Electron acceleration by young supernova remnant blast waves

Details Electron acceleration by young supernova remnant blast waves Electron acceleration by young supernova remnant blast waves

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..430b&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

Physics

2

Electron Acceleration, Galactic Cosmic Rays, Magnetohydrodynamic Stability, Relativistic Particles, Shock Wave Interaction, Supernova Remnants, Blasts, Cosmic Plasma, Radio Observation

Scientific paper

Some general considerations regarding relativistic particle acceleration by young supernova remnants are reviewed. Recent radio observations of supernova remnants apparently locate the bounding shock and exhibit large electron density gradients which verify the presence of strong particle scattering. The radio 'rim' in Tycho's remnant has been found to contain a predominantly radial magnetic field. This may be attributable to an instability of the shock surface and a progress report on an investigation of the stability of strong shocks in partially ionized media is presented.

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