Status of GEO600. Harald Lück. for the GEO Team LIGO-G Z. GWADW May06, H. Lück
|
|
- Myron Dickerson
- 5 years ago
- Views:
Transcription
1 Status of GEO600 Harald Lück for the GEO Team LIGO-G Z
2
3 Tube / Trench
4 Triple Pendulum + Reaction Pendulum
5 GEO600 Optical Layout 53 W kw 3 5 kw 10 6 W
6 Tunable optical transfer function Signal Recycling provides an adjustable optical response (see talk by Stefan Hild) Lock acquistion at 2.5 khz, OPERATION NOW at 550 Hz.
7 Recent work on GEO600 Comissioning: improving detector sensitivity improving detector reliability improving detector characterization Joined S5 in overnight & weekend mode January 20th Joined S5 in 24/7 mode May 1st
8 Locking procedure (fully automated) PR error signal always available due to asymmetry in BS (~48/52) MI lock to dark fringe SR lock with three different signals in detuned state (~2kHz) Tuning to desired frequency (changing parameters in the process (see Stefans talk)) Switching MI lock to Single element diode Switching Servo parameters to lower noise & lower tolerance ones Ramping up power to final value In Total: ~ 3min
9 Calibration: Slides Courtesy Martin Hewitson
10
11
12
13
14 The Result Combining HP and HQ nfft/fs = 1.00 : navs = 200 : enbw = 1.50 : nsecs = G1:DER_DATA_H fs = : :25:00 - G1:DER_DATA_HP fs = : :25:00 - G1:DER_DATA_HQ fs = : :25:00 - Amplitude (Vrms / Hz 1/2 ) Frequency (Hz)
15
16 Sensitivity in Science Runs Typical Sensitivity: Science Runs S1 Aug 26 `02 S3I Nov 5 `03 S3II Dec 31 `03 S4 Feb 22 `05 S5 N&W Mar 23 `06 S5 24/7 May '06 ASD [h / Hz] Freq. [Hz]
17 Sensitivity in Science Runs Typical Sensitivity: Science Runs S1 Aug 26 `02 S3I Nov 5 `03 S3II Dec 31 `03 S4 Feb 22 `05 S5 N&W Mar 23 `06 S5 24/7 May '06 GEO Design 550Hz ASD [h / Hz] Freq. [Hz]
18 Sensitivity in Science Runs ASD [h / Hz] Typical Sensitivity: Science Runs S1 Aug 26 `02 S3I Nov 5 `03 S3II Dec 31 `03 S4 Feb 22 `05 S5 N&W Mar 23 `06 LHO4k Mar ' 06 LLO 4k Jan '06 LHO 2k Jan '06 GEO Design 550Hz S5 24/7 May ' x Freq. [Hz]
19 Displacement Sensitivity LHO 4k LHO 2k LLO 4k GEO Displacement ASD [m/sqrt(hz)] Frequency [Hz]
20 S5 Duty Cycle N&W + 24/7 (24/05/06) N&W 24/7 100 Total science time: 46.5 days, Overall Duty Cycle: 46.5 % Science duty cycle (%) Accumulated science time [days] Time from :59:47 ( ) [days]
21 Noise Projections ASD [h/ (Hz)] Projections to H for :05:00 Model Shot 550Hz Proj Dark PD+Mix Proj MI AA Rot Proj MI AA Tilt Proj MI Slow FB Proj SR FB Proj Dark Port PWR Proj MI Local Osc. Phase Proj EOM Osc. Amp Proj PR EP Proj Uncorrelated Sum h Theoretical Limit 550Hz See talk of Josh Smith Frequency [Hz]
22 Online Monitors: h(f) Current Current + last 12 hours
23 Online Monitors: Sensitivity Burst Sensitivity for Sine-Gaussians with Q=8.9 and an SNR of 8.0 for optimal orientation Sensitivity for inspiralling binary (NS-NS, NS-BH, BH-BH) systems
24 Online Monitors
25 Online Monitors: HACR burst-like events 2000 Time-frequency plot of events: h HACRMon (Total events =3192) Marker size corresponds to 20*log10(N pixels) pipeline: G1:DER_DATA_H_ _5.0_ Central frequency (Hz) Hours starting from UTC :32:15 1
26 Online Monitors: Spectra MIC + power signals, etc. Photon pressure Calibration MID OPN SR FP MID Signals Magnetic Seismic Online spectra + references to see at a glance whether every system behaves well Acoustic
27 ALARM! On Site Alarm KW 22 MO DI MI DO FR SA SO 29. Mai Mai Mai Jun Jun Jun Jun 06 00:00 NORBERT 01:00 02:00 03:00 04:00 MICHA MICHA MICHA MARC MARC 05:00 06:00 07:00 08:00 09:00 NORBERT MICHA 10:00 11:00 12:00 13:00 13:00 NORBERT NORBERT NORBERT NORBERT MICHA 14:00 15:00 16:00 17:00 18:00 MARC MARC MARC MICHA NORBERT 19:00 20:00 21:00 MICHA NORBERT 22:00 23:00 3 Operators hired, 2 shifts / working day (8:00-18:00)
28 SMS Alarm System
29 GEO Summary pages: monthly developments Inspiral H history BLRMS history HACR H history BurstSensMon history P params history Q params history # Report Tag Start Time (UTC) Start Time (GPS) Duration (s) Duration (H) Duty Cycle (%) 1 Wed_ :59: Tue_ :59: GREP_Tue_2_ _065946_ Tue_ :59: _28800 Lin k GREP_Wed_1_ _225946_ _28800 GREP_Tue_3_ _145946_ _28800
30 GEO Summary pages (reader/readonly) Segments of 8 hours: Sensitivity h(f) band-limited rms inspiral & burst sensitivity monitor HARC events (TF events), null-stream, coincidences with other detector channels (35 channels) Data Quality and Calibration Data quality, chi^2, DAQs timing offsets (alchemist), tuning parameters (P,Q) Detector Characterization lines, glitches, coincidences, saturation monitor
31 GEO summary pages (reader/readonly) Sensitivity H Spectrum HP Spectrum HQ Spectrum H Spectrogram BLRMS Inspiral Monitor burstsensmon H
32 Sensitivity for 8 h Shift secs from :59:46 ( ) ref from :58: min/max ref h best 175Hz at :01:06 Amplitude (RMS / Hz 1/2 ) each spectrum nsecs 10 navs 10 nfft fs ndata Frequency (Hz)
33 Sensitivity Monitors RMS Strain RMS Strain Time from ( :59:46) to ( :59:36) Step size of 10 secs H: Hz (mu= e-21 sigma= e-21) HP: Hz (mu= e-21 sigma= e-21) HQ: Hz (mu=2.0733e-21 sigma= e-21) InspiralSenseMon for G1:DER_DATA_H pipeline: G1:DER D ATA H burstsensmon 6 for G1:DER_DATA_H 7 pipeline: G1:DER_DATA_H_ _0.0_234.0_489.0_894.0_1234.0_1554.0_1893.0_0.0 x SG with Q=8.9, optimal SNR=8.0 Time from ( :59:46) to ( :59:36) 2.5 Step size of 10 secs 234 Hz H: Hz (mu= e-22 sigma= e-23) 589 Hz 894 Hz HP: Hz (mu= e-22 sigma= e-22) 1234 Hz 2 HQ: Hz (mu= e-22 sigma= e-23) 1554 Hz 1893 Hz Effective Distance (MPc) 1.5 h_rss BH-BH BH-NS NS-NS Hours starting from UTC :59: Hours starting from UTC :59:46
34 GEO summary pages Data Quality and Calibration Data quality chi^2 DAQs timing offsets (alchemist) P Params Q Params
35 GEO summary pages (Det. Char.) Glitch rate DER_DATA_H (HACR) Glitch rate DER_DATA_HNULL (HACR) Glitch rate DER_DATA_HP (HACR) Glitch rate DER_DATA_HQ (HACR) Further HACR timefrequency plots HACR coincident events hnull veto HACR Loudest events Saturation information
36 Events, Vetoes & Coincidences 2000 Time-frequency plot of events: h HACRMon (Total events =2966) Marker size corresponds to (N pixels) pipeline: G1:DER_DATA_H_ _5.0_ Central frequency (Hz) Frequency (Hz) Starttime: :59:46 ( ) Total number of h(t) events: 2966 Total number of hnull(t) events: 4229 Vetoed 544 out of 544 coincident events Using Twin = 0.040s and fwin = 32Hz Efficiency = Hours starting from UTC :59: h events hnull 3.5 events time/freq consistent Vetoed events Time (H)
37 Remaining Problems after comissioning The Owl a rapidly moving line with higher harmonics
38 Power up Glitches nfft/fs = 0.30 : navs = 120 : enbw = 5.00 : nsecs = 36 G1:LSC_MID_EP-P_HP : fs = : :19: Frequency (Hz) Time (s)
39 Dust (problem solved? See Josh s talk)
40 Prospect Stay in current state (owl permitting) until ~autumn and take data Continue detector characterization (Coincidences, Vetoes, ) ~autumn: maintenance period, try to find source of power-up glitches, owl, power loss
Comparison of tuned and detuned Signal-Recycling. Stefan Hild for the GEO-team
Comparison of tuned and detuned Signal-Recycling Stefan Hild for the GEO-team Stefan Hild 1 ILIAS WG1 meeting, Cascina, November 2006 Stefan Hild 2 ILIAS WG1 meeting, Cascina, November 2006 Signal-Recycling
More informationMystery noise in GEO600. Stefan Hild for the GEO600 team. 14th ILIAS WG1 meeting, October 2007, Hannover
Mystery noise in GEO600 Stefan Hild for the GEO600 team 14th ILIAS WG1 meeting, October 2007, Hannover Intro: What is mystery noise? There is a big gap between the uncorrelated sum (pink) of all known
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 informationExperience with Signal- Recycling in GEO600
Experience with Signal- Recycling in GEO600 Stefan Hild, AEI Hannover for the GEO-team Stefan Hild 1 GWADW, Elba, May 2006 Stefan Hild 2 GWADW, Elba, May 2006 Motivation GEO600 is the 1st large scale GW
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 informationM Hewitson, K Koetter, H Ward. May 20, 2003
A report on DAQ timing for GEO 6 M Hewitson, K Koetter, H Ward May, Introduction The following document describes tests done to try and validate the timing accuracy of GEO s DAQ system. Tests were done
More informationTiming accuracy of the GEO 600 data acquisition system
INSTITUTE OF PHYSICS PUBLISHING Class. Quantum Grav. 1 (4) S493 S5 CLASSICAL AND QUANTUM GRAVITY PII: S64-9381(4)6861-X Timing accuracy of the GEO 6 data acquisition system KKötter 1, M Hewitson and H
More informationStatus report : about the Monolithic Accelerometers(ACCs) Test
Updated on 2016.6.3 Goal 1 Estimate the sensitivity of the ACC on(and off) the IP, by comparing to L-4C geophone sensitivity, and 3 channel correlation analysis. Get the ACC s sensitivity limit at high
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 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 informationG5100A: 50 MHz Arbitrary Function Generator
G5100A: 50 MHz Arbitrary Function Generator Key Features 50 MHz Sine Wave 25 MHz Square Wave Pulse, Ramp, Triangle, Noise, and DC waveforms AM, FM, PM, FSK, and PWM modulation types Linear & logarithmic
More informationBeam Diagnostics, Low Level RF and Feedback for Room Temperature FELs. Josef Frisch Pohang, March 14, 2011
Beam Diagnostics, Low Level RF and Feedback for Room Temperature FELs Josef Frisch Pohang, March 14, 2011 Room Temperature / Superconducting Very different pulse structures RT: single bunch or short bursts
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 informationControl Servo Design for Inverted Pendulum
JGW-T1402132-v2 Jan. 14, 2014 Control Servo Design for Inverted Pendulum Takanori Sekiguchi 1. Introduction In order to acquire and keep the lock of the interferometer, RMS displacement or velocity of
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 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 informationModel MHz Arbitrary Waveform Generator Specifications
50MHz Arbitrary Waveform Generator s DISPLAY: Graph mode for visual verification of signal settings. CAPABILITY: Standard waveforms: Sine, Square, Ramp, Triangle, Pulse, Noise, DC Built-in arbitrary waveforms:
More informationArm Cavity Finesse for Advanced LIGO
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO - CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Technical Note LIGO-T070303-01-D Date: 2007/12/20 Arm Cavity Finesse
More informationReview of MPS Solid State Laser Systems
Review of MPS Solid State Laser Systems P.F. Moulton Q-Peak 135 South Road Bedford, MA 01730 LEOS 2006 Montreal, Canada November 2, 2006 Outline General design Specific systems Nd:YLF, 1047 and 1053 nm
More informationR. De Rosa INFN Napoli For the VIRGO collaboration
R. De Rosa INFN Napoli For the VIRGO collaboration The lesson of VIRGO+ and VIRGO Science Runs; The Technical Design Report of the Advanced VIRGO project; Conclusion. CSN2 - Frascati, 16-18 Aprile 2012
More informationHarvesting a Clock from a GSM Signal for the Wake-Up of a Wireless Sensor Network
Harvesting a Clock from a GSM Signal for the Wake-Up of a Wireless Sensor Network Jonathan K. Brown and David D. Wentzloff University of Michigan Ann Arbor, MI, USA ISCAS 2010 Acknowledgment: This material
More informationAnalog Arts SG985 SG884 SG834 SG814 Product Specifications [1]
www.analogarts.com Analog Arts SG985 SG884 SG834 SG814 Product Specifications [1] 1. These models include: an oscilloscope, a spectrum analyzer, a data recorder, a frequency & phase meter, and an arbitrary
More informationarxiv: v1 [gr-qc] 10 Sep 2007
LIGO P070067 A Z A novel concept for increasing the peak sensitivity of LIGO by detuning the arm cavities arxiv:0709.1488v1 [gr-qc] 10 Sep 2007 1. Introduction S. Hild 1 and A. Freise 2 1 Max-Planck-Institut
More informationMODEL AND MODEL PULSE/PATTERN GENERATORS
AS TEE MODEL 12010 AND MODEL 12020 PULSE/PATTERN GENERATORS Features: 1.6GHz or 800MHz Models Full Pulse and Pattern Generator Capabilities Programmable Patterns o User Defined o 16Mbit per channel o PRBS
More informationSCG2000 Series Synchronous Clock Generators
SCG2000 Series Synchronous Clock Generators PLL 2111 Comprehensive Drive Aurora, Illinois 60505 Phone: 630-851-4722 Fax: 630-851- 5040 www.conwin.com Bulletin SG035 Page 1 of 20 Revision 00 Date 23 AUG
More informationStructure of Speech. Physical acoustics Time-domain representation Frequency domain representation Sound shaping
Structure of Speech Physical acoustics Time-domain representation Frequency domain representation Sound shaping Speech acoustics Source-Filter Theory Speech Source characteristics Speech Filter characteristics
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 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 informationGoals of the Lab: Photodetectors and Noise (Part 2) Department of Physics. Slide 1. PHYSICS6770 Laboratory 4
Slide 1 Goals of the Lab: Understand the origin and properties of thermal noise Understand the origin and properties of optical shot noise In this lab, You will qualitatively and quantitatively determine
More informationThe Pre Stabilized Laser for the LIGO Caltech 40m Interferometer: Stability Controls and Characterization.
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY LIGO CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Document Type LIGO-T010159-00-R 10/15/01 The Pre Stabilized Laser for the
More informationToward the Advanced LIGO optical configuration investigated in 40meter prototype
Toward the Advanced LIGO optical configuration investigated in 4meter prototype Aspen winter conference Jan. 19, 25 O. Miyakawa, Caltech and the 4m collaboration LIGO- G547--R Aspen winter conference,
More informationExperiment begins this autumn. This Talk: Motivation for TAMA300 recycling Length sensing/control system Lock acquisition
Experiment begins this autumn. This Talk: Motivation for TAMA300 recycling Length sensing/control system Lock acquisition Earlier operation as a gravitational wave detector ~ We could start the operation
More informationThe Florida control scheme. Guido Mueller, Tom Delker, David Reitze, D. B. Tanner
The Florida control scheme Guido Mueller, Tom Delker, David Reitze, D. B. Tanner Department of Physics, University of Florida, Gainesville 32611-8440, Florida, USA The most likely conguration for the second
More informationSCG4000 V3.0 Series Synchronous Clock Generators
SCG4000 V3.0 Series Synchronous Clock Generators PLL 2111 Comprehensive Drive Aurora, Illinois 60505 Phone: 630-851-4722 Fax: 630-851- 5040 www.conwin.com Bulletin SG031 Page 1 of 12 Revision 01 Date 30
More informationIn this chapter we describe the history of GW detectors and the design of the LIGO GW detectors,
19 Chapter 3 Introduction to LIGO In this chapter we describe the history of GW detectors and the design of the LIGO GW detectors, which have been built for the detection of GWs. This description is broken
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 informationFFT Spectrum Analyzer
FFT Spectrum Analyzer SR770 100 khz single-channel FFT spectrum analyzer SR7770 FFT Spectrum Analyzers DC to 100 khz bandwidth 90 db dynamic range Low-distortion source Harmonic, band & sideband analysis
More informationEMX-1434 APPLICATIONS FEATURES A SMART PXI EXPRESS 4-CHANNEL KSA/S ARBITRARY WAVEFORM GENERATOR
83-0061-000 15A D A T A S H E E T EMX-1434 SMART PXI EXPRESS 4-CHANNEL 204.8 KSA/S ARBITRARY WAVEFORM GENERATOR APPLICATIONS Modal / GVT (Ground Vehicle Testing) Acoustics Shock / Vibration Rotational
More informationHigh Power and Energy Femtosecond Lasers
High Power and Energy Femtosecond Lasers PHAROS is a single-unit integrated femtosecond laser system combining millijoule pulse energies and high average powers. PHAROS features a mechanical and optical
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 informationJitter Measurements using Phase Noise Techniques
Jitter Measurements using Phase Noise Techniques Agenda Jitter Review Time-Domain and Frequency-Domain Jitter Measurements Phase Noise Concept and Measurement Techniques Deriving Random and Deterministic
More informationCal-Chip Electronics, Inc.
Cal-Chip Electronics, Inc. Feature: These new SSL Series is designed for the smallest possible size, low cost and high performance. It's high energy storage and very low DC resistance offer higher saturated
More informationVariable Gain Photoreceiver - Fast Optical Power Meter
The picture shows model -FC with fiber optic input. Features Conversion gain switchable from 1 x 10 3 to 1 x 10 11 V/W InGaAs-PIN detector Spectral range 900-1700 nm Calibrated at 1550 nm (fiber optic
More information7th Edoardo Amaldi Conference on Gravitational Waves (Amaldi7)
Journal of Physics: Conference Series (8) 4 doi:.88/74-6596///4 Lock Acquisition Studies for Advanced Interferometers O Miyakawa, H Yamamoto LIGO Laboratory 8-34, California Institute of Technology, Pasadena,
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 information5kW DIODE-PUMPED TEST AMPLIFIER
5kW DIODE-PUMPED TEST AMPLIFIER SUMMARY?Gain - OK, suggest high pump efficiency?efficient extraction - OK, but more accurate data required?self-stabilisation - Yes, to a few % but not well matched to analysis
More informationModel Hz to 10MHz Precision Phasemeter. Operating Manual
Model 6610 1Hz to 10MHz Precision Phasemeter Operating Manual Service and Warranty Krohn-Hite Instruments are designed and manufactured in accordance with sound engineering practices and should give long
More informationSupplementary Figures
1 Supplementary Figures a) f rep,1 Δf f rep,2 = f rep,1 +Δf RF Domain Optical Domain b) Aliasing region Supplementary Figure 1. Multi-heterdoyne beat note of two slightly shifted frequency combs. a Case
More informationTesting with Femtosecond Pulses
Testing with Femtosecond Pulses White Paper PN 200-0200-00 Revision 1.3 January 2009 Calmar Laser, Inc www.calmarlaser.com Overview Calmar s femtosecond laser sources are passively mode-locked fiber lasers.
More informationSC5407A/SC5408A 100 khz to 6 GHz RF Upconverter. Datasheet. Rev SignalCore, Inc.
SC5407A/SC5408A 100 khz to 6 GHz RF Upconverter Datasheet Rev 1.2 2017 SignalCore, Inc. support@signalcore.com P R O D U C T S P E C I F I C A T I O N S Definition of Terms The following terms are used
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 informationThis is a brief report of the measurements I have done in these 2 months.
40m Report Kentaro Somiya This is a brief report of the measurements I have done in these 2 months. Mach-Zehnder MZ noise spectrum is measured in various conditions. HEPA filter enhances the noise level
More informationCLIO Pocket is Audiomatica's new Electro-Acoustical Multi-Platform Personal measurement system.
Release 1.5! CLIO Pocket is Audiomatica's new Electro-Acoustical Multi-Platform Personal measurement system. The system comes complete of the CLIO Pocket software (Windows and OSX native), the CLIO CP-01
More informationPQ for Industrial Benchmarking with various methods to improve. Tushar Mogre.
General PQ: Power Quality has multiple issues involved. Thus, need to have some benchmarking standards. Very little is spoken about the LT supply installation within an industry. There is need to understand
More informationEMC Test Data. Radio Test Report R Summit Data Communications SDC-MCF10G. Test Report R76253 Rev 3.0. Revision History.
EMC Test Data Radio Test Report R76253 For The Summit Data Communications Model SDC-MCF10G Revision History Rev # Made By Date Comments 1.0 Mark Hill 31-Jul-09 Initial Release 2.0 Mark Briggs 11-Aug-09
More informationDG5000 Series Specifications
DG5000 Series Specifications All the specifications can be guaranteed if the following two conditions are met unless where noted. The generator is within the calibration period and has performed self-calibration.
More informationDatasheet SHF D Synthesized Clock Generator
SHF Communication Technologies AG Wilhelm-von-Siemens-Str. 23D 12277 Berlin Germany Phone +49 30 772051-0 Fax +49 30 7531078 E-Mail: sales@shf.de Web: http://www.shf.de Datasheet SHF 78210 D Synthesized
More informationOvercurrent Protection / 7SJ45
Overcurrent Protection / SJ SIPROTEC easy SJ numerical overcurrent protection relay powered by CTs Fig. / Description SIPROTEC easy SJ numerical overcurrent protection relay powered by current transformers
More informationComplex Sounds. Reading: Yost Ch. 4
Complex Sounds Reading: Yost Ch. 4 Natural Sounds Most sounds in our everyday lives are not simple sinusoidal sounds, but are complex sounds, consisting of a sum of many sinusoids. The amplitude and frequency
More informationLLS - Introduction to Equipment
Published on Advanced Lab (http://experimentationlab.berkeley.edu) Home > LLS - Introduction to Equipment LLS - Introduction to Equipment All pages in this lab 1. Low Light Signal Measurements [1] 2. Introduction
More informationWave Form: Square x 20.2 x 5.88H [0.504 x x 0.231] G8 500 khz ~ 170 MHz 4 pin DIL half size
V C X O G series What is a VCXO? Logic: TTL / CMOS Wave Form: Square MERCURY Since 1973 Unlike regular clock oscillator which has fixed output frequency, the output frequency of a VCXO (also known as frequency
More informationThe Multiplier-Type Ring Modulator
The Multiplier-Type Ring Modulator Harald Bode Introduction- Robert A. Moog Vibrations of the air in the frequency range of 20-20,000 cycles per second are perceived as sound. The unit of frequency is
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 informationUnderstanding Probability of Intercept for Intermittent Signals
2013 Understanding Probability of Intercept for Intermittent Signals Richard Overdorf & Rob Bordow Agilent Technologies Agenda Use Cases and Signals Time domain vs. Frequency Domain Probability of Intercept
More informationADC, FFT and Noise. p. 1. ADC, FFT, and Noise
ADC, FFT and Noise. p. 1 ADC, FFT, and Noise Analog to digital conversion and the FFT A LabView program, Acquire&FFT_Nscans.vi, is available on your pc which (1) captures a waveform and digitizes it using
More informationCHAPTER 5 FINE-TUNING OF AN ECDL WITH AN INTRACAVITY LIQUID CRYSTAL ELEMENT
CHAPTER 5 FINE-TUNING OF AN ECDL WITH AN INTRACAVITY LIQUID CRYSTAL ELEMENT In this chapter, the experimental results for fine-tuning of the laser wavelength with an intracavity liquid crystal element
More informationEULAMBIA ADVANCED TECHNOLOGIES LTD. Datasheet EAT-EOM-CTL-1. Alexandros Fragos
EULAMBIA ADVANCED TECHNOLOGIES LTD Datasheet Alexandros Fragos 2/5/2018 05/02/2018 Datasheet Datasheet 05/02/2018 Electro-Optic Modulator Bias Control Unit v2.0 Datasheet 3 05/02/2018 Datasheet Datasheet
More informationPlanar External Cavity Low Noise Narrow Linewidth Lasers
Planar External Cavity Low Noise Narrow Linewidth Lasers Lew Stolpner Redfern Integrated Optics Inc. Santa Clara, CA 95054, USA 1 Outline 1550 nm narrow linewidth lasers for fiber optic sensing Planar
More informationSC5307A/SC5308A 100 khz to 6 GHz RF Downconverter. Datasheet SignalCore, Inc.
SC5307A/SC5308A 100 khz to 6 GHz RF Downconverter Datasheet 2017 SignalCore, Inc. support@signalcore.com P RODUCT S PECIFICATIONS Definition of Terms The following terms are used throughout this datasheet
More informationHigh-Power Femtosecond Lasers
High-Power Femtosecond Lasers PHAROS is a single-unit integrated femtosecond laser system combining millijoule pulse energies and high average power. PHAROS features a mechanical and optical design optimized
More informationTransfer Function (TRF)
(TRF) Module of the KLIPPEL R&D SYSTEM S7 FEATURES Combines linear and nonlinear measurements Provides impulse response and energy-time curve (ETC) Measures linear transfer function and harmonic distortions
More informationKoji Arai / Stan Whitcomb LIGO Laboratory / Caltech. LIGO-G v1
Koji Arai / Stan Whitcomb LIGO Laboratory / Caltech LIGO-G1401144-v1 General Relativity Gravity = Spacetime curvature Gravitational wave = Wave of spacetime curvature Gravitational waves Generated by motion
More informationHF Power Amplifier (Reference Design Guide) RFID Systems / ASP
16 September 2008 Rev A HF Power Amplifier (Reference Design Guide) RFID Systems / ASP 1.) Scope Shown herein is a HF power amplifier design with performance plots. As every application is different and
More informationHigh collection efficiency MCPs for photon counting detectors
High collection efficiency MCPs for photon counting detectors D. A. Orlov, * T. Ruardij, S. Duarte Pinto, R. Glazenborg and E. Kernen PHOTONIS Netherlands BV, Dwazziewegen 2, 9301 ZR Roden, The Netherlands
More informationHP Archive. This vintage Hewlett Packard document was preserved and distributed by www. hparchive.com Please visit us on the web!
HP Archive This vintage Hewlett Packard document was preserved and distributed by www. hparchive.com Please visit us on the web! On-line curator: Glenn Robb This document is for FREE distribution only!
More informationGPS10RBN-26: 10 MHz, GPS Disciplined, Ultra Low Noise Rubidium Frequency Standard
GPS10RBN-26: 10 MHz, GPS Disciplined, Ultra Low Noise Rubidium Standard Key Features Completely self-contained unit. No extra P.C needed. Full information available via LCD. Rubidium Oscillator locked
More informationRakon Product Proposal
RTX5032A -- SMD Temperature Compensated Crystal Oscillator -- -- High performance TCXO offering excellent Phase Noise, Frequency Stability and VCO tilt compensation. -- Product description -- The RTX5032A
More informationMechanical modeling of the Seismic Attenuation System for AdLIGO
Mechanical modeling of the Seismic Attenuation System for AdLIGO Candidato: Valerio Boschi Relatore interno: Prof. Virginio Sannibale Relatore esterno: Prof. Diego Passuello 1 Introduction LIGO Observatories
More informationThe Measurement of Digitally Modulated RF Signals (The Basic Principles) Chris Swires, FSCTE. Swires Research.
The Measurement of Digitally Modulated RF Signals (The Basic Principles) Chris Swires, FSCTE. Swires Research. This paper was first presented to the Society of Cable Telecommunications Engineers at the
More informationSiPMs for solar neutrino detector? J. Kaspar, 6/10/14
SiPMs for solar neutrino detector? J. Kaspar, 6/0/4 SiPM is photodiode APD Geiger Mode APD V APD full depletion take a photo-diode reverse-bias it above breakdown voltage (Geiger mode avalanche photo diode)
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 informationThe rangefinder can be configured using an I2C machine interface. Settings control the
Detailed Register Definitions The rangefinder can be configured using an I2C machine interface. Settings control the acquisition and processing of ranging data. The I2C interface supports a transfer rate
More informationA 10-Gb/s Multiphase Clock and Data Recovery Circuit with a Rotational Bang-Bang Phase Detector
JOURNAL OF SEMICONDUCTOR TECHNOLOGY AND SCIENCE, VOL.16, NO.3, JUNE, 2016 ISSN(Print) 1598-1657 http://dx.doi.org/10.5573/jsts.2016.16.3.287 ISSN(Online) 2233-4866 A 10-Gb/s Multiphase Clock and Data Recovery
More informationData and Computer Communications Chapter 3 Data Transmission
Data and Computer Communications Chapter 3 Data Transmission Eighth Edition by William Stallings Transmission Terminology data transmission occurs between a transmitter & receiver via some medium guided
More informationLecture 6 ECEN 4517/5517
Lecture 6 ECEN 4517/5517 Experiment 4: inverter system Battery 12 VDC HVDC: 120-200 VDC DC-DC converter Isolated flyback DC-AC inverter H-bridge v ac AC load 120 Vrms 60 Hz d d Feedback controller V ref
More informationSHF Communication Technologies AG
SHF Communication Technologies AG Wilhelm-von-Siemens-Str. 23D 12277 Berlin Germany Phone +49 30 772051-0 Fax +49 30 7531078 E-Mail: sales@shf.de Web: http://www.shf.de Datasheet SHF 78120 D Synthesized
More information2400C Series Microwave Signal Generators 10 MHz to 40 GHz. Preliminary Technical Datasheet. Low Phase Noise and Fast-Switching Speed in a Single Unit
Preliminary Technical Datasheet 2400C Series Microwave Signal Generators 10 MHz to 40 GHz Low Phase Noise and Fast-Switching Speed in a Single Unit 2400C Series Microwave Signal Generator Signal Generator
More informationMultiply Resonant EOM for the LIGO 40-meter Interferometer
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO - CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY LIGO-XXXXXXX-XX-X Date: 2009/09/25 Multiply Resonant EOM for the LIGO
More informationAnalog Arts AG900 AG885 AG875 AG815 Product Specifications
www.analogarts.com Analog Arts AG900 AG885 AG875 AG815 Product Specifications Arbitrary Waveform Generator General ( Typical ) Specifications AG900 AG885 AG875 AG815 Arbitrary waveform length 2 to 64K
More informationLab 4. Crystal Oscillator
Lab 4. Crystal Oscillator Modeling the Piezo Electric Quartz Crystal Most oscillators employed for RF and microwave applications use a resonator to set the frequency of oscillation. It is desirable to
More informationOperation Manual. Model SG Elenco Precision Wide Band Signal Generator
99 Washington Street Melrose, MA 02176 Phone 781-665-1400 Toll Free 1-800-517-8431 Visit us at www.testequipmentdepot.com Elenco Precision Wide Band Signal Generator Model SG-9000 Operation Manual CONTENTS
More informationCommon Mode Servo Board Test Procedure
Author: Refer to: Dani Atkinson / Daniel Sigg LIGO-E1100429-v3 Date: April 29, 2011 Common Mode Servo Board Test Procedure Test Preparation Enter Name, Date, Revision, Board Serial Number and board to
More informationSwitch Mode Power Supply Measurements
Switch Mode Power Supply Measurements Application Note Using an Agilent InfiniiVision 3000/4000 X-Series Oscilloscope With the Power Measurements Option Introduction Agilent s 3000 and 4000 X-Series oscilloscopes
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 informationMeasurement of Digital Transmission Systems Operating under Section March 23, 2005
Measurement of Digital Transmission Systems Operating under Section 15.247 March 23, 2005 Section 15.403(f) Digital Modulation Digital modulation is required for Digital Transmission Systems (DTS). Digital
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 informationAD9772A - Functional Block Diagram
F FEATURES single 3.0 V to 3.6 V supply 14-Bit DAC Resolution 160 MPS Input Data Rate 67.5 MHz Reconstruction Passband @ 160 MPS 74 dbc FDR @ 25 MHz 2 Interpolation Filter with High- or Low-Pass Response
More informationOscilloscope Calibration Options for Fluke 5500A/5520A Multi-Product Calibrators Extended Specifications
Oscilloscope Calibration Options for Fluke 5500A/5520A Multi-Product Calibrators Extended Specifications These specifications apply to the 5520A-SC1100, 5500A-SC600 and 5500A-SC300 Oscilloscope Calibration
More informationSynchronized Crystal Oscillator, General Requirements. AH-ASCMXXXG-X Series PATENT PENDING
PATENT PENDING Description The Synchronized Crystal Oscillator is intended for use in the system, which requires multiple clocks in different nodes of the system to run synchronously in frequency without
More informationLecture 8 Fiber Optical Communication Lecture 8, Slide 1
Lecture 8 Bit error rate The Q value Receiver sensitivity Sensitivity degradation Extinction ratio RIN Timing jitter Chirp Forward error correction Fiber Optical Communication Lecture 8, Slide Bit error
More information