It consists of the assembly of 60 30-seconds CCD pictures taken between 10m35m UT and 21h10m UT of February 18th 1999. At this moment the comet was about 11mag bright. I registered the images on the comet's head during the processing procedure. A logarithm filter was used in order to enhance the soft luminosity of the tail.
North is up ,East is left.
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