'Synchrotron' diaporamas de présentation

3 rd Generation Synchrotron Light Sources

3 rd Generation Synchrotron Light Sources. Francis Perez. Outline. 2. Synchrotron Radiation Synchrotron Light Sources 1st, 2nd, 3rd and Next Generation Enabling technologies Insertion devices Vacuum (NEG coating) Electronics (BPMs, LLRF, FOFB) Top UP Simulation tools

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Synchrotron Radiation, continued

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Cracow, June 26-30, 2006

Josep M. Paredes. BROAD-BAND EMISSION FROM MICROQUASAR JETS. Cracow, June 26-30, 2006. OUTLINE. How many microquasars we know Non-thermal low energy radiation from MQ jets MQ jets as HE and VHE ? -ray sources: Theoretical point of view

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Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School

Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School. 1. Unidentified CMB signal (T.Shmaonov, 1957, Ph.D) 2. CMB or Black Body population of Radio Sources? (Y.Par, 1968) 3.CMB polarization (Penzias: <100mK; Pulkovo: <1mK)

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Large-circumference, Low-field Optimization of a Future Circular Collider

350 GeV e + e -. Large-circumference, Low-field Optimization of a Future Circular Collider. 3 00 TeV pp. Peter McIntyre, Saeed Assadi, Chase Collins, James Gerity, Joshua Kellams, Tom Mann, Al McInturff, Chris Mathewson, Nate Pogue , Akhdiyor Sattarov, Richard York 1

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Leptonic and Hadronic Modeling of Gamma-Ray Blazars

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Status of J-PARC K1.8 Beam Line

Status of J-PARC K1.8 Beam Line. Kiyoshi Tanida Department of Physics and Astronomy, Seoul National University HNP2011 , POSTECH Feb. 24, 2011. J-PARC: W here is it?. Tokai, Japan. 50 GeV Synchrotron (15 m A). Material and Biological Science Facility. 3 GeV Synchrotron (333 m A).

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PARAMETRIC X-RAYS: READY FOR APPLICATION

PARAMETRIC X-RAYS: READY FOR APPLICATION. Alexander LOBKO Institute for Nuclear Problems, Belarus State University Minsk. IX Gomel School - July 200 7. Light sources. nano-science. http://www.lightsources.org/cms/?pid=1000166. Spectral brilliance of T- & x-ray sources.

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GAMMA-RAY BLAZARS NEAR EQUIPARTITION AND THE ORIGIN OF THE GEV SPECTRAL BREAK

Colliding Shell and External Shock Origin of the Prompt and Early Afterglow Emissions of Fermi GRBs Chuck Dermer Naval Research Laboratory, Washington, DC charles.dermer@nrl.navy.mil. Following ideas presented in papers with. Matteo Cerruti,* Catherine Boisson, Andreas Zech

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Dwarf galaxies and the Magnetisation of the IGM

Dwarf galaxies and the Magnetisation of the IGM. Uli Klein. ?. Coma. Giovannini et al. (1993). Clarke et al. (2001). ICM is magnetized (throughout?) Galaxy clusters exhibit: radio halos Faraday rotation peripheral radio structures. relativistic electrons have short lifetimes.

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Synchrotron Diffraction

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Conflict of Interest Disclosure <Hidezo> <Mori>, <MD>

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Introduction Cyclotron vs synchrotron Design issues Beam delivery issues Conclusion

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Particle Accelerators for Research and for Medicine

Particle Accelerators for Research and for Medicine. Prof. Ted Wilson (CERN and Oxford University) based on the book:. ISBN-013 978-981-270-070-4 http://www.enginesofdiscovery.com/ This talk: http://www.enginesofdiscovery.com /eod.pdf. The race to high energies.

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Far infrared emission of solar flares

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Update on ACD for Project X

Update on ACD for Project X. Sergei Nagaitsev May 21, 2009. PrX Research Program Task Force. Formed recently; leader : R. Tschirhart Motivation: the ICD does not provide beam to rare decay experiments directly, ends at the extraction kicker in the Recycler.

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ACA Etter Prize for X-ray optics innovations Sterling Cornaby (CHESS/Cornell, NY), DMR-0225180

ADSC Q4 Detector. ACA Etter Prize for X-ray optics innovations Sterling Cornaby (CHESS/Cornell, NY), DMR-0225180.

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C. H. Jaroschek and R. A. Treumann

Synchrotron Radiation in Pair Reconnection. Figure 1 . Left : Accelerating reconnection-electric field. Right : Time evolution of synchrotron power emissivity ( top ) and total power spectrum ( bottom ) for the corresponding pair plasma.

96 views • 1 slides