Fine Scale Structure in Cometary Dust Tails - Figure 5.8 - Temporal map sequence of C/2011 L4 dust tail as seen by HI-1B with fine-scale difference enhancement
mediaposted on 2021-12-07, 15:13 authored by Oliver Price, Geraint JonesGeraint Jones
A sequence of 235 temporal maps, with a fine-scale difference enhancement (i.e. using temporal difference images with a wide dynamic range). This shows the main dust tail of C/2011 L4 from 2013 March 11 00:00 UT until March 18 02:00 UT. Dust is displayed from the region of 0.3 < βr < 3 with a range of ejection times from 2013 March 01 00:00 UT through to March 13 00:00 UT.
This research was supported by a UK Science and Technology Facilities Council (STFC) PhD studentship.
I confirm that I am not uploading any: personal data as defined by data protection legislation, including information that may identify a living individual; information provided in confidence; or information that would contravene a third-party agreement
I have considered whether the data to be published may be licensed commercially before deciding to freely release it to the public. Further information and advice may be sought from UCL Business https://www.uclb.com/about/our-people/