2026-05-14T09:01:21Z https://api.figshare.com/v2/oai
oai:figshare.com:article/17082203 2021-12-07T15:25:16Z category_30091 category_30106 category_30259 category_30265 category_30109 portal_549 item_type_2 month_year_12_2021
10.5522/04/17082203.v1 https://figshare.com/articles/media/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/17082203 https://ndownloader.figshare.com/files/31584956 Price, Oliver Oliver Price Jones, Geraint Geraint Jones <![CDATA[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]]> Astronomical instrumentation Planetary science (excl. solar system and planetary geology) Solar system planetary science (excl. planetary geology) Space sciences not elsewhere classified Solar physics Comet Dust Tail Finson Probstein Solar Wind Plasma NEAT C/2002 V1 CME Filament Instrumentation, Techniques, and Astronomical Observations Planetary Science Planetary Science (excl. Extraterrestrial Geology) Solar System, Solar Physics, Planets and Exoplanets Space Science Space and Solar Physics 2021-12-07 2021-12-07 Media 2021 University College London
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.
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