PDF-Excitements and Challenges forFuture Light Sources Based on X-Ray FELs

SASE FELs Undulator Regime Undulator RegimeExponential Gain Regime Exponential Gain RegimeSaturation Saturation 1 of XRay Pulse 1 of XRay Pulse Electron BunchMicroBunching Electron BunchMicroB. On tex straddle thi schemati divide A large d lux publicatio n appeare i 187 fro th publishin hous o Gran Co title London a pilgrimage Produc o th collaboratio o a Britis journalis Blanchar Jerrol d an a Frenc artis Gustav Dore i initiall appeare i Energy . Q. uantiles. Jaesub Hong. Spring, 2011. Outline. The X-ray sources in the Galactic Bulge. Quantile. Analysis. Periodic. Bulge X. -ray . Sources and Modulating Energy . Quantiles. Galactic Center Region (32’ . Andrew Levan. University of Warwick. Parameter space. Kouveliotou. et al. 1993. Parameter space. Kulkarni. & . Kasliwal. 2010. Parameter space. LGRBs. SGRBs. SGRs. ?. TDEs?. Galactic sources (SGR, LMXB, HMXB, . Briefing for SEAB. 20 June 2014. Patricia M. Dehmer. Acting Director, Office of Science. U.S. . Department of . Energy. What, why, how, where?. Office of Science light sources. Storage rings. Free electron lasers. Centaurus. X-3 Over its Binary Orbit”. -. Sachindra. Naik, . Biswajit. Paul, and . Zulfikar. Ali. Introduction:. Interest: Extended dips in the light curve. Cen-X: Eclipsing HMXRB pulsar. Orbital period ~2.1 days, pulse period ~4.8 s. Measurements of the speed of light:. c = 3 . × 10. 8. m/s = . 186,000 miles/s. light propagating through matter – . transparent vs. opaque. materials. colors. The bending of light – refraction. with matter. Interaction of x-ray photons with matter. . When a beam of x-ray photons passes through matter, its intensity (energy . –. or number of x-ray photons - flowing per second) is reduced: . 1. November 8, 2011. Greensboro, North Carolina. Bill Cox. Deputy Director. Grants, Training and Outreach. North Carolina State Education Assistance Authority. Topics. Forgivable Loans for Education Service (NC FELS). Computational Photography. Derek Hoiem, University of Illinois. Many slides from Debevec, some from Efros. T2. Next week. Derek away for ICCV (Venice). Zhizhong and Aditya will teach and . hold office hours, etc.. Measurements of the speed of light:. c = 3 . × 10. 8. m/s = . 186,000 miles/s. light propagating through matter – . transparent vs. opaque. materials. colors. The bending of light – refraction. USING DATA ON EXTRAGALACTIC DIFFUSE . GAMMA-RAY EMISSION. . A. . Uryson. Lebedev. Physical Institute RAS, . Moscow. INTRODUCTION. UHECR data are obtained by Pierre Auger Observatory (PAO) and Telescope Array (TA):. Visibility Problem. Rendering: converting a model to an . image. Visibility. : deciding which objects (or parts) will appear in the image. Object-. order. OpenGL (later). Image-order . Ray Tracing (now). Jon Marangos, Imperial College London. Motivation for . attosecond. science. Current capability. Future trends. Requirements. 1. What is . attoscience. ?. Electron Orbit in Bohr Model. T. orbit. .  150 . X ray film. It has 2 principal components:. Emulsion and Base. Emulsion is sensitive to x rays and visible light, records the r/g image. Base is a plastic supporting material onto which emulsion is coated.