<![CDATA[Fine Scale Structure in Cometary Dust Tails - Figure 5.9, 5.10 -Temporal map sequence of C/2011 L4 dust tail as seen by HI-1B with coarse-scale difference enhancement]]>

2026-05-06T23:49:23Z https://api.figshare.com/v2/oai

oai:figshare.com:article/17082038 2021-12-07T15:13:58Z category_30091 category_30106 category_30259 category_30265 category_30109 portal_549 item_type_2 month_year_12_2021

10.5522/04/17082038.v1 https://figshare.com/articles/media/Fine_Scale_Structure_in_Cometary_Dust_Tails_-_Figure_5_9_5_10_-Temporal_map_sequence_of_C_2011_L4_dust_tail_as_seen_by_HI-1B_with_coarse-scale_difference_enhancement/17082038 https://ndownloader.figshare.com/files/31584698 Price, Oliver Oliver Price Jones, Geraint Geraint Jones <![CDATA[Fine Scale Structure in Cometary Dust Tails - Figure 5.9, 5.10 -Temporal map sequence of C/2011 L4 dust tail as seen by HI-1B with coarse-scale 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 HCS C/2011 L4 Pan-STARRS 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 β_r < 3 with ejection times from 2013 March 05 00:00 UT through to March 11 00:00 UT.

Highlighted are two dust points which the analysis later focuses on. Point P is highlighted in purple with β_r = 1.7 and t_e = 2013-03-08 04:50 UT. Point G is highlighted in green with β_r = 0.8 and t_e = 2013-03-05 12:00 UT.

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