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Fine Scale Structure in Cometary Dust Tails - Figure 5.2b - C/2011 L4 as seen by the STEREO-B HI-1 instrument (MGN)

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posted on 2021-12-07, 15:12 authored by Oliver Price, Geraint JonesGeraint Jones

Views of C/2011 L4 Pan-STARRS from STEREO-B HI-1, with Multiscale Gaussian Normalisation enhancement. The sun is centre below relative to all images (rotated 90$ degrees counter-clockwise and flipped from nominal orientation).

Fine Scale Structure in Cometary Dust Tails - Figure 5.2b - C/2011 L4 as seen by the STEREO-B HI-1 instrument (MGN)

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

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