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ICEFLUX allometric measurements of polar zooplankton and fish
This dataset summarizes allometric measurements on zooplankton and nekton species performed in the framework of the Dutch and German ICEFLUX projects. Measurements were... -
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... -
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...
