Fine Scale Structure in Cometary Dust Tails - Figure 6.7 - Temporal maps of C/2002 V1's dust tail from C3 Clear images with difference enhancement

DOI

A sequences of 70 temporal maps of C/2002 V1's main dust tail created from the SOHO LASCO C3 clear filter data, enhanced as temporal difference images.The tail is shown from 2003 February 16th at 18:54 UT until February 19th 17:54 UT. Dust is displayed from the region of 0.2 < βr < 2.5 with ejection times from 2003 February 14th 00:00 UT through to February 18th 00:00 UT.The CME passes through the tail at around 08:54 UT on February 18th. Eight hours later, the oldest dust in the tail has decreased in brightness, although in these difference image temporal maps, some structure can still be discerned.

Identifier
DOI https://doi.org/10.5522/04/17082227.v1
Related Identifier https://ndownloader.figshare.com/files/31584989
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17082227
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