Fine Scale Structure in Cometary Dust Tails - Figure 6.6 - Temporal maps of C/2002 V1's dust tail from C3 Clear images with MGN enhancement
A sequences of 70 temporal maps of C/2002 V1's main dust tail created from the SOHO LASCO C3 clear filter data using MGN enhancement.<div><br></div><div>The tail is shown from 2003 February 16th at 18:54 UT until February 19th 17:54 UT. Dust is displayed from the region of 0.2 < <b>β<sub>r</sub></b> < 2.5 with ejection times from 2003 February 14th 00:00 UT through to February 18th 00:00 UT.</div><div><br></div><div>The CME passes through the tail at around 08:54 UT on February 18th. Eight hours later, the oldest dust in the tail is barely visible, and a new prominent stria feature has formed.<br></div>
