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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... -
Morphometric traits of birds on Kilimanjaro
This dataset includes morphological trait measurements of all bird species recorded on the study sites of Mt. Kilimanjaro. We measured traits related to the size of birds, as... -
Shear Stability of Emulsions in the Presence of Co-Surfactants with Various C...
High internal phase aqueous-in-oil emulsions prepared by oil-soluble polyisobutylenesuccinicanhydride (PIBSA) with a water-soluble co-surfactant n-alkylpolyacrylamide (PAM)... -
Magnetic interactions in honeycomb iridates Na2IrO3
We propose to study the magnetic excitation spectrum of Na2IrO3 with inelastic neutron scattering. Na2IrO3 is a promising candidate to realize Kitaev interaction. By mapping out... -
Understanding the Affect of Lipid Tail Saturation on Anaesthetic Interaction ...
The mechanism of general anaesthetic action is poorly understood despite their widespread use. It is hoped that investigating the interaction of anaesthetics with lipid bilayers... -
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 5.24 - 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 6.5 - 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 6.2a, 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 6.12 - Sunward aligned m...
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... -
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 6.15a - Temporal maps of...
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... -
Fine Scale Structure in Cometary Dust Tails - Figure 6.15b - Temporal maps of...
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... -
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 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 5.15 - Stria breaking up...
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... -
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 6.7 - 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, enhanced as temporal difference images.The tail is shown from... -
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 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...