Magnetic Field Configurations in SN 1006 NE Rim

Details Magnetic Field Configurations in SN 1006 NE Rim Magnetic Field Configurations in SN 1006 NE Rim

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2417y&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Characteristic scale lengths of nonthermal X-rays from the SN 1006 NE rim, which are observed by Chandra, are interpreted in the context of the diffusive shock acceleration on the assumption that the observed spatial profile of nonthermal X-rays corresp onds to that of accelerated electrons with energy a few tens of TeV. To explain observed scale lengths, we construct two simple models with a test particle approximation, the age-limited and the energy loss-limited model, and discuss the condition that the magnetic field configuration or the diffusion coefficients of accelerated electrons should satisfy.

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