31 datasets found

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).

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...

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...

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

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...

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 =...

File size: 6 kB File format: Plain Text Using observations of the Sym-H index, the dataset provides the date and time for the start of the initial phase, start of the main...

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...

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...

A sequence of 235 temporal maps, with coarse-scale difference enhancement (i.e. using temporal difference images with a narrow dynamic range). This shows the main dust tail of...

Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter, enhanced as temporal difference images.

A sequence of images extracted from the STEREO-B HI-1 view of C/2011 L4, using coarse scale difference images. The breakup of a stria early on the 14th march is shown, centred...

A collection of IDL save files for creating the paper figures entitled Fine structure of type III solar radio bursts from Langmuir wave motion in turbulent plasma

A sequence of 275 temporal maps of C/2011 L4's dust tail with MGN enhancement. This shows the main dust tail of C/2011 L4 from 2013 March 10 00:00 UT until March 18 00:00 UT....

A sequences of 70 temporal maps of C/2002 V1's main dust tail created from the SOHO LASCO C3 clear filter data, enhanced as temporal difference images.The tail is shown from...

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.The tail is shown from 2003 February 16th at...

Sunward-aligned temporal maps of McNaught's main dust tail region as seen by HI-1A with MGN enhancement.After a 6 hour data gap, on 22:01 UT on January 12th 2007, new near...

A sequence of images extracted from the STEREO-B HI-1 view of C/2011 L4, using coarse scale difference images. The breakup of a stria early on the 14th march is shown, centred...

Views of C/2011 L4 Pan-STARRS from STEREO-B HI-1, with Multiscale Gaussian Normalisation enhancement. The sun is centre below relative to all images (rotated 90$ degrees...

IDL files required to recreate the figures using the data files added.