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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 5.3a - 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 6.14 - Localised high de...
View 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 the... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.9 - CME shell model sh...
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 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 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 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 5.3b - 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 narrow dynamic range. The sun is centre below relative to all... -
Fine Scale Structure in Cometary Dust Tails - Figure 5.12 - Temporal Map sequ...
A sequence of 211 temporal maps, with fine-scale difference enhancement, showing C/2011 L4's short straight tail. The tail is shown from 2013 March 10 04:50 UT until March 16... -
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. -
van der Pauw and Hall effect data for high conductive and transparent zinc ox...
This data set includes transport measurements data of zinc oxide (ZnO) and indium tin oxide (ITO) thin films. The measurements were done using the van der Pauw / Hall effect... -
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...
