2026-06-23T02:43:00Z https://api.figshare.com/v2/oai
oai:figshare.com:article/17082299 2021-12-07T15:27:30Z category_30091 category_30106 category_30259 category_30265 category_30109 portal_549 item_type_2 month_year_12_2021
10.5522/04/17082299.v1 https://figshare.com/articles/media/Fine_Scale_Structure_in_Cometary_Dust_Tails_-_Figure_6_9_-_CME_shell_model_showing_area_of_high_density_as_seen_by_C3_Clear_with_difference_enhancement_/17082299 https://ndownloader.figshare.com/files/31585067 Price, Oliver Oliver Price Jones, Geraint Geraint Jones <![CDATA[Fine Scale Structure in Cometary Dust Tails - Figure 6.9 - CME shell model showing area of high density (as seen by C3 Clear 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 shell of the CME has been modelled as an area of high density, outlined in green. Note that as the CME moves past the comet, it becomes much harder to keep track of the CME's leading edge.
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