The polarization evolution of the optical afterglow of GRB 030329

Details The polarization evolution of the optical afterglow of GRB 030329 The polarization evolution of the optical afterglow of GRB 030329

2003-12-03

arxiv.org/abs/astro-ph/0312089v1

Astronomy and Astrophysics

Astrophysics

2003 GRB Conference, Santa Fe, Oct. 2003, 1 ps-figure

Scientific paper

10.1063/1.1810845

We report 31 polarimetric observations of the afterglow of GRB 030329 with
high signal-to-noise and high sampling frequency. The data imply that the
afterglow magnetic field has small coherence length and is mostly random,
probably generated by turbulence.

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