Simulink/Front Model & MEDM Screen Mods from ECR E1300578 (For SUS’ in BSC Chambers) J. Kissel for the SUS and ISC Team G1301192-v3 1.

Slides:



Advertisements
Similar presentations
Global longitudinal quad damping vs. local damping G v8 1.
Advertisements

8/13/2004 Stefan Ballmer, MIT / LIGO Hanford 1 Length and angular control loops in LIGO Stefan Ballmer Massachusetts Institute of Technology LIGO Hanford.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Global longitudinal quad damping vs. local damping Brett Shapiro Stanford University 1/32G v13 LIGO.
Bits and Bytes + Controlling 8 LED with 3 Pins Binary Counting and Shift Registers.
QUAD Testing Outline, Phase 2B Fiber Lower “half” Build-up and Testing M. Barton, B. Bland, D. Cook, J. Kissel, N. Robertson, J. Romie, T. Sadecki, for.
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.
1 Virgo commissioning status M.Barsuglia LAL Orsay.
Initial Work on Suspension Diagonalisation – August 2004 Bryan W Barr.
E2E school at LLO1  Han2k »Model of the LHO 2k IFO »Designed for lock acquisition study  SimLIGO1 »Model of all LIGO 1 IFOs »Designed for –noise hunting.
Suspended Mirror control: Learning through Virgo Experience E. Majorana - I.N.F.N. Pisa Aspen GWAD February 16, 2004.
LIGO-G W Commissioning Data on Vibration Isolation & Suspensions Fred Raab 24 October 02.
Ilya Berdnikov, Cornell University. Characterization of the LIGO 40m Lab Mode Cleaner Digital Suspensions Summer Project by Ilya Berdnikov Mentors:
Use ofSiesta in VIRGO commissioning Lisa Barsotti University of Pisa – INFN Pisa For the Virgo collaboration Caltech, December 19th 2003.
Suspension Control with Thoughts on Modern Control Brett Shapiro 19 May May GWADW- G – v3.
Making LIGO wind-resistant Krishna Venkateswara Borrowing from J. Kissel, B. Lantz, L. Barsotti, S. Dwyer, R. Schofield, D. Talukder, G. Vajente, M. Vidrio,
LIGO-G Z1 E2e modeling of violin mode S. Yoshida Southeastern Louisiana University V. Sannibale M. Barton, and H. Yamamoto Caltech LIGO NSF: PHYS
Towards aLIGO Heirarchical Control Scheme J. Kissel G v31.
11 A First Game Program Session Session Overview  Begin the creation of an arcade game  Learn software design techniques that apply to any form.
Prototype Test of Vibration Isolation System Current Status & Schedule
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
Ideal Order of QUAD Testing J. Kissel, S. Aston for the SUS Team G v5 01/18/13 1G v5.
Takanori Sekiguchi External Review Alignment control servo for type-B/type-Bp (OpLev/WFS) 1 T. Sekiguchi.
04. November 2004 A. Freise A. Freise, M. Loupias Collaboration Meeting November 04, 2004 Alignment Status.
Takanori Sekiguchi External Review Control and tuning of suspension 1 T. Sekiguchi KAGRA 4th External Review.
The purpose of the change of basis matrices is to combine local instruments to sense (or drive ) the platforms rigid body motions along the axis of the.
System Identification for LIGO Seismic Isolation Brett Shapiro GWADW – 19 May G v1.
G D LSC Changes in Preparation of High Power Operations Commissioning Meeting, May 5, 2003 Peter Fritschel, Daniel Sigg, Matt Evans.
Cavity Work at LASTI LSC-VIRGO Meeting, Hannover - 24 th October 2007 Lisa Barsotti and Matthew Evans for the LASTI group G D.
LIGO-G D Commissioning, Part II PAC 12, June 2002 Peter Fritschel, LIGO MIT.
Global longitudinal quad damping vs. local damping Brett Shapiro Stanford University 1/36 LIGO G v15.
LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.
MSC - 18 Oct 071 LOW FREQUENCY SEISMIC NOISE: LOCKING AND SENSITIVITY ISSUE Paolo Ruggi noise meeting.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
The ATF Damping Ring BPM Upgrade Nathan Eddy, Eliana Gianfelice-Wendt Fermilab for the ATF Damping Ring BPM Team.
LIGO-G D 1 Status of Detector Commissioning LSC Meeting, March 2001 Nergis Mavalvala California Institute of Technology.
Laser Frequency Stabilization – 2004, May 04 1 Laser Frequency Stabilization François BONDU CNRS – ARTEMIS, Nice VIRGO How it works (Design) Make it work.
Modeling of the Effects of Beam Fluctuations from LIGO’s Input Optics Nafis Jamal Shivanand Sanichiro Yoshida Biplab Bhawal LSC Conference Aug ’05 LIGO-G Z.
The VIRGO Suspensions Control System Alberto Gennai The VIRGO Collaboration.
The control of the Virgo Superattenuator: present and future Giovanni Losurdo - INFN Firenze/Urbino on behalf of the Virgo Collaboration.
LSC Meeting at LHO LIGO-G E 1August. 21, 2002 SimLIGO : A New LIGO Simulation Package 1. e2e : overview 2. SimLIGO 3. software, documentations.
Microsoft Project 2010 ® Tutorial 4: Assigning Resources and Costs.
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.
Elba Gravitational Wave Adv. Detector Workshop1May 22, 2002 Simulation of LIGO Interferometers 1. End to End simulation 2. Lock acquisition 3. Noise.
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.
Filter #7 control April 18, 2016 –, Cascina Paolo Ruggi.
Automation of the Lock Acquisition of the 3 km Arm Virgo Interferometer F. Carbognani for The Virgo Collaboration ICALEPCS - Geneva 14 October, 2005.
Thoughts on an SPI for AdLIGO SPI: Suspension Point Interferometer, or Seismic Platform Interferometer with Rana Adhikari and Matt Evans.
S5 Data Quality John Zweizig LIGO/Caltech Hanover, October 25, 2007.
ALIGO HSTS Damping Loops Design Comparison J. Kissel, for the SUS and ISC Teams.
ALIGO QUAD "Level 2" Damping Loop Design (Supplemental to LLO aLOG 6949)LLO aLOG 6949 J. Kissel G v21.
Time domain simulation for a FP cavity with AdLIGO parameters on E2E
ALIGO BSFM “Level 2” Damping Loop Design (Supplemental to LHO aLOG 6392) J. Kissel G v1.
Control State Definition
Type-A SAS Local Control Simulation (Current Status)
Digital readout architecture for Velopix
Clocks A clock is a free-running signal with a cycle time.
VIRGO–KAGRA Meeting about bottom filter damping
Time domain simulation for a FP cavity with AdLIGO parameters on E2E
O2 DARM Loop Design Comparisons and Critiques
First Lessons from the Advanced LIGO Integration Testing
A Proposed Capacitive Position Sensor Timing Synchronization and Distribution Solution Ben Abbott May 9, 2014 G v1.
Lecture 25 More Synchronized Data and Producer/Consumer Relationship
Features in the Quad State Space Model
O1 DARM Loop Design Comparisons and Critiques
The Advanced LIGO Angular Control System (ASC) (Hanford edition)
Alignment Investigations towards Advanced Virgo
Presentation transcript:

Simulink/Front Model & MEDM Screen Mods from ECR E (For SUS’ in BSC Chambers) J. Kissel for the SUS and ISC Team G v3 1

Added SVN $Id$ String to All Parts G v3 2 Added to all top level models and library parts Great for visual assessment of version control Must be added to each top-level model (but comes for free with library parts) See instructions / description here:

Removal of ISI OFFLOAD G v3 3 A part of reducing wasted computation cycles Experience has shown that ISC offloading is only needed up to TOP mass of each suspension Affects top-level of models, so every model must be reconnected and IPCs senders removed SEI needs to get rid of their IPC receivers No longer anything here (for every suspension type)

G v3 4 Removal of ISI OFFLOAD Nothing up here any more, So you have to move up and reconnect everything

DRIVEALIGN Mods G v3 5 Move drive align to only affect ISC / “LOCK” Filters DRIVEALIGN designed to decouple L, P, and Y force and torque at each stage from L of the optic (the main chain on the QUAD), so it doesn’t make sense to include these filters in, say the damping path The means Move it up to only affect LOCK path at every stage Reduce the size of M0 M1 matrix from 6x6 to 3x3 Totally removed from R0 Only involves library parts => Comes for free with update

Added ODC Bits G v3 6 Added to all LOCK, DAMP, OLDAMP, etc (Actually ECR E )

G v3 7 Added ODC Bits State logic is now on every one of the DAMP, LOCK, OLDAMP filter screens Only includes filter modules in the state, no gains  Thought about doing this for OSEMINFs, but they need unique gain number for every OSEM, so not compatible with library parts

Added ODC Bits G v3 8 (Actually ECR E ) All bits get piped into new ODC V2 Block which is much cleaner QUADs have 13 bits, BSFMs have 10 bits, TMTSs have 5 bits, Etc. depending on how many stages of LOCKing and DAMPing Channel is now spit out to the top level to be collected by ODC master

G v3 9 Added ODC Bits (Actually ECR E ) IPC “channel” is $(IFO):SUS-$(OPTIC)_ODC_IPC (one per model) Affects top models!

Added switch after ISC (internal) OFFLOAD G v3 10 Added independent on/off switch between offload to upper stages and the DRIVEALIGN matrix This is so when we use “offloaded” (as opposed to “distributed”) hierarchy, we can pipe the ASC signals up to only the TOP mass, as opposed to LSC which needs to go to every stage

Divided up Commissioning vs. Science Frames G v3 11 Chose to store forever: One SUS/BSC-ISI’s worth of Calibrated Cartesian Basis in [nm / nrad] ($(IFO):SUS- $(OPTIC)_$(M0/M1)_ISIINF_$( DOF)_OUT_DQ) i.e. the QUADs and the BSFMs are in charge of storing this Every SUS’ Calibrated suspension point motion [nm / nrad] Only one version of OSEM / Oplev / ISC sensor signal at each stage – Euler basis, Calibrated into [um / urad] Only one version of control signal at each stage – OSEM basis, (uncalibrated) DAC counts

Removed QUAD lower stage damping G v3 12 No longer needed now that ISIs are commissioned Means $(IFO):SUS-$(OPTIC)_$(L1/L2)_DAMP_$(DOF)_IN1_DQ becomes $(IFO):SUS-$(OPTIC)_$(L1/L2)_WIT_$(DOF)_DQ

G v3 13 1) drive suspensions longitudinally and minimize the coupling to angle. Should we minimize coupling of M1_L to M1_A or M1_L to M3_A? The latter seems to make sense, but I haven't modeled what the effect will be for both cases. 2) balance the coil gains of all stages. here we want to use the logic of the old f2pRatio script written by Vuk/Matt which makes three measurements to find 3 of 4 coil gains (the remaining one is set to 1). The old way to do this was to use the OL for the readout. Naturally, we cannot do this for the M1/M2 stages anymore. And we can't use the OSEM readbacks at high frequency because of the pickup between the drive coil and the osem sensor. 3) Do a FD balance of P2Y and Y2P using something as the reference sensor. But what's the sensor? 4) Also, how do we do the A2L balancing for low frequencies (below the GW band)? For the GW band, we want to do this in the regular scalar way by just driving angle of each stage and minimizing the IFO readout. What's the harm in just punting on the f < 10 Hz FD part? 5) In cases where we don't have OL on the mirror we can use the WFS DC. In case #4, we want to use the LSC signal. Both require some communication between SUS/ISC. I don't want to add a bunch of IPC to handle this. Perhaps for the cases where we use WFS_DC to balance SUS we can utilize the ASC lockins. Not sure how to do #4. Added Optical Lever LOCK-IN

G v3 14 Added Optical Lever LOCK-IN Sent directly to coil basis, so we can do any configuration we want Sent to every stage One for PITCH, and one for YAW

G v3 15 Added Optical Lever LOCK-IN Sent directly to coil basis, so we can do any configuration we want Uses ISC library part Needs new $(SUBSYSTEM) and $(INSTANCE) variables in macro files

Added CD State and PUM WD to OVERVIEW G v3 16

Added CDS STATE Word and ODC Screen Link G v3 17 Shows the health of the CDS system (which is *not* on the GDS_TP screen!)

Accumulate Individual Overflows G v3 18 changes the overflow counters for each DAC and ADC channel to accumulate until the reset button is hit (as opposed to clearing once a second) So can find *which* channel saturated, as opposed to just finding that "there has been a saturation" from the overall counter on the GDS_TP screen. Affects top models!

Left to do Fix filter files Take new safe.snaps The HAM SUS. G v3 19