Alignment: Virgo+ changes.
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.
Interferometer Control Matt Evans …talk mostly taken from…
Takanori Sekiguchi ALPS Report, Dec. 26th, 2013 Prototype Test of Type-B 1 Takanori Sekiguchi KAGRA F2F MEETING Feb
May Chuck DiMarzio, Northeastern University ECE-1466 Modern Optics Course Notes Part 7 Prof. Charles A. DiMarzio Northeastern University.
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.
Cavity Work at LASTI LSC-VIRGO Meeting, Hannover - 24 th October 2007 Lisa Barsotti and Matthew Evans for the LASTI group G D.
The Hong Kong Polytechnic University Optics 2----by Dr.H.Huang, Department of Applied Physics1 Diffraction Introduction: Diffraction is often distinguished.
Global longitudinal quad damping vs. local damping Brett Shapiro Stanford University 1/36 LIGO G v15.
Laser-Based Finger Tracking System Suitable for MOEMS Integration Stéphane Perrin, Alvaro Cassinelli and Masatoshi Ishikawa Ishikawa Hashimoto Laboratory.
LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.
G D Commissioning Progress and Plans Hanford Observatory LSC Meeting, March 21, 2005 Stefan Ballmer.
March 2004 Charles A. DiMarzio, Northeastern University ECEG287 Optical Detection Course Notes Part 15: Introduction to Array Detectors Profs.
Optical Part of the CMB for AHCAL-CALICE Jaroslav Zalesak Institute of Physics, Prague.
Abstract The Hannover Thermal Noise Experiment V. Leonhardt, L. Ribichini, H. Lück and K. Danzmann Max-Planck- Institut für Gravitationsphysik We measure.
On behalf of joint ITEP / IHEP team: A. Arefiev, N. Filimonov, T. Kvaratskheliya, I. Machikhiliyan, P. Shatalov, T. Zakoryuchkina, A. Zhokhov, S. Zvyagintsev.
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.
Calibration in the Front End Controls Craig Cahillane LIGO Caltech SURF 2013 Mentors: Alan Weinstein, Jamie Rollins Presentation to Calibration Group 8/21/2013.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
Linearity Tests The laser induced high noise pulses on the APD rendering it useless. We tried several methods to shield and filter the noise. With a stabilized.
Low frequency anti-vibration system of LCGT Vibration Isolation Group R. Takahashi (ICRR), K. Yamamoto (ICRR), T. Uchiyama (ICRR), T. Sekiguchi (ICRR),
Speed Sensor Calibration
Two Layers SAS: Damping of Torsion Mode Feb. 5th, 2011 F2F Meeting Takanori Sekiguchi, Riccardo DeSalvo, Ryutaro Takahashi 1/8.
Caltech, February 12th1 Virgo central interferometer: commissioning and engineering runs Matteo Barsuglia Laboratoire de l’Accelerateur Lineaire, Orsay.
Advanced LIGO UK 1 LIGO-G K OSEM Development UK Advanced LIGO project Stuart Aston University of Birmingham for the UK Advanced LIGO Team LSC.
Space Gravitational Wave Antenna DECIGO Project 3rd TAMA Symposium February 7, Institute for Cosmic Ray Research, Japan Seiji Kawamura National.
NLC - The Next Linear Collider Project Keeping Nanometer Beams Colliding Vibration Stabilization of the Final Doublet Tom Himel SLAC NLC MAC review October.
The VIRGO detection system
1|8J.V. van Heijningen Reasons for these measurements Intensity noise measurementAngular distribution measurement NAOJ VIS Meeting,
Mobile Microscopy Group #33 Rui Guo, Yongli Chen, Xiaoyu Qin.
Roller Coaster Speed Sensor Calibration. Lab Safety  Do not stand on chairs, or sit or stand on the tables  Know the location of the first-aid kit 
Development of a pellet tracking system for PANDA and WASA Goal:  know interaction point with a few 100  m accuracy in 3d(xyz). Method: Track pellets.
Local control sensors for iKAGRA payloads and perspective (Optical lever) Kazuhiro Agatsuma 2013/Dec./5 ELiTES meeting at Tokyo1.
Studying the use of masses on the microwaves cables to isolate seismic noise in the Schenberg Detector. Carlos Frajuca Fábio da Silva Bortoli São Paulo.
Digital Light Sources First introduced in 2001.
Type-A SAS Local Control Simulation (Current Status)
LV Meeting – 22 September 2009 Brett Shapiro G v1
From: A fast high-voltage switching multiwire proportional chamber
IMAGE ORTHICON.
Commissioning Update PAC 15, Dec. 11, 2003 Daniel Sigg.
Speed Sensor Calibration
The Superattenuator upgrades and the SAFE Project
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
Complex Metabolic Oscillations in Plants Forced by Harmonic Irradiance
Improving LIGO’s stability and sensitivity: commissioning examples
PURE Mid-Semester Report
Talk prepared by Stefan Hild AEI Hannover for the GEO-team
Spot-Projector System for the Measurement of Intra-Pixel Response
Presentation transcript:

1|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements NAOJ GW Meeting, May 8 th, 2014

2|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements 10 cables from bottom filters to OSEMs

3|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements Wire lengths and masses are wrong!

4|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements Measurement set-up intensity noise Determined with the first (!) fully assembled OSEM what current to run the LED, now with collimator, to have -12V on U TIA output: R s,LED = 300  U LED = 8V I LED ≈ 25mA For fast comparative measurement, LED is run in a simple set-up at 25 mA and ASD on the U TIA signal is taken First, a dependence of intensity noise on the LED intensity magnitude is investigated

5|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements Intensity noise first batch of LEDs RMS determined by f df from 1-40 Hz

6|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements Measurement set-up angular distribution OSEM optics LED Lens (f = 8mm) CCD Camera 1 DoF TrSt with end-stop

7|8J.V. van Heijningen Cables finished! Assemble/ Disassemble Type B Payload LED selection measurements Determining the optimal lens position Image analysis code: Determine maximum and a radius in which every value is 95% or higher of this value Middle of this circle is the defined as the middle of the blob Square with edges equal to the radius (half the diameter) to determine the fall of intensity with respect to the ‘0mm’ image When lens is at optimal position, radius shouldn’t change and power shouldn’t fall (as)much

8|8J.V. van Heijningen Assemble/ Disassemble Type B Payload LED selection measurementsNext weeks’ plan In my last weeks here, I’d like to… I’ll be at NAOJ until May 23, so 2 weeks to go… Select the 10 LEDs that will provide low(est) noise, most linear read-out for the OSEMs in their ‘new’ set-up (with collimator lens) Calibrate 10 OSEMs using the calibration stage (last part received last week!) Attach OSEMs to full type B payload prototype in their individual regions of highest sensitivity and linearity Use these 10 OSEMs in a feedback loop to damp the resonant modes of the Test Mass stage (3 DoFs) and Intermediate Mass stage (6 DoFs)