activity
19992017
most citedCosmic ray acceleration at perpendicular shocks in supernova remnants

48 citations · 123 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2017★ 24 cited

WOMBAT: A Scalable and High Performance Astrophysical MHD Code

Peter Mendygral, Nick Radcliffe, Krishna Kandalla +6

We present a new code for astrophysical magneto-hydrodynamics specifically designed and optimized for high performance and scaling on modern and future supercomputers. We describe…

astro-ph.HE2014★ 48 cited

Cosmic ray acceleration at perpendicular shocks in supernova remnants

Gilles Ferrand, Rebecca J. Danos, Andreas Shalchi +3

Supernova remnants (SNRs) are believed to accelerate particles up to high energies through the mechanism of diffusive shock acceleration (DSA). Except for direct plasma simulations…

astro-ph.HE2013★ 27 cited

Nonthermal Radiation from Supernova Remnants: Effects of Magnetic Field Amplification and Particle Escape

Hyesung Kang, T. W. Jones, Paul P. Edmon

We explore nonlinear effects of wave-particle interactions on the diffusive shock acceleration (DSA) process in Type Ia-like, SNR blast waves, by implementing phenomenological mode…

astro-ph.HE2011★ 20 cited

Nonthermal Radiation from Type Ia Supernova Remnants

Paul P. Edmon, Hyesung Kang, T. W. Jones +1

We present calculations of expected continuum emissions from Sedov-Taylor phase Type Ia supernova remnants (SNRs), using the energy spectra of cosmic ray (CR) electrons and protons…

astro-ph2007★ 2 cited

Time Evolution of Cosmic Ray MHD Shocks and Their Emissions

P. P. Edmon, T. W. Jones, H. Kang

We present results of time evolution of oblique MHD plane shocks including diffusive cosmic ray acceleration with backreaction on the plasma flows. The simulations include self-con…

astro-ph1999★ 2 cited

The Washington Large Area Time Coincidence Array

J. G. Cramer, S. R. Elliott, J. F. Wilkerson +2

The number and density of schools in the Seattle area is convenient for the study of distributed particle showers produced at the top of the atmosphere by ultra-high energy (about…