Changes to sediment sources following wildfire in a forested upland catchment,southeastern Australia     

Hugh G. Smith  Gary J. Sheridan  Patrick N. J. Lane  Philip J. Noske  Henk Heijnis 《水文研究》2011,25(18):2878-2889

Few investigations link post‐fire changes to sediment sources and erosion processes with sediment yield response at the catchment scale. This linkage is essential if downstream impacts on sediment transport after fire are to be understood in the context of fire effects across different forest environments. In this study, we quantify changing source contributions to fine sediment (<63 µm) exported from a eucalypt forest catchment (136 ha) burnt by wildfire. The study catchment is one of a pair of research catchments located in the East Kiewa River valley in southeastern Australia that have been the subject of a research program investigating wildfire effects on runoff, erosion, and catchment sediment/nutrient exports. This previous research provided the opportunity to couple insights gained from a range of measurement techniques with the application of fallout radionuclides ¹³⁷Cs and ²¹⁰Pb_ex to trace sediment sources. It was found that hillslope surface erosion dominated exports throughout the 3·5‐year post‐fire measurement period. During this time there was a pronounced decline in the proportional surface contribution from close to 100% in the first six months to 58% in the fourth year after fire. Over the study period, hillslope surface sources accounted for 93% of the fine sediment yield from the burnt catchment. The largest decline in the hillslope contribution occurred between the first and second years after fire, which corresponded with the previously reported large decline in sediment yield, breakdown of water repellency in burnt soils, substantial reduction in hillslope erodibility, and rapid surface vegetation recovery. Coupling the information on sediment sources with hillslope process measurements indicated that only a small proportion of slopes contributed sediment to the catchment outlet, with material derived from near‐channel areas dominating the post‐fire catchment sediment yield response. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

Preserving the unpreservable: a lost world rediscovered at Christian Malford, UK     

Philip R. Wilby  Keith Duff  Kevin Page  & Susan Martin 《Geology Today》2008,24(3):95-98

The small village of Christian Malford, Wiltshire (UK) is known to palaeontologists the world over because of the chance discovery of an astonishing fossil bonanza in the mid-nineteenth century. Pits in the Jurassic Oxford Clay yielded thousands of specimens of exquisitely preserved ammonites, fish and crustaceans, but became most famous for squid-like cephalopods and belemnites (collectively termed coleoids) with fossilized soft-parts. The precise location of the find has remained obscure, until now, and a new attempt is underway to understand the ancient environment that triggered this unusual preservation.  相似文献   

The flux-dependent amplitude of broadband noise variability in X-ray binaries and active galaxies     

Philip Uttley  Ian M. McHardy 《Monthly notices of the Royal Astronomical Society》2001,323(2):L26-L30

Standard shot-noise models, which seek to explain the broadband noise variability that characterizes the X-ray light curves of X-ray binaries and active galaxies, predict that the power spectrum of the X-ray light curve is stationary (i.e. constant amplitude and shape) on short time-scales. We show that the broadband noise power spectra of the black hole candidate Cyg X-1 and the accreting millisecond pulsar SAX J1808.4−3658 are intrinsically non-stationary, in that rms variability scales linearly with flux. Flux-selected power spectra confirm that this effect is due to changes in power-spectral amplitude and not shape. The light curves of three Seyfert galaxies are also consistent with a linear relationship between rms variability and flux, suggesting that it is an intrinsic feature of the broadband noise variability in compact accreting systems over more than six decades of central object mass. The rms variability responds to flux variations on all measured time-scales, raising fundamental difficulties for shot-noise models which seek to explain this result by invoking variations in the shot parameters. We suggest that models should be explored where the longest time-scale variations are fundamental and precede the variations on shorter time-scales. Possible models which can explain the linear rms-flux relation include the fractal break-up of large coronal flares, or the propagation of fluctuations in mass accretion rate through the accretion disc. The linear relationship between rms variability and flux in Cyg X-1 and SAX J1808.4−3658 is offset on the flux axis, suggesting the presence of a second, constant-flux component to the light curve which contributes ∼25 per cent of the total flux. The spectrum of this constant component is similar to the total spectrum, suggesting that it may correspond to quiet, non-varying regions in the X-ray emitting corona.  相似文献   

Cyclic and secular variation in the temperatures and radii of extreme helium stars     

C. Simon Jeffery  Rhaana L. C. Starling  †  Philip W. Hill ‡  Don Pollacco 《Monthly notices of the Royal Astronomical Society》2001,321(1):111-130

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The inception and early evolution of the North Alpine Foreland Basin, Switzerland   总被引：11，自引：1，他引：10  

Philip A. Allen  Sarah L. Crampton  Hugh D. Sinclair 《Basin Research》1991,3(3):143-163

The stratigraphy of the Eocene-Miocene peripheral foreland basin in Switzerland consists of basal deposits of Nummulitic Limestones and Globigerina Marls representing a phase of deepening, followed by two shallowing-up megacycles culminating in fully continental sedimentation. The onset of sedimentation was diachronous and took place on an unconformity surface with increasing stratigraphic gap to the north and west. In the Ultrahelvetic units, which were derived from the south and have a provenance between the Helvetic shelf and the Penninic ocean, the stratigraphic gap is minimal. This restricts the initiation of erosion of the southern European margin due to emersion to post-Maastrichtian and pre-late Palaeocene. This coincides with the final closing of the Valais trough and may therefore be interpreted as the point at which continental flexure s. s. started. In the autochthon, the subcrop map of the unconformity surface shows that the regional pattern of subcropping units is oblique to both neo-Alpine tectonic structures and Helvetic (Mesozoic) passive margin structures. There are local zones of disruption to the broad regional pattern suggesting that the basal unconformity was corrugated. Both the paliaspastic restoration of the autochthon relative to the thrust front during the Palaeocene, and the regional pattern of erosion indicate that the basal unconformity may be due to erosion of a flexural forebulge. Following deposition of the shallow water Nummulitic Limestones and the deeper water Globigerina Marls, clastic sediments were shed from the orogenic wedge in the south. These turbidites, the Taveyannaz Sandstones, filled both ponded basins at the contemporaneous thrust front and the frontal trench or foredeep. Evidently, early thrusts drove at a shallow level into the embryonic basin as ‘front-runners’, whereas most shortening and uplift continued to take place within the main part of the orogenic wedge further to the south. Eventually, the frontal palaeohighs, together with the turbidite basins, were buried by the northward emplacement of surface mud-slides, and sediment depocentres were translated northwards onto the foreland. The most likely cause of the underfilled ‘Flysch’ stage is the rapid advance of a submarine thrust wedge over the flexed European plate which resulted in (i) low sediment fluxes and (ii) high subsidence rates associated with the rapid migration of the load and depocentre. Later, as the rate of advance slowed and the wedge became subaerially exposed, the basin rapidly filled with coarse-grained detritus representing the ‘Molasse’ stage.  相似文献   

The brown dwarf desert as a consequence of orbital migration     

Philip J.Armitage  Ian A.Bonnell 《Monthly notices of the Royal Astronomical Society》2002,330(1):L11-L14

We show that the dearth of brown dwarfs in short-period orbits around Solar-mass stars – the brown dwarf desert – can be understood as a consequence of inward migration within an evolving protoplanetary disc. Brown dwarf secondaries forming at the same time as the primary star have masses which are comparable to the initial mass of the protoplanetary disc. Subsequent disc evolution leads to inward migration, and destruction of the brown dwarf, via merger with the star. This is in contrast with massive planets, which avoid this fate by forming at a later epoch when the disc is close to being dispersed. Within this model, a brown dwarf desert arises because the mass at the hydrogen-burning limit is coincidentally comparable to the initial disc mass for a Solar mass star. Brown dwarfs should be found in close binaries around very low mass stars, around other brown dwarfs, and around Solar-type stars during the earliest phases of star formation.  相似文献   

New Validity Conditions for the Multivariate Matérn Coregionalization Model,with an Application to Exploration Geochemistry     

Emery  Xavier  Porcu  Emilio  White  Philip 《Mathematical Geosciences》2022,54(6):1043-1068

Mathematical Geosciences - This paper addresses the problem of finding parametric constraints that ensure the validity of the multivariate Matérn covariance for modeling the spatial...  相似文献   

Macau’s role as a recreation/tourist center in the Pearl River Delta city-region     

Clifton W. Pannell  Philip H. Loughlin 《Urban geography》2015,36(6):883-904

The return of Macau to Chinese sovereignty in 1999 brought far-reaching change to Macau as a special administrative region (SAR). China’s policy and plans for a revitalized Macau as a key urban node offers an opportunity to conceptualize a leading role for Macau as the pre-eminent recreational and tourist center in the dynamic and globally connected Pearl River Delta city-region. We examine and assess the new policies that have led to Las Vegas-style casinos bringing explosive growth in visitors, gambling revenues, and Macau’s economy. New problems of corruption, crime, and social pathologies have appeared as well owing in part to the secretive VIP gambling centers for high rollers from the mainland. Has Macau met China’s goals and expectations for a great tourist and recreational center? Our findings indicate a mixed record with more challenges emerging in the wake of China’s recent anti-corruption campaign.  相似文献   

Evaluation of Development Options for Alaska North Slope Viscous and Heavy Oil     

Emil D. Attanasi  Philip A. Freeman 《Natural Resources Research》2015,24(1):85-106

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The status of measurement of the Mediterranean mean dynamic topography by geodetic techniques   总被引：1，自引：1，他引：0  

Philip L. Woodworth  Médéric Gravelle  Marta Marcos  Guy Wöppelmann  Chris W. Hughes 《Journal of Geodesy》2015,89(8):811-827

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