Fine Scale Structure in Cometary Dust Tails - Figure 5.18 - Sunward aligned temporal maps of McNaught as seen by HI-1A with MGN enhancement

DOI

Sunward-aligned temporal maps of McNaught's main dust tail region as seen by HI-1A with MGN enhancement.After a 6 hour data gap, on 22:01 UT on January 12th 2007, new near vertical combed features are visible which intersect older striae. Note that features on the far left of the temporal maps are artefacts from the overexposed region near the comet's nucleus.

Identifier
DOI https://doi.org/10.5522/04/17082149.v1
Related Identifier https://ndownloader.figshare.com/files/31584893
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17082149
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