'Mode amplitude' diaporamas de présentation

The Nonlinear Development of Instabilities in Rotating Stars and Binary Star Systems

387 views • 25 slides

Magnetic Steering and ECCD Mitigation of locked NTMs

Magnetic Steering and ECCD Mitigation of locked NTMs. Presented by Francesco Volpe In collaboration with: R.J. Buttery, R.J. La Haye, G. Jackson, M. Okabayashi, F.W. Perkins, R. Prater, H. Takahashi Acknowledgements to:

301 views • 22 slides

Energetic Particle Physics Progress and Plans

NSTX. Supported by. Energetic Particle Physics Progress and Plans. College W&M Colorado Sch Mines Columbia U CompX General Atomics INL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U Old Dominion U ORNL PPPL PSI Princeton U Purdue U SNL Think Tank, Inc.

319 views • 21 slides

Shu-Hua Yang ( ??? ) Hua Zhong Normal University

The role of r-mode damping in the thermal evoltion of neutron stars. Shu-Hua Yang ( ??? ) Hua Zhong Normal University. Outline. Introduction R-mode heating of neutron stars Our results. 1 ? Introduction. Yakovlev et al. (2008) , AIPC,983,379.

335 views • 20 slides

Coherent Synchro-Betatron Resonance in the FNAL Booster

Coherent Synchro-Betatron Resonance in the FNAL Booster. A. Burov, V. Lebedev. HB 2008. Booster. Booster is a fast cycling proton synchrotron operating at 15 Hz. Transverse Instability.

374 views • 18 slides

Longitudinal impedance identification

Longitudinal impedance identification. T. Argyropoulos, T. Bohl, J. E. Muller, H. Timko, E. Shaposhnikova Thanks to H. Damerau for preparing the beam LIU-SPS BD WG 30/08/2012. Motivation. The increase of the average bunch length of the batches along the flat bottom

180 views • 8 slides