'100 mev' presentation slideshows

High-Energy Astrophysics with AGILE

638 views • 52 slides

Gamma-ray Large Area Space Telescope

527 views • 36 slides

444 views • 35 slides

Neutron spectra in Atmosphere at various Altitudes and Latitudes

Neutron spectra in Atmosphere at various Altitudes and Latitudes. A. Zanini, L.Visca INFN-Istituto Nazionale di Fisica Nucleare Sezione di Torino. GCR (Galactic cosmic Rays): galactic origin, generated outside the solar system.

816 views • 33 slides

Statistical Issues in High-Energy Gamma-Ray Astronomy for GLAST

Statistical Issues in High-Energy Gamma-Ray Astronomy for GLAST. PHYSTAT2003 S. Digel (Stanford Univ./HEPL). 10 September 2003. Outline. Introduction Gamma-ray astro- & astroparticle physics Important points about gamma-ray astronomy GLAST mission

429 views • 28 slides

Search for ? -meson production in ?? interactions with e + e - colliding beams at ?s = 1 GeV

351 views • 28 slides

Status of Radiation Protection Studies for the Linac4 beam dumps

431 views • 28 slides

On-Orbit Anomalies : Investigations and Root Cause Determination

707 views • 25 slides

Cheolho Pyeon Research Reactor Institut e, Kyoto University, Japan pyeon@rri.kyoto-u.ac.jp

Thorium-Loaded Accelerator-Driven System Experiments in Kyoto University Research Reactor Institute. Cheolho Pyeon Research Reactor Institut e, Kyoto University, Japan pyeon@rri.kyoto-u.ac.jp. Contents. Background and P urpose

428 views • 23 slides

STATUS OF THE ALBA SYNCHROTRON LIGHT SOURCE: FROM COMMISSIONING TO OPERATION

STATUS OF THE ALBA SYNCHROTRON LIGHT SOURCE: FROM COMMISSIONING TO OPERATION. M.Pont, CELLS-ALBA 08.08.2012. OUTLINE. The ALBA synchrotron light source Results of Commissioning Operation in 2012 Summary and outlook. ALBA SYNCHROTRON LIGHT SOURCE. Offices. Synchrotron building.

405 views • 23 slides

Increase of PXR intensity due to Borrmann effect

Increase of PXR intensity due to Borrmann effect. 1) Islamic Azad University, Malayer , Iran, Physics department 2) Belarusian State University, Minsk, Belarus, Physical faculty, Department of Theoretical physics. A. Ahmadi 1),2) , I.Feranchuk 2) , A. Benediktovitch 2 ). Outline.

338 views • 19 slides

Pass 6: GR V13R9 Muons, All Gammas, & Backgrounds Overview

Gamma-ray Large Area Space Telescope. Pass 6: GR V13R9 Muons, All Gammas, & Backgrounds Overview. Bill Atwood SCIPP/UCSC. Data Sets: Muons: allMuon-GR-v13r9 (14- Jan-2008) AG: allGamma-GR-v13r9 (14-Jan-2008)

247 views • 19 slides

Pass 6: Event Classes

Pass 6: Event Classes. The final chapter. Working Definitions TRANSIENT : E > 100 MeV ~ 2 Hz. Maximize Aeff at low energy SOURCE : E> 100 MeV ~ .4 Hz. Maximize Aeff 500 MeV - 10 GeV DIFFUSE : E> 100 MeV ~ .1 Hz. Minimize High energy tail > 10 GeV.

255 views • 17 slides

Performance of a Magnetised Scintillating Detector for a Neutrino Factory

Performance of a Magnetised Scintillating Detector for a Neutrino Factory. Scoping Study Meeting U.C. Irvine Monday 21 st August 2006 M. Ellis & A. Bross. Outline. Detector description Simulation Digitisation Data Set Reconstruction Performance: Reconstruction efficiency

308 views • 17 slides

Radiation Damage Studies for Si Diode Sensors Subject to MRaD Doses

Radiation Damage Studies for Si Diode Sensors Subject to MRaD Doses. Bruce Schum UC Santa Cruz June 26 2013. The Issue: ILC BeamCal Radiation Exposure. ILC BeamCal: Covers between 5 and 40 miliradians Radiation doses up to 100 MRad per year

344 views • 17 slides

ILC Technical Highlights

ILC Technical Highlights. Superconducting RF Main Linac. Parametric Approach. A working space - optimize machine for cost/performance. The Baseline Machine (500GeV). ~30 km. ML ~10km (G = 31.5MV/m). 20mr. RTML ~1.6km. 2mr. BDS 5km. e+ undulator @ 150 GeV (~1.2km). x2. R = 955m

225 views • 15 slides

Missing E T & Data Quality

276 views • 15 slides

Forward end-cap challenges

175 views • 7 slides

Rad. Bhabha: generator level

132 views • 4 slides

I. Evidence for energy release in the Galactic center:

De-Excitation Gamma-ray Line Emission from the Galactic Center . D.O. Chernyshov (MIPT), V.A. Dogiel (FIAN/ISAS), V. Tatischeff (CNRS), K.-S. Cheng (HKU), C.-M. Ko (NCU), W.H. Ip (NCU). II. Energy source in the Galactic center

163 views • 1 slides