Observations made by the Cassini spacecraft at the bow shock of Saturn suggest that electrons are likely to be accelerated to near-relativistic energies by strong astrophysical shocks.
References
Blandford, R. & Eichler, D. Phys. Rep. 154, 1–75 (1987).
Lee, M. A. AIP Conf. Proc. 528, 3–18, (2000).
Masters, A. et al. Nature Phys. 9, 164–167, (2013).
Fermi, E. Phys. Rev. 75, 1169–1174 (1949).
Ball, L. & Melrose, D. B. Publ. Astron. Soc. Aust. 18, 361–373 (2001).
Guo, F. & Giacalone, J. Astrophys. J. 715, 406–411 (2010).
Armstrong, T., Pesses, M. E. & Decker, R. B. in Collisionless Shocks in the Heliosphere: Reviews of Current Research (eds. Tsurutani, B. T. & Stone, R. G.) 271–285 (Geophysical Monograph Series 35, American Geophysical Union, 1985).
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Richardson, I. An unexpected shock. Nature Phys 9, 131–132 (2013). https://doi.org/10.1038/nphys2565
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DOI: https://doi.org/10.1038/nphys2565
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