Sediment Transport and Depositional Processes     

TIM Best 《Basin Research》1994,6(2-3):179-180

  相似文献   

Convective dispersion modelling utilising acoustic sounder information     

P.R. Best  M. Kanowski  L. Stmer  D. Green 《Atmospheric Research》1986,20(2-4)

  相似文献   

Test of IGRF (1980) main field and secular variation in Europe     

W. Mundt  E. Ritter  A. Best 《Physics of the Earth and Planetary Interiors》1985,37(1):20-24

The IGRF-models for the main field and the secular variation (IGRF 1980 and IGRF-SV 1980–1985) have been compared with geomagnetic ground based data for epoch 1980.5 in the GDR, and also with the secular variation at 34 European observatories. The results for the main magnetic field were much better than for IGRF 1965. With a level-error of ～ 45 nT, the IGRF 1980 included ～ 75% of the magnetic crust field. The structure of the IGRF-field is similar to that of other regional reference fields.The IGRF-SV for 1965, 1975 and 1980–1985 have been compared with analytical SV-models, based on low-degree polynomial approximations. It is shown that the main features of SV in Europe are represented correctly. The mean differences between observatory data and IGRF-SV 1980–1985 are 1.5′/a for declination, and 7 nT/a for total intensity.  相似文献   

Form roughness and the absence of secondary flow in a large confluence–diffluence,Rio Paraná, Argentina     

Daniel R. Parsons  James L. Best  Stuart N. Lane  Oscar Orfeo  Richard J. Hardy  Ray Kostaschuk 《地球表面变化过程与地形》2007,32(1):155-162

Confluence–diffluence units are key elements within many river networks, having a major impact upon the routing of flow and sediment, and hence upon channel change. Although much progress has been made in understanding river confluences, and increasing attention is being paid to bifurcations and the important role of bifurcation asymmetry, most studies have been conducted in laboratory flumes or within small rivers with width:depth (aspect) ratios less than 50. This paper presents results of a field‐based study that details the bed morphology and 3D flow structure within a very large confluence–diffluence in the Río Paraná, Argentina, with a width:depth ratio of approximately 200. Flow within the confluence–diffluence is dominated largely by the bed roughness, in the form of sand dunes; coherent, channel‐scale, secondary flow cells, that have been identified as important aspects of the flow field within smaller channels, and assumed to be present within large rivers, are generally absent in this reach. This finding has profound implications for flow mixing rates, sediment transport rates and pathways, and thus the interpretation of confluence–diffluence morphology and sedimentology. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

Seabed characterization through a range of high-resolution acoustic systems – a case study offshore Oman     

Magdalena Szuman  Christian Berndt  Colin Jacobs  Angus Best 《Marine Geophysical Researches》2006,27(3):167-180

This study uses three acoustic instruments (different in their operating frequencies, 13, 3.5, and 6–10 kHz, and deployment type, hull-mounted, surface-towed and deep-towed) to investigate and characterize the acoustic response of seafloor NE of Oman in a frequency-independent manner. High-resolution control was achieved by having selected areas of our acoustic transects ground-truthed by sampling and/or sea-floor photography. On the regional scale, the greatest degree of change in backscatter amplitude was correlated with major changes of seabed morphology and lithology. However, small-scale roughness had the biggest effect on amplitude on the local scale, i.e. within each area of specific seafloor type. The study also shows that seafloor reflection amplitude changes are far more easily detected by deep-towed instrument than by surface-towed or hull-mounted systems. Whilst there are significant changes in bioturbation types and density along the transects, the suite of instruments deployed was not able to pick up the effect of the bioturbation on acoustic signals.  相似文献   

Ionization, shocks and evolution of the emission-line gas of distant 3CR radio galaxies     

P. N. Best  H. J. A. Röttgering  M. S. Longair 《Monthly notices of the Royal Astronomical Society》2000,311(1):23-36

  相似文献   

The cluster environments of the z ∼ 1 3CR radio galaxies     

P. N. Best † 《Monthly notices of the Royal Astronomical Society》2000,317(3):720-736

An analysis of the environments around a sample of 28 3CR radio galaxies with redshifts 0.6< z <1.8 is presented, based primarily upon K -band images down to K ∼20 taken using the UK Infrared Telescope (UKIRT). A net overdensity of K -band galaxies is found in the fields of the radio galaxies, with the mean excess counts being comparable to that expected for clusters of Abell Class 0 richness. A sharp peak is found in the angular cross-correlation amplitude centred on the radio galaxies that, for reasonable assumptions about the luminosity function of the galaxies, corresponds to a spatial cross-correlation amplitude between those determined for low-redshift Abell Class 0 and 1 clusters.
These data are complemented by J -band images also from UKIRT, and by optical images from the Hubble Space Telescope . The fields of the lower redshift ( z ≲0.9) radio galaxies in the sample generally show well-defined near-infrared colour–magnitude relations with little scatter, indicating a significant number of galaxies at the redshift of the radio galaxy; the relations involving colours at shorter wavelengths than the 4000 Å break show considerably greater scatter, suggesting that many of the cluster galaxies have low levels of recent or on-going star formation. At higher redshifts the colour–magnitude sequences are less prominent owing to the increased field galaxy contribution at faint magnitudes, but there is a statistical excess of galaxies with the very red infrared colours ( J − K ≳1.75) expected of old cluster galaxies at these redshifts.
Although these results are appropriate for the mean of all of the radio galaxy fields, there exist large field-to-field variations in the richness of the environments. Many, but certainly not all, powerful z ∼1 radio galaxies lie in (proto)cluster environments.  相似文献   

A new automated nondestructive system for high resolution multi-sensor core logging of open sediment cores     

D. E. Gunn  A. I. Best 《Geo-Marine Letters》1998,18(1):70-77

 A new system for logging the geophysical properties of marine sediment cores allows both whole cores and split cores to be measured in a nondestructive fashion. The current sensor configuration measures compressional (P) wave velocity (500 kHz), bulk density (using gamma-ray attenuation), and magnetic susceptibility at user-defined sample intervals down the core. Split-core logging gives more reliable results than whole core logging as it mostly eliminates core-slumping effects that can lead to spurious results; it also gives higher resolution magnetic susceptibility readings. Received: 16 May 1997 / Revision received: 24 October 1997  相似文献   

The bubble bursts for cavitation in natural rivers: laboratory experiments reveal minor role in bedrock erosion          下载免费PDF全文

Paul A. Carling  Mauricio Perillo  Jim Best  Marcelo H. Garcia 《地球表面变化过程与地形》2017,42(9):1308-1316

The erosion of rock‐bedded channels generally is considered a slow process caused mainly by abrasion due to bedload or suspended sediments, but the mechanisms of rapid erosion remain unclear. Cavitation is a clear‐fluid erosive process, well known for its effect on engineering structures, when water vapour bubbles collapse and the resultant pressure shocks erode the boundary. However, although the occurrence of cavitation erosion in natural watercourses has long been a matter of debate, as yet there are no incontrovertible examples of cavitation damage to natural river beds. Using flume experiments, we show for the first time that only weakly‐cavitating clear‐water flows can occur for the range of flow velocities observed in rivers, and these do not erode medium‐hardness rocks after 68 hours. During this time period, only a very soft rock featured erosional marks due to dissolution. Thus, our results cast significant doubt on the likelihood of identifying cavitation damage in most rivers, and provide pointers to those river systems that might be investigated further to identify cavitation erosion. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

The nature and origin of pigments in black opal from Lightning Ridge,New South Wales,Australia     

J. R. Herrmann  R. Maas  P. F. Rey  S. P. Best 《Australian Journal of Earth Sciences》2013,60(7):1027-1039

Abstract

Black opal (opal-AG) owes its dark coloration to a fine-grained pigment commonly inferred to be mainly carbon, yet chemical compositions for black opals suggest there may be additional components. Here we search for such components in pigment concentrates prepared by dissolving black opal nodules (nobbies) from Lightning Ridge (NSW) in hydrofluoric acid, using electron microscopy (scanning electron microscopy, transmission electron microscopy), X-ray diffraction and laser-ablation ICP-MS. The results demonstrate the presence of sulfides—predominantly pyrite and chalcopyrite, with minor galena and Ti-oxide phases, as additional components of the pigment. ATR-FTIR analysis indicates the presence of C=O and C–H groups, consistent with an organic origin. Transmission electron microscopy images of pigment show variously deformed, originally spherical ～100?nm particles rich in sulfide and carbon, which are interpreted as thin coatings of pigment on now dissolved opaline silica spheres. Laser-ablation ICP-MS analysis identifies remnant silica in pigment concentrates, which may be interpreted as opaline silica surviving HF treatment protected as inclusions in sulfides. When examined within the context of petrographic observations from more than 1000 opal nodules (nobbies) at Lightning Ridge, these new results suggest that pigment carbon and sulfides in the nodules formed microbially under initially anoxic groundwater conditions, within pre-existing cavities concurrently being filled with silica sol ultimately derived from chemical weathering of feldspar-rich volcaniclastic sediment. Intensely black pigment layers observed at the floor of many nodules indicate settling of dark, high-density (sulfide–Ti-oxide-rich) pigment within cavities, with the implication that sulfate-reducing bacterial (SRB) activity commences early during the silica sol-gel ripening process. Microbial activity may persist until after the cavity has completely filled with the silica sol, as illustrated by abundant black opals with uniformly distributed pigment. Pigment formed at this stage may no longer be able to settle out within the ripening and increasingly viscous silica gel, thus forming pigmentation throughout the opal cavity. The existence of ‘amber’, pigment-poor opal with intensely black basal pigment layers is interpreted as signalling a lack of sulfate to sustain further SRB activity, or a change to more oxidising conditions, possibly related to interaction with surface waters within a downward-penetrating weathering front. A change in redox conditions would shut off activity of SRB and thus sulfide pigment production and allow development of aerobic microbial activity as described by others.  相似文献