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Bernhard Holzer CERN-LHC * Bernhard Holzer CERN CAS Prague 2014 x´ x ● ● ● ● ● ● Liouville: in reasonable storage rings area in phase space is constant A = π*ε=const…
Atom Atomic number A Number of protons Z Number of neutrons A-Z Number of electrons Z Charge of electron = charge of proton ~16×10-19 C Size of the atom ~10-10 m Size of…
Jochen Stahn Laboratorium für Neutronenstreuung ETH Zürich Paul Scherrer Institut A neutron polariser based on magnetically remanent FeSi supermirrors ILL Grenoble 26…
Aperture Radiation: Huygen’s Equation y z ϕx θ R x αx r(x, y) Superposition of contributions from radiating patches ϕy Aperture in X-Y plane “A” Radiating patch,…
Well-typed programs can’t be blamed ESOP 2009 Robert Bruce Findler Northwestern University Philip Wadler University of Edinburgh Aussois 14–18 October 2013 Part I Evolving…
IOP PUBLISHING INVERSE PROBLEMS Inverse Problems 24 (2008) 055001 (23pp) doi:10.1088/0266-5611/24/5/055001 Coherent interferometric imaging for synthetic aperture radar in…
Risoluzioni radar Risoluzione in azimut (along-track): ∆∆∆∆x = ra = ββββ R ≅≅≅≅ R λλλλ/L R: “slant range” Migliore risoluzione: L Risoluzione…
Seoul Nat’l Univ. NRL HoloTech 4. 4. FresnelFresnel and and FraunhoferFraunhofer DiffractionDiffraction Seoul Nat’l Univ. NRL HoloTech 3 2max22 4 ηξλ π −+− yxz…
Prompt GRB Optical Follow-up Experiments Hye-Sook Park Lawrence Livermore National Laboratory Livermore, CA USA Hye-Sook Park Upper Limits on the Prompt Optical Emission…
Slide 1R. Bruce, M. Giovannozzi, S. Redaelli With essential input from G. Arduini, R. De Maria, S. Fartoukh, M. Fitterer, R. Tomas, J. Wenninger, aperture team Aperture calculations…
EXPLICIT BOUNDS FOR SUMS OF SQUARES JEREMY ROUSE Abstract For an even integer k let r2kn be the number of representations of n as a sum of 2k squares The quantity r2kn is…
Closing the Feedback Loop: A 12-month Evaluation of ASTA, a Self-Tracking Application for ASHAs Brian DeRenzi† Jeremy Wacksmanφ Nicola Dell‡ Scott LeeΨ Neal Leshφ…
PNM-9081VQ VIDEO Imaging Device 1/1.8" 6M CMOS x 4 Total / E�ective Pixels 3,096(H) x 2,094(V) 6M x 4 / 2,616(H) x 1,976(V) 5M x 4 Scanning System Progressive Scan…
Document TitleDescription 1 Diffraction and Fourier OpticsDiffraction and Fourier Optics Ethan Brown Derrick Toth Document TitleDescription 2 Fourier Transforms in Optics…
International Association of Mathematical Physics Μ Φ U Invitation Dear IAMP Members according to Part I of the By-Laws we announce a meeting of the IAMP General Assembly…
Appendix A Definitions and Symbols A.1 Symbols and Conversion Factors A absorptivity a distance aperture b net increase in number of molecules per formula unit b = μ−…
Proposal for KL → π0νν Experiment at J-Parc April 28 2006 Revised: May 2 2006 Joseph Comfort and Jeremy Figgins Arizona State University Physics Department Tempe Arizona…
TeV Astrophysics with HAWC Gus Sinnis Los Alamos National Laboratory PACIFIC 2014G Sinnis The Electromagnetic Spectrum 103 10 10-1 10-3 10-5 10-7 10-9 10-11 10-13 10-15 10-17…
The James Webb Space Telescope JWST is a 6.5-meter-aperture observatory optimized for infrared astronomy 0.6 - 28 μm. JWST is the first infrared space telescope to employ…
11 12 MEGAPIXEL C-MOUNT LENS ● 8 12 16 25 35 50mm 6 Lens Series ● Compatible with 11 φ176mm Large Format Sensor ● Ultra-High Resolution 12MP ● Compact 11 Design…