The continuum polarization observations, spread over a period from Oct
ober 1996 to May 1997, of the coma region of comet Hale Bopp are made
at various phase angles, varying from 17.1 to 47.4 degrees, using IAU/
IHW filter set. The linear polarization measured through 3650, 4845 an
d 6840 Angstrom bands shows stronger wavelength dependence as compared
to what is seen in comet Halley at similar phase angles. Comparisons
are made with Comet Halley polarization properties and it is inferred
that Comet Hale Bopp has smaller grains than those found for Comet Hal
ley. However, this comet shows similarity with Comet Halley so far as
the albedo of the grains is concerned. This comet appears to belong to
the high polarization class in the classification scheme based on pol
arization characteristics.