Diffusive electron acceleration at SNR shock fronts and the observed SNR radio spectral indices

Details Diffusive electron acceleration at SNR shock fronts and the observed SNR radio spectral indices Diffusive electron acceleration at SNR shock fronts and the observed SNR radio spectral indices

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icrc....9..543b&link_type=abstract

In NASA. Goddard Space Flight Center Nineteenth International Cosmic Ray Conference. Conference Papers: Invited Rapporteur, High

Physics

Cosmic Rays, Electron Acceleration, High Energy Electrons, Relativistic Particles, Shock Fronts, Supernova Remnants, Electron Energy, Energy Spectra, Interstellar Matter

Scientific paper

The radio synchrotron emission from relativistic electrons in shell supernova remnants (SNRs) provides a unique opportunity to probe the energy distribution of energetic electrons at their acceleration site (SNR shock fronts). This information provides insight into the acceleration mechanism(s). Here the authors discuss the implications of these observations for the diffusive (first-order Fermi) acceleration of electrons at the SNR shock fronts.

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