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(Table 1) Accumulation of opal and eaolian sediment in ODP Site 145-886
This dataset has no description
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(Table 1) Accumulation of opal and eaolian sediment in ODP Hole 145-885A
This dataset has no description
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Dust content in sediments of ODP Hole 108-659A in the North Atlantic
This dataset has no description
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(Table 4) Dust and opal content from DSDP Hole 68-503B
This dataset has no description
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(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... -
(Table 1) Age, porocity, density, mass accumulation rates and grain size of t...
Eolian dust preserved in deep-sea sediments provides a record of atmospheric circulation throughout geologic time. This eolian component has been isolated to determine its mass... -
(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 3) Aeolian component of North Pacific pelagic sediments
Isolation and analysis of the eolian component of late Cenozoic pelagic sediments from the North Pacific provides direct information concerning changes in atmospheric... -
Accumulation rates of Late Cretaceous eolian sediments in DSDP Hole 62-463 in...
Eolian dust preserved in deep-sea sediment can provide a direct historical record of global atmospheric circulation. Data from a reasonably complete Upper Cretaceous section of... -
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 =...
