'Magnetic field configuration' diaporamas de présentation

Long-range c orrelations in driven systems David Mukamel

Long-range c orrelations in driven systems David Mukamel. Driven, non-equilibrium systems. s ystems with currents. d o not obey detailed balance. the probability to be at a microscopic configuration C at time t . heat current. T 1. T 2. T 1 >T 2. charge current. E.

658 views • 60 slides

Accelerator Physics: Synchrotron radiation

653 views • 42 slides

Pulsar timing noises as evidence of Hall drift and Hall Weves in crusts of isolated neutron stars

Pulsar timing noises as evidence of Hall drift and Hall Weves in crusts of isolated neutron stars. Speaker ? Yi Xie 2014-04-30 Lunch Talk. Pulsars: The Most Stable Rotators. Observed pulse series. Irregular Period Changes. Two Main Types of Irregularity ?

471 views • 36 slides

Constraints on X-ray polarization of synchrotron jets from stellar-mass BHs

Constraints on X-ray polarization of synchrotron jets from stellar-mass BHs. Dave Russell niversity of Amsterdam In collaboration with: Dipankar Maitra, Robert Dunn, Sera Markoff, Rob Fender, Fraser Lewis, Piergiorgio Casella, Peter Curran... and some results from a larger collaboration

230 views • 10 slides

C10 with different damping

C10 with different damping. Grudiev 23/10/2008. Radial Choke cell geometry. ~30mm. Two disks per cell are necessary to implement radial choke geometry. Electric field configuration. C10_vg1.16 WG damping. C10_vg1.35. C10_vg1.15 Radial Choke damping. Magnetic field configuration.

153 views • 7 slides