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991.
The growth and collapse of mud mounds at a site on the Liverpool Plains in northern New South Wales, Australia has been observed over a 12-year period. The mud mounds appeared in a flat field for the first time in living memory in 1989, but their prior existence in the early Holocene is indicated by archaeological data. The piezometric head in bores drilled through a 7-m bed of clayey silt and screened in weathered basalt at a depth of 8 m was more than 2 m above ground level. Clay has been carried in suspension by water seeping to the ground surface where it has accumulated and formed a mound. Approximately eight years after their initial appearance, the growth of the mounds stopped and within a further three years they had almost completely disappeared.Mechanisms for the growth and decay of the mounds are reviewed. The chemistry of the shallow bore water and the water seeping from the surface of the mounds was dominated by sodium bicarbonate with a 4 mEq/l increase between the weathered basalt and the surface of the mound. Inverse modelling (PHREEQC) is used to determine possible chemical reactions that can account for this increase.

Electronic Supplementary Material Supplementary material is available in the online version of this article at http://dx.doi.org/10.1007/s10040-003-0278-0.
Resumen Se ha observado durante 12 años el crecimiento y el colapso de montículos de lodo en un emplazamiento ubicado en las Llanuras de Liverpool, en el estado australiano de Nueva Gales del Sur. Según la memoria existente, los montículos de lodo aparecieron en un campo llano por vez primera en 1989, pero, por datos arqueológicos, se conoce de su existencia a comienzos del Holoceno. Los niveles piezométricos en sondeos perforados a través de 7 m de limos arcillosos y ranurados en el basalto meteorizado a 8 m son superiores en más de 2 m a la superficie del terreno. La arcilla es portada en suspensión por el agua que descarga hacia la superficie del terreno, donde se acumula y forma el montículo. Unos 8 años después de su aparición, el crecimiento de los montículos se detiene y éstos acaban prácticamente desapareciendo en otros 3 años.Se revisa los mecanismos que originan el crecimiento y desaparición de los montículos. La química de las aguas someras de los sondeos y del agua que se filtra desde la superficie de los montículos está dominada por bicarbonato sódico, con un incremento de 4 meq/L entre el basalto meteorizado y la superficie del montículo. Se utiliza la modelación inversa (PHREEQC) para determinar las reacciones químicas que pueden explicar dicho aumento.

Résumé La croissance et l'effondrement de monticules de vase situés dans les plaines de Liverpool, dans le nord des Nouvelles Galles du Sud, ont été observés pendant 12 ans. Les monticules de vase sont apparus en terrain plat pour la première fois de mémoire d'homme en 1989; mais leur existence antérieure dès le début de l'Holocène est attesté par des données archéologiques. Le niveau piézométrique dans des forages traversant 7 m de silt argileux et recouvrant un basalte altéré à 8 m était de plus de 2 m au-dessus de la surface du sol. L'argile a été apportée en suspension par l'eau suintant à la surface du sol où elle s'est accumulée pour former un monticule. Environ 8 ans après leur première apparition, la croissance des monticules s'est arrêtée et ils ont presque complètement disparu dans les 3 ans qui ont suivi.Les mécanismes de croissance et de régression de ces monticules sont passés en revue. La chimie de l'eau des forages à proximité de la surface et de l'eau filtrant à la surface des monticules était dominée par le bicarbonate de sodium, avec une augmentation de 4 meq/l entre le basalte altéré et la surface du monticule. Une modélisation inverse (PHREEQC) a été mise en uvre pour déterminer les réactions possibles pouvant rendre compte de cet accroissement.
  相似文献   
992.
Simulations of LGM climate of East Asia by regional climate model   总被引:3,自引:0,他引:3  
ClimateconditionsintheLastGlacialMaximum(LGM)wereremarkablydifferentfromthepresentones.LGMglobalmeantemperaturewas5℃-10℃dropbutprecipitationdecreasescommonly.LGMhasbecomethekeyphasetoreconstructtheearthenvironmentalfield,retrieveextremecoldclimatecondit…  相似文献   
993.
This article describes a methodology to localise areas with high potential towards natural snowpack instability under particular meteorological conditions, at the scale of an Alpine valley. Localisation is based on statistically relating known release areas of past avalanche events to maps of: (1) slope inclination, (2) slope orientation (aspect), (3) elevation, (4) distance from crest lines, (5) terrain roughness and (6) concavities/convexities. The maps have been built using two different GIS softwares while the statistical analyses have been performed with a specific software handling also Fuzzy Set theory algorithms. The results of the statistical analyses have been verified on test release—areas which have not been used as input data for the statistical analyses. Verification allowed to quantify how reliably the susceptibility values were calculated, to compare the values obtained using different combinations of terrain features and to finally decide on the most efficient combination. The susceptibility maps were calculated and verified for three different meteorological scenarios (given by three classes of snow depth). Verification has shown that the accuracy of the susceptibility maps was between 67% and 82%. The three susceptibility maps show a remarkable difference in the spatial pattern of the highest susceptibility pixels suggesting that for different meteorological scenarios different classes of terrain features need to be considered.The possibility to make combinations of terrain features and to assess and verify their statistical relationship with release areas of past avalanche events is the major original step made by STARTER. Linking those release areas to meteorological scenarios is an attempt to include in the analysis the combined influence of terrain features and meteorological conditions towards snowpack instability.  相似文献   
994.
The present study was undertaken with the objective of deriving constraints from available geological and geophysical data for understanding the tectonic setting and processes controlling the evolution of the southern margin of the East European Craton (EEC). The study area includes the inverted southernmost part of the intracratonic Dnieper-Donets Basin (DDB)–Donbas Foldbelt (DF), its southeastern prolongation along the margin of the EEC–the sedimentary succession of the Karpinsky Swell (KS), the southwestern part of the Peri-Caspian Basin (PCB), and the Scythian Plate (SP). These structures are adjacent to a zone, along which the crust was reworked and/or accreted to the EEC since the late Palaeozoic. In the Bouguer gravity field, the southern margin of the EEC is marked by an arc of gravity highs, correlating with uplifted Palaeozoic rocks covered by thin Mesozoic and younger sediments. A three-dimensional (3D) gravity analysis has been carried out to investigate further the crustal structure of this area. The sedimentary succession has been modelled as two heterogeneous layers—Mesozoic–Cenozoic and Palaeozoic—in the analysis. The base of the sedimentary succession (top of the crystalline Precambrian basement) lies at a depth up to 22 km in the PCB and DF–KS areas. The residual gravity field, obtained by subtracting the gravitational effect of the sedimentary succession from the observed gravity field, reveals a distinct elongate zone of positive anomalies along the axis of the DF–KS with amplitudes of 100–140 mGal and an anomaly of 180 mGal in the PCB. These anomalies are interpreted to reflect a heterogeneous lithosphere structure below the supracrustal, sedimentary layers: i.e., Moho topography and/or the existence of high-density material in the crystalline crust and uppermost mantle. Previously published data support the existence of a high-density body in the crystalline crust along the DDB axis, including the DF, caused by an intrusion of mafic and ultramafic rocks during Late Palaeozoic rifting. A reinterpretation of existing Deep Seismic Sounding (DSS) data on a profile crossing the central KS suggests that the nature of a high-velocity/density layer in the lower crust (crust–mantle transition zone) is not the same as that of below the DF. Rather than being a prolongation of the DDB–DF intracratonic rift zone, the present analysis suggests that the KS comprises, at least in part, an accretionary zone between the EEC and the SP formed after the Palaeozoic.  相似文献   
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