2026-05-15T14:53:56Z https://api.figshare.com/v2/oai
oai:figshare.com:article/17082305 2021-12-07T15:26:03Z category_30091 category_30106 category_30259 category_30265 category_30109 portal_549 item_type_2 month_year_12_2021
10.5522/04/17082305.v1 https://figshare.com/articles/media/Fine_Scale_Structure_in_Cometary_Dust_Tails_-_Figure_6_11_-_Sunward_aligned_temporal_maps_of_C_2002_V1_showing_tracked_striae_with_and_without_modelled_CME_interaction_from_C3_Clear_images_with_MGN_enhancement_/17082305 https://ndownloader.figshare.com/files/31585070 Price, Oliver Oliver Price Jones, Geraint Geraint Jones <![CDATA[Fine Scale Structure in Cometary Dust Tails - Figure 6.11 - Sunward aligned temporal maps of C/2002 V1 showing tracked striae with and without modelled CME interaction (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 expected positions of striae under normal Finson Probstein physics have been tracked and are shown in cyan. Their expected positions calculated through enhanced Finson Probstein modelling of CMEs with various multiplier values are shown in magenta.

The CME model only causes significant deviation in expected striae behaviour where the Finson Probstein multiplier is at least one order of magnitude greater than unity.
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