PPT-Frequency Scanning Interferometry (FSI) measurements

PACMAN internal meeting 28042014 Solomon William Kamugasa Background concepts Interferometry Displacement amp FSI Sources of error in FSI System components How to determine 3D position using FSI. measurements: . One physicist’s crooked . path from quantum optics to quantum information. Introduction . Squeezed states and optical . interferometry. Ramsey . interferometry. and cat states. Quantum information perspective. A. dvanced . M. etrology . U. sing . L. as. E. r . T. racers. John Dale. 2. Project Aim. To take Frequency Scanning Interferometry (FSI) from the lab into a product. 3. Frequency Scanning Interferometry (FSI) Absolute measurements. Berlin/. Zeuthen. ;. . May 2010. Dainis Dravins & . Hannes. Jensen. Lund Observatory, Sweden. www.astro.lu.se. /~dainis. HUNDRED TIMES SHARPER THAN . HUBBLE !. Intensity Interferometry with. Summary output from FSI “Away Day” – April 2012. High level overview. The following is a high-level summary of the comments entered into Think Tank by participants at the meeting.. It is not a record of all the comments made and some comments have been summarised or aggregated into common themes.. interferometry. Steven van den Berg. International Colloquium . Observatoire. de Haute Provence . 23-27 September 2013. Outline. . 2. Introduction to VSL. Introduction to the frequency comb. Distance determination based on:. Launch App Switcher - Click on Assessments . Choose folder and test . Scroll to the bottom of Assessment Overview Page and click on PDF with Student Names . School Admins . – . Select School and click Choose this school and continue to next step. in. Mumbai, Navi Mumbai. By. Mr. M.D. . Lele. Chief Planner, CIDCO. On 31.8.2013 at 11.45a.m.. Venue: Buddha . Purnima. Project Authority, Tank Bund, Hyderabad. Table of Contents. Background. Computation of FSI. Lesson 7. Scanning. Ping Sweeps. Port Scanners. Vulnerability Scanning tools. Ping Sweep. PING (Packet INternet Groper). A utility designed to determine whether or not a remote system is accessible.. Jonathan Singh . (. jonathan.singh@ed.ac.uk. ). A Curtis, I Main, A . Cartwright-Taylor, I . B . Butler, M Chapman, F . Fusseis. Outline. What is the Velocity?. CWI for Monitoring Velocity Change. Experimental Rock Physics Applications. Material for this talk: A.M.S. Richards, T.W.B.Muxlow, N.J.Jackson (JBCA Manchester); . R.A.Laing (ESO Garching); I. Marti-Vidal (OSO, Onsala); R. Perley (NRAO Socorro) and Wikipedia. Summary. Radio astronomy – key aspects. Dainis Dravins, . Hannes. Jensen . Lund Observatory, Sweden. Stephan LeBohec, Paul D.. . Nuñez. . The University of Utah, Salt Lake City. STELLAR INTENSITY INTERFEROMETRY. . Astrophysical targets for sub-. Very Long Baseline Interferometry. Very Long Baseline Interferometry. time.  . θ.  . t. Very Long Baseline Interferometry. Moving Sources.  .  .  .  .  .  . 0 .  .  .  .  .  .  . What is the signal made of?. small energies. Hartmut. Machner, FZ . Jülich. and Univ. Duisburg-Essen. Frank . Hinterberger. , Univ. Bonn. Regina . Siudak. , PAN Krakow. for the . HIRES & GEM . collaborations. Why. . is. . (g) Candidates should be able to show an understanding of how the image of an 8-voxel cube can . be developed . using CT scanning.. X-ray: The beginning . X-Rays . discovered . in 1895 by Wilhelm Conrad Roentgen .