Polarization studies of comet C/2000 WM1 (LINEAR)

Observatory during November 2001 and March 2002. The observations in November were at low phase angle ( < 22(degree)) when the polarization is negative and where the data for most of the comets are rather meager. The observations during March were made when the phase angle was ~47(degree). Observations were conducted through the IHW narrow band and BVR broad band filters. Based on these polarization observations we infer that the comet C/2000 WM1 belongs to high polarization class i.e. the dusty comet family.