PPT-Principles of Interferometry

I CASS Radio Astronomy School R D Ekers 24 Sep 2012 292Sep 2012 R D Ekers 2 WHY Importance in radio astronomy ATCA VLA WSRT GMRT MERLIN IRAM VLBA JIVE VSOP RADIOASTON ALMA LOFAR MWA ASKAP MeerKat SKA. 1 uct brPage 2br 2 Stati tical methods of age resto on 3 Present lculat ns brPage 3br brPage 4br 4 nc us on Ack owledg ments Refer nces 23 69 73 15 6 22 60 21 A2 O Nitti 1 L De Vitis 1 F Bovenga 2 R Nutricato 3 A Refice 2 J Wasowski 4 1 Dipartimento Interateneo di Fisica Politecnico di Bari Via Amendola 173 70126 Bari Italy mail davidenittifisicaunibait 2 CNRISSIA Via Amendola 122D 70126 Bari Italy Emai 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. Berlin/. Zeuthen. ;. . May 2010. Dainis Dravins & . Hannes. Jensen. Lund Observatory, Sweden. www.astro.lu.se. /~dainis. HUNDRED TIMES SHARPER THAN . HUBBLE !. Intensity Interferometry with. limits on . dark . energy. Jun. 17. 2011. Geena Kim. P. Hamilton, D. Schlippe, and H. Mueller. University of California, Berkeley. Paul Hamilton. Müller group. University of California at Berkeley. . Clare Burrage. University of Nottingham. Clare.Burrage@nottingham.ac.uk. Outline:. Chameleon dark energy. A . review of atom interferometry. Dark energy in the laboratory. Solutions to the Cosmological Constant Problem.


Interferometry Independent Validation and Intercomparison of Results. Final Report BRGM/RP-55649 -FR June 2007









PSIC4 Persistent Scatterer Interferometry Independent Valida 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?. during the last decade. Olivier CHESNEAU. delivered and distorted by John . Monnier. 2. 3. Albert A. Michelson (1852-1931). 1974: I2T. 4. . MIDI . First direct recombination (2T) in the mid-IR (8-13. Achuta . Kadambi. , Jamie . Schiel. and Ramesh . Raskar. , IEEE CVPR16 . An interferometric 3D camera for multipath imaging for meter scale scenes. Swept Frequency Electronic Interferometry. Take-home message:. Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics, Northwestern University. NPS Colloquium. February 1, 2019 . Conceptual overview of atom interferometry. Motivation for gravitational wave detection in the “mid-band” frequency range of ~ 0.1 Hz to 10 Hz.