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

DOI

View of C/2011 L4 Pan-STARRS from STEREO-B HI-1. The sun is centre below relative to all images (rotated 90 degrees counter-clockwise and flipped from nominal orientation).

Identifier
DOI https://doi.org/10.5522/04/17081939.v1
Related Identifier https://ndownloader.figshare.com/files/31584605
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17081939
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