'Test mass' diaporamas de présentation

Multiplicity in a decision-making context

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aLIGO Photon Calibrators Calibration Pablo Daveloza University of Texas at Brownsville and

aLIGO Photon Calibrators Calibration Pablo Daveloza University of Texas at Brownsville and B. Abbott, J. Berliner, C. Conley, S. Shankle, T. Steckler, R. Savage. Overall Concept. Pcal Receiver. End Test Mass. Pcal Transmitter.

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The search for gravitational waves Matthew Pitkin

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An Optical Readout System for the LISA Gravitational Reference Sensor

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Selim Shahriar, Northwestern University

LIGO G0900207. Design constraints and optimization for a white light cavity based GW interferometer including power and signal recycling. Selim Shahriar, Northwestern University. Laboratory of Atomic and Photonic Technologies. URL: http://lapt.ece.northwestern.edu.

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Dynamics Modeling and First Design of Drag-Free Controller for ASTROD I

Dynamics Modeling and First Design of Drag-Free Controller for ASTROD I. Hongyin Li, W.-T. Ni Purple Mountain Observatory, Chinese Academy of Sciences S. Theil, L. Pettazzi, M. S. Guilherme. ZARM University of Bremen, Germany. Outline. Introduction of the Mission Simulator

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Advanced LIGO

Advanced LIGO. David Shoemaker NSF LIGO Review 23 October 2002. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Must be of significance for astrophysics

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Vibrations

Today : Finish Chapter 14 (Gases and Plasmas) Chapter 15 (Temp, Heat, Expansion ) Next homework due Tuesday. Vibrations. Some Preliminaries Vibration = oscillation = anything that has a back-and-forth to it Eg . Draw a pen back and forth over the same line, repeatedly:

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Cosmology

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8. Hypotheses 8.2 The Likelihood ratio at work

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Measurements of electrical charge variations on fused silica samples

Measurements of electrical charge variations on fused silica samples. L.G.Prokhorov, V.P.Mitrofanov Moscow State University LIGO-G060080-00-Z. Variation of charge as a source of noise.

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Spectral shape of solar particle events at energies above

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AdLIGO Optical configuration and control Nov 10, 2005 Alan Weinstein

AdLIGO Optical configuration and control Nov 10, 2005 Alan Weinstein for AdLIGO Interferometer Sensing and Control (ISC) and the 40 meter lab. 40 KG FUSED SILICA. AdLIGO optical configuration and control.

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Critical mechanical technologies for future gravitational-wave astronomy

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Acceleration Noise in LISA

Surface Potential Measurements with the LISA Kelvin Probe Jordan Camp LIGO/LISA Charging Workshop July 26, 2007 G070573-00-R. Acceleration Noise in LISA. LISA measurement sensitivity is 10 -12 m over 1000 sec A force of 10 -16 N will produce this displacement in 1000 sec!

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Combined approach for vehicle test weight, stepless inertia and vehicle selection

Combined approach for vehicle test weight, stepless inertia and vehicle selection. Revised proposal by The Netherlands (Andre Rijnders ), T&E (Iddo Riemersma) and ICCT (Peter Mock). 16 April 2012 DTP meeting Geneva. General consideration.

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Combined approach for vehicle test weight, stepless inertia and vehicle selection

Combined approach for vehicle test weight, stepless inertia and vehicle selection. WLTP-DTC-08-04. Revised proposal by The Netherlands (Andre Rijnders ), T&E (Iddo Riemersma) and ICCT (Peter Mock). 18 January 2012 DTP meeting Geneva. General consideration.

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Technical Progress Planned/Needed in FY07

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Motion Sensor

Motion Sensor. Muhajir Ab. Rahim School of Mechatronic Engineering, KUKUM. Introduction. Designed to measure the rate of change of position, location, or displacement of an object that is occurring.

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System Design Assessment for a Mission to Explore the Pioneer Anomaly

System Design Assessment for a Mission to Explore the Pioneer Anomaly. Jonathan Fitt School of Physics and Astronomy, University of Birmingham, Edgbaston, UK. A New Mission

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