Should be quite an improvement over the 400 ISO film. HB was obvious to the unaided eye as an oblong hazy patch with a stellar core. I found HB to be about 2.2 mag. The parabolic hood was very distinct. Several knots were apparent, with a bright knot to the north side of this formation.
Jets continue to be active.
The jet at PA 10deg. There was much activity between PA 120deg and 200deg. Jet at PA 220 bent sharply away from the coma, flowing directly into the southern tail ribbon. It was straddled by the north and south tail segments. Cranked out a number of hours doing meteors, grabbed a nap, then got up for the comet.