'Www ligo caltech edu' presentation slideshows

Experiment 2

Experiment 2. * Part A: Intro to Transfer Functions and AC Sweeps * Part B: Phasors, Transfer Functions and Filters * Part C: Using Transfer Functions and RLC Circuits * Part D: Equivalent Impedance and DC Sweeps. P 1. I. Constriction. Pump. I. P 2. In Class Solution.

1.01k views • 68 slides

Experiment 2

Experiment 2. * Part A: Intro to Transfer Functions and AC Sweeps * Part B: Phasors, Transfer Functions and Filters * Part C: Using Transfer Functions and RLC Circuits * Part D: Equivalent Impedance and DC Sweeps. Part A. Introduction to Transfer Functions and Phasors

870 views • 61 slides

Experiment 5

Experiment 5. * AC Steady State Theory * Part A: RC and RL Circuits * Part B: RLC Circuits. AC Steady State Theory. Transfer Functions Phasors Complex Impedance Complex Transfer Functions. Transfer Functions.

798 views • 60 slides

LIGO Data & Computing Update Albert Lazzarini LIGO Laboratory at Caltech

LIGO Data & Computing Update Albert Lazzarini LIGO Laboratory at Caltech 12 th Meeting of the LIGO Laboratory PAC 26 June 2002 Cambridge, MA. Outline for this talk. Simulation & Modeling Data Analysis Systems Grid Computing Staffing. Modeling & Simulation Activities Overview.

555 views • 41 slides

Data Analysis Techniques for Gravitational Wave Observations

Data Analysis Techniques for Gravitational Wave Observations. S. V. Dhurandhar. I U C A A Pune, India. Great strides taken by experimentalists in improving sensitivity of GW detectors. Technology driven to its limits. Gravitational Wave Data Analysis

504 views • 37 slides

There is a big difference between the Newtonian and the Relativistic frameworks:

464 views • 23 slides

S2/S3 calibration

349 views • 23 slides

292 views • 17 slides

A proposal for additional L ow F requency G ravitational W ave I nterferometric D etectors at LIGO

A proposal for additional L ow F requency G ravitational W ave I nterferometric D etectors at LIGO. Riccardo DeSalvo California Institute of Technology Globular Cluster 17 th October 2003 LIGO- xxx. Status of observations now and here!!. TAMA has been running for >3 years

243 views • 12 slides

S3 Data Quality Investigation

John Zweizig LIGO/Caltech. S3 Data Quality Investigation. S3 Data Quality Segments. Data quality results will be presented as segments Segment list available at: http://tenaya.physics.lsa.umich.edu/~keithr/S3DQ/

144 views • 6 slides

Background: simulation of merging black holes by Werner Berger

Gravitational Waves and LIGO Tiffany Summerscales, Dept. of Physics. What are gravitational waves?

135 views • 1 slides

Background: simulation of merging black holes by Werner Berger

Gravitational Waves and LIGO Tiffany Summerscales, Dept. of Physics. What are gravitational waves?

86 views • 1 slides