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Figure IDL save files
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 -
Figure IDL files
IDL files required to recreate the figures using the data files added. -
Fine Scale Structure in Cometary Dust Tails - Figure 5.2a - C/2011 L4 as seen...
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). -
Fine Scale Structure in Cometary Dust Tails - Figure 5.3a - C/2011 L4 as seen...
Views of C/2011 L4 Pan-STARRS from STEREO-B HI-1, enhanced as temporal difference images, using a scale with a wide dynamic range. The sun is centre below relative to all images... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.2b - C/2011 L4 as seen...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.7 - Temporal map seque...
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.... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.11 - Temporal Map sequ...
A sequence of 117 temporal maps, with fine-scale difference enhancement, C/2011 L4's clumpy tail region. The tail is shown from 2013 March 13 00:00 UT until March 16 12:00 UT.... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.8 - Temporal map seque...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.9, 5.10 -Temporal map ...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.18 - Sunward aligned t...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.24 - Solar Wind adjust...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.2a, 6.2b - C/2002 V1 a...
Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter. -
Fine Scale Structure in Cometary Dust Tails - Figure 5.19 - Sunward aligned t...
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 =... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.23 - Solar Wind adjust...
Three solar wind aligned temporal maps of McNaught's main dust tail region as seen by HI-1A with MGN enhancement.The x-axis corresponds to the paths through the comet tail taken... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.6 - Temporal maps of C...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.5 - Radial view of C/2...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.2e, 6.2f, 6.3a - C/200...
Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter, enhanced as temporal difference images. -
Fine Scale Structure in Cometary Dust Tails - Figure 6.2c, 6.2d, 6.3b - C/200...
Views of C/2002 V1 NEAT from SOHO LASCO C3, using the clear filter, with Multiscale Gaussian Normalisation enhancement. -
Fine Scale Structure in Cometary Dust Tails - Figure 6.11 - Sunward aligned t...
Sunward aligned temporal maps of C/2002 V1's dust tail as seen by LASCO C3 (clear filter) with MGN enhancement, showing the effects of increased solar wind dynamic pressure of... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.8 - Sunward aligned te...
A sequences of 70 sunward aligned temporal maps of C/2002 V1's main dust tail created from the SOHO LASCO C3 clear filter data using MGN enhancement.These are the same temporal...
