Fine Scale Structure in Cometary Dust Tails - Figure 6.6 - Temporal maps of C/2002 V1's dust tail from C3 Clear images with MGN 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 using MGN enhancement.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 is barely visible, and a new prominent stria feature has formed.

Identifier
DOI https://doi.org/10.5522/04/17082203.v1
Related Identifier https://ndownloader.figshare.com/files/31584956
Metadata Access https://api.figshare.com/v2/oai?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:figshare.com:article/17082203
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