The impact sites are still quite distinct, although they have begun to spread in longitude. The table contains a listing site identifications visible from east to west in each set of images. In some cases sites that were separate in the center of the disk are combined due to foreshortening when near the limb. We plan to continue infrared monitoring of the impact sites until Jupiter becomes inaccessible. Here is a UNIX compressed tar archive of all Whately Observatory observations during Summer 1994, whately.logs.Z , and here is a typical fits image, image.fits .
Considerable structure is visible in the diffused debris from the impacts.
Observers were Mike Skrutskie and David Morris from the University of Massachusetts and Kester Allen from Amherst College. Click here for a plethora of general information about the comet impacts.