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RINGO on the Liverpool Telescope has now measured the optical polarization ofGRB 060418 (where a 2 sigma upper limit of P<8% was determined) and GRB 090102(when a detection of P = 10 +/-1 % was made). We discuss the implications ofthese observations for the various competing models of GRB jet magnetizationand describe a possible unified model that can explain both measurements.

Early time optical polarization of GRB Afterglows: GRB 060418 and GRB 090102