PPT-Modeling Auger processes DUE to high Intensity, ultrafast x-ray pulses

drhgfdjhngngfmhgmghmghjmghfmf Ray sullivan Undergraduate Intern Under supervision of Antonio Picón Argonne National Lab Lemont IL SULI Program Outline Introduction and Background Information. (AES). 1. Brief History. Auger . E. ffect discovered in 1920’s. Meitner published first journal. Auger transitions . considered noise at first. 1953-JJ Lander. Characterization of solids today. 2. Three Steps of Auger Electron Spectroscopy. Pierre Auger Observatory. Lawrence Wiencke. Colorado School of Mines. IS@AO, Apr. 18 2011, Cambridge. 1. 2. Wiencke. Logarithmic Scale. Linear Scale. Linsleys. x10. 5. Linsleys. TA. The Pierre Auger Observatory. ELI’s Lynchpin. ELI-NP: The . W. ay Ahead . Bucharest . March 10, 2011. Gérard . Mourou. ,. . Institut. de Lumière . Extrême. 28/02/11. mourou CEA Bruyere. The laser is 50!! . . by Mike Plum. Ring Area Manager. Spallation Neutron Source. Workshop on Optics . Measurements, Corrections, and Modeling at High Performance Storage . Rings, CERN, . June 20-22, 2011 . High . i. ntensity challenges. Relativistic . Surface . High Harmonic Generation. Christian Rödel. , Silvio Fuchs, Martin Heyer, Oliver Jäckel, Gerhard G. Paulus. . FSU Jena, Institut für Optik und Quantenelektronik, Helmholtz Institut Jena. (2).  .  . Maria Novella Piancastelli.  . Sorbonne . Universités. , UPMC . Univ. Paris 06, CNRS, . Laboratoire . de Chimie Physique-Matière et . Rayonnement, . France.  . Department of Physics and Astronomy, . Martin Centurion. Department of Physics and Astronomy. University of Nebraska – Lincoln. 1. Outline. 2. Diffraction from aligned molecules:. 3D molecular images with sub-Angstrom resolution. Imaging of transient structures: Molecules in intense laser fields.. Cosmic Ray Experiment. Glenn . Sembroski. QuarkNet. Summer Workshop. July 24,2012. The Big Question. Which has become the Big Mystery. Where do Cosmic Rays come from?. A multi-part question. i.e. Lots of small mysteries. and. Potential Interactions with . the . ACME . Community. June 5, 2017. . RGCM program - Overview. Goal . is . to enhance . a . predictive . and process- and system-level understanding. of the . modes of variability and change. Paragraph 2 of the Administrative Order issued by the Pennsylvania Department of Environmental Protection on January 3 2018 to Sunoco Pipeline LP 147Sunoco148 requested that Sunoco submit a detailed d Nathan D. Wong, PhD,a Dan Kouwabunpat,b Anthony N. Vo, BS, a Robert C. Detrano, MD, PhD,C Harvey Eisenberg, MD,d Mukesh Goel, MD,a and Jonathan M. Tobis, MD” Irvine, Newport Beach, and Torrance, Lighting Basics. Equipment. Dynalite. Fiber optics. Modeling lights. SolMate. Light Pad. Moving Modeling Lights. Adjusting the intensity on the . Dynalite. Flash . Powerpack. Additional Equipment Used. Also known as: AES, Auger, SAM. 1. Auger Electron Spectroscopy. E. KLL. = E. K. - E. L. - E. L. ’. 2p. 1s. 2s. 1/2. 3/2. E. f. K. L. I. L. II. L. III. Incident Beam. Auger. Electron. E. KLL. 0. Glenn . Sembroski. QuarkNet. Summer Workshop. July 24,2012. The Big Question. Which has become the Big Mystery. Where do Cosmic Rays come from?. A multi-part question. i.e. Lots of small mysteries. Different answers for different energy regimes.