'Capture efficiency' presentation slideshows

616 views • 44 slides

RF capture of KURRI FFAG Main Ring

RF capture of KURRI FFAG Main Ring. 2011.09.15 T. Uesugi, Y. Ishi, Y. Kuriyama, J-B. Lagrange, Y. Mori, R. Nakano, B. Qin, E. Yamawa (KURRI), Y. Niwa, K. Okabe, I. Sakai (Fukui-univ). === Introduction ===. Charge-exchange multi-turn injection without Bump-magnets.

560 views • 42 slides

How to Calculate Your Emissions

526 views • 41 slides

Polarized Positrons for Future Linear Colliders

Polarized Positrons for Future Linear Colliders. Sabine Riemann, DESY Zeuthen Thanks to the members of the ILC/CLIC Positron Source Group High precision measurements of luminosity at future linear colliders and polarization of lepton beams October 3-5, 2010. Outline.

456 views • 34 slides

Gaseous And Particulate Dispersion In Street Canyons

Gaseous And Particulate Dispersion In Street Canyons. Kambiz Nazridoust Department of Mechanical and Aeronautical Engineering Clarkson University, Potsdam, NY 13699-5725. Objectives.

408 views • 29 slides

e + ??????

e + ??????. ??? GDE meeting ????. ?? GDE ????? 2008 ? 10 ? 6 ?. ?? GDE ????? 2008 ? 6 ? 23 ?. ?????????????????????? "2nd Asia ILC R&D Seminar, Sep 29-30, 2008" ???????????????????. Working Groups and Conveners ILC08 - Accelerator 1. Sources Axel Brachmann, Jim Clarke.

406 views • 27 slides

HALO - a Helium and Lead Observatory

HALO - a Helium and Lead Observatory. Outline Overview Motivation / Physics SNEWS Signal and Backgrounds Monte Carlo studies Further Work. Use materials on hand (Phase 1) 80 tonnes of Pb from decommissioned Deep River Cosmic-ray station

285 views • 21 slides

Jeff Dooling Presented at The Ninth

Second Harmonic capture in the IPNS RCS: Transition from SH to fundamental rf operation during the acceleration cycle using CAPTURE_SPC. Jeff Dooling Presented at The Ninth Second Harmonic RF/Low Output-Impedance Amplifier Collaboration Meeting Argonne National Laboratory, June 14-15, 2004.

336 views • 20 slides

HALO - a Helium and Lead Observatory

HALO - a Helium and Lead Observatory. Outline Overview Motivation / Physics SNEWS Signal and Backgrounds Monte Carlo studies Further Work. Use materials on hand 80 tonnes of Pb from decommissioned Chalk River Cosmic-ray station 3 He proportional counter neutron detectors To produce a

268 views • 20 slides

Motoi Tachibana (Saga Univ.)

Dark matter capture in n eutron stars with exotic phases. Dark matter capture in n eutron stars -stellar constraints on dark matter-. Motoi Tachibana (Saga Univ.). Oct. 25, 2013 ? NS matter symposium, Kyoto . Why their connections?

281 views • 17 slides

Capture Efficiency vs Spot Size

Capture Efficiency vs Spot Size. Wanming Liu, Wei Gai ANL Aug 15, 2007. Conditions. 100m undulator, K=0.92, l u=1.15cm Target: Ti, 0.4 rl Drift to target: from 450m up to 700m(spot size: 1.5mm up to 2.3mm) Immersed case: 6T-0.5T, 20cm Non Immersed case: ramp(0-6T) 2cm, 6T-0.5T 20cm

127 views • 3 slides

110 views • 2 slides