PPT-Polarization in Interferometry

Rick Perley NRAOSocorro Recap and Plan Dave has shown you why determining the full polarization state of natural radiation is important In this lecture I describe how an interferometer determines the Stokes parameters for distant sources. 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. . Class Activities: . Polarization (1). Class Activities: . Polarization (2). A stationary point charge +Q is near a block of polarization material (a linear dielectric). The net electrostatic force on the block due to the point charge is . in . Interferometry. . Rick . Perley. (NRAO-Socorro). Recap, and Plan. Dave has shown you why determining the full polarization state of natural radiation is important. . In this lecture I describe how an interferometer determines the Stokes parameters for distant sources. 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. 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. 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?. Carma. probing small-scale magnetic fields in star-forming regions. Chat Hull. University of California, . Berkeley. Radio Astronomy Laboratory. 10 April 2013. Special Session: Polarization. ALMA 2013 Rocks!. 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:. Polarization (1). Class Activities: . Polarization (2). A stationary point charge +Q is near a block of polarization material (a linear dielectric). The net electrostatic force on the block due to the point charge is . Markus . B. öttcher. North-West University. Potchefstroom, South . Africa. 0. Most of this work done by:. Haocheng. Zhang. . (Ohio University & Los Alamos). Leptonic. . Blazar. . Model. Relativistic jet outflow with . Tom Patterson. April 20, 2023. The Making of a Polarized Nation. The gradual realignment . that fueled today’s polarized politics. Race. – 1964 Civil Rights Act, plus. Cultural issues . – late 1960s and 1970s.