Observational signatures of sub-Larmor scale magnetic fields in astrophysical objects and HEAD lab experiments

Details Observational signatures of sub-Larmor scale magnetic fields in astrophysical objects and HEAD lab experiments Observational signatures of sub-Larmor scale magnetic fields in astrophysical objects and HEAD lab experiments

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..aprq10005m&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #Q10.005

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Scientific paper

An extensive body of studies indicate that small-scale (sub-Larmor-scale) magnetic turbulence are produced at relativistic shocks, in reconnection events and other high-energy density environments. Here we present a general description of radiation produced by relativistic electrons moving in such fields and stress its non-synchrotron spectral characteristics. We illustrate the results with spectral data from gamma-ray burst observations. )

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