Fine Scale Structure in Cometary Dust Tails - Figure 5.12 - Temporal Map sequence of C/2011 L4's iron tail region as seen by HI-1B with fine-scale difference enhancement

DOI

A sequence of 211 temporal maps, with fine-scale difference enhancement, showing C/2011 L4's short straight tail. The tail is shown from 2013 March 10 04:50 UT until March 16 12:00 UT. Dust is displayed in the region of of 10 < βr < 300. The short extent of this tail means that displaying dust on an axis with fixed ejection time and date proves unsuitable. Dust is therefore shown over a fixed range of ages for each image, i.e. when dust was between 0.1 and 2 days old. As such, the dates and times on the axis are not constant, and fixed points with a specific βr and te move along the axis at the same rate as the cadence of images.

Identifier
DOI https://doi.org/10.5522/04/17082062.v1
Related Identifier https://ndownloader.figshare.com/files/31584743
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17082062
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