Fig. 7
Dust surface brightness profiles B as a function of projected cometocentric distance ρ in double logarithmic representation, obtained from the spectroscopic measurements on October 27 and 29, 2010 in the ~ tailwards (red crosses) – sunward (black open circles) directions. The selected continuum region is 482–485 nm. Symbols refer to the observational data and a solid line refers to the linear fit.
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