2026-05-07T12:47:25Z https://api.figshare.com/v2/oai
oai:figshare.com:article/17082200 2021-12-07T15:25:28Z category_30091 category_30106 category_30259 category_30265 category_30109 portal_549 item_type_2 month_year_12_2021
10.5522/04/17082200.v1 https://figshare.com/articles/media/Fine_Scale_Structure_in_Cometary_Dust_Tails_-_Figure_6_5_-_Radial_view_of_C_2002_V1_getting_hit_by_a_CME_as_seen_by_SOHO_LASCO_C3_with_difference_enhancement_/17082200 https://ndownloader.figshare.com/files/31584953 Price, Oliver Oliver Price Jones, Geraint Geraint Jones <![CDATA[Fine Scale Structure in Cometary Dust Tails - Figure 6.5 - Radial view of C/2002 V1 getting hit by a CME (as seen by SOHO LASCO C3 with difference 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 field of view of the instrument has been projected into the orbital plane of the comet, where it is shown in an unravelled radial plot. Phase angle isolines are also shown.

The CME hits the comet and its dust tail at a phase angle of between 80 and 85 degrees, close to the limb where the filament eruption was observed.
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