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Fine Scale Structure in Cometary Dust Tails - Figure 5.3a - C/2011 L4 as seen by the STEREO-B HI-1 instrument (coarse scale difference images)

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posted on 07.12.2021, 13:42 by Oliver Price, Geraint JonesGeraint Jones
Views of C/2011 L4 Pan-STARRS from STEREO-B HI-1, enhanced as temporal difference images, using a scale with a wide dynamic range. The sun is centre below relative to all images (rotated 90$ degrees counter-clockwise and flipped from nominal orientation).


This research was supported by a UK Science and Technology Facilities Council (STFC) PhD studentship.