29 datasets found

Three temporal maps of the bright stria in C/2002 V1's dust tail as seen by LASCO C3.The tail is shown from 2003 February 18th at 07:54 UT until February 19th 04:54 UT. Dust is...

These files contain the raw code used to produce simulated image data for the following PhD thesis:Brydon, G., 2021, 'Spin Scanning Cameras for Planetary Exploration: Imager...

Three temporal maps showing how the localised density enhancement model compares to observations of the bright stria in C/2002 V1's dust tail as seen by LASCO C3 clear with MGN...

Sunward-aligned temporal maps of C/2011 L4's main dust tail region as seen by HI-1B with coarse-scale difference enhancement.Two points of note in the tail are points P (βr =...

Three sunward aligned maps of C/2002 V1's simulated dust tail position as seen by LASCO C3, showing the effects of increased solar wind dynamic pressure of varying strength.Dust...

Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter.

Views of C/2002 V1 NEAT from SOHO LASCO C3, taken with the clear filter and enhanced as temporal difference images.The field of view of the instrument has been projected into...

Three solar wind aligned temporal maps of C/2011 L4's main dust tail region as seen by HI-1B with coarse-scale difference enhancement. The x-axis corresponds to the paths...

View of C/2011 L4 Pan-STARRS from STEREO-B HI-1. The sun is centre below relative to all images (rotated 90 degrees counter-clockwise and flipped from nominal orientation).