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)

DOI

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).

Identifier
DOI https://doi.org/10.5522/04/17081996.v1
Related Identifier HasPart https://ndownloader.figshare.com/files/31584659
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17081996
Provenance
Creator Price, Oliver; Jones, Geraint
Publisher University College London UCL
Contributor Figshare
Publication Year 2021
Rights https://creativecommons.org/licenses/by/4.0/
OpenAccess true
Contact researchdatarepository(at)ucl.ac.uk
Representation
Language English
Resource Type Media; Audiovisual
Discipline Astrophysics and Astronomy; Geology; Geosciences; Geospheric Sciences; Natural Sciences; Physics; Solar Physics