The polarization evolution of the optical afterglow of GRB 030329

A.A. Kaas; A. Henden; A. Kaufer; A. Rau; B. Stecklum; C. Kouveliotou; C. Ries; C. Straubmeier; D.H. Hartmann; E. Jehin

arxiv: astro-ph/0312089 · v1 · submitted 2003-12-03 · 🌌 astro-ph

The polarization evolution of the optical afterglow of GRB 030329

J. Greiner , S. Klose , K. Reinsch , H.M. Schmid , R. Sari , D.H. Hartmann , C. Kouveliotou , A. Rau

show 18 more authors

E. Palazzi C. Straubmeier B. Stecklum S. Zharikov G. Tovmassian O. Barnbantner C. Ries E. Jehin A. Henden A.A. Kaas T. Grav J. Hjorth H. Pedersen R.A.M.J. Wijers A. Kaufer H.-S. Park G. Williams O. Reimer

This is my paper

classification 🌌 astro-ph

keywords afterglowhighcoherencedataevolutionfieldfrequencygenerated

0 comments

read the original abstract

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.

This paper has not been read by Pith yet.

The polarization evolution of the optical afterglow of GRB 030329

discussion (0)