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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 5.9, 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 6.15b - 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 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 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 6.12 - 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 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 6.5 - 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 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 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). -
(Table T1) Sedimentation rate, bulk density and mass accumulation rate of ODP...
Ocean Drilling Program Leg 198 Site 1208 is located on the Central High of Shatsky Rise (36°7.6301'N, 158°12.0952'E) in the North Pacific Ocean at a water depth of 3346 m. A... -
(Table 1) Mass-accumulation rates for the non-authigenic, inorganic, crystall...
Elevated regions in the central parts of ocean basins are excellent for study of accumulation of eolian material. The mass-accumulation rates of this sediment component appear... -
Chemistry, dust and pollen analysis of ice core VAV88
This dataset has no description
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(Table 1) Eolian mass accumulation rates of sediment core KODOS_02_01_02 in t...
This dataset has no description
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(Table T2) Terrigenous grain-size median and mode and percent eolian of ODP L...
This dataset has no description
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EDC dust flux 800 kyr (25 yr mean)
The file "EDC_DustFlux_25yr.dat" contains the 25-year constant time-step averages of the high-resolution 1cm data, averages being made of many data-points at the top, but only... -
EDC dust flux 800 kyr (full resolution)
The file "EDC_DustFlux_1cm.dat" contains the principal component (EOF1) of the high-resolution calcium, non-sea-salt calcium, and insoluble dust records from the EPICA Dome C... -
EDC calcium and dust concentrations
The file "EDC_CaDustConc_1cm.dat" contains the EPICA Dome C Calcium (in ppb), insoluble dust (in P/ml), and non-sea-salt Calcium (in ppb) on depth and EDC3 age scale. Note that... -
(Table 4) Weight percentage, accumulation rate, and size of eolian materials ...
Sediment depth is given in mbsf. Age interpolated from age and LSR values in Table 2 -
(Table 1) Mass-accumulation rates for the non-authigenic, inorganic, crystall...
Sediment depth is given in mbsf. Empty cells mean no data. Rates for sediments below Core 5, Section 2 (the brown clays) are uncertain.
