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101.
John Kemp 《Journal of African Earth Sciences》1996,22(4):507-523
The Kuara Formation was originally described in the Nuqrah quadrangle, northern Arabian Shield, as composed of sedimentary and volcanic rocks and attributed to the Neoproterozoic Shammar group. The group has been examined in the type area of the Kuara Formation. The name ‘Kuara Formation’ is here formally proposed and restricted to the essentially sedimentary succession. The sediments were most likely deposited in an approximately north-south to northeast-southwest fault-bounded basin more than 20 km wide and closed to the south by an approximately east-west fault. The formation probably attained more than 600 m in thickness and is characterized by abundant, locally derived conglomerate and by coarsening-upward sequences organized in megasequences; these are interpreted as representing the progradation of alluvial fans into a lake. Sharp contacts of siltstone overlying conglomerate are interpreted as due to the lowering of the trough floor by faulting, subsequent lacustrine sedimentation corresponding to periods of maximum tectonic activity and alluvial fans prograding, periods of reduced activity. The interpretation of the tectonic environment as one of extensional faulting in a continental setting is in agreement with interpretations proposed for other successions of similar age in Arabia and Egypt. 相似文献
102.
Ecosystem model of an estuarine submersed plant community: Calibration and simulation of eutrophication responses 总被引:1,自引:0,他引:1
As water quality in the Chesapeake Bay has declined over recent decades, formely healthy submersed plant communities have disappeared from littoral areas of the mesohaline estuary. A dynamic simulation model of shallow regions of bay tributaries (<1 m) was developed to investigate growth responses of submersed vascular plants to eutrophication and habitat degradation. Our objectives were to elucidate mechanisms responsible for the decline and to evaluate conditions required for plant restoration and survival. State varibles in the model are plant leaves, roots, phytoplankton, epiphytes, and detrital material. The model calculates biomass pools and biogeochemical rate processes over annual cycles with a time step of 6 h. Simulations were performed to investigate the influence of phytoplankton and epiphytes on the underwater light environment, how the balance of limiting resources (light and nutrients) controls growth and productivity of submersed plants, and conditions necessary, for the restoration of submersed vegetation. Model output for submersed plants was calibrated to baseline data from the mid 1970s (r2=0.86); simulations reproduced declines in plant biomass with increasing nutrient enrichment. Model experiments showed, that by increasing nutrient inputs 40% above levels observed in the 1960s, submersed plants disappeared within 1–2 yr due to enhanced growth of phytoplankton and epiphytes, which reduced light below required levels. Epiphytes were more important than were phytoplankton in attenuating light. The relationship between nutrient enrichment and plant loss rate was complex, as epiphyte density on leaf surfaces was not linearly related to nutrient levels. Relatively small nutrient increases could have a large effect on submersed plants because epiphyte density on leaves increased exponentially as leaf surface area decreased. Exchanges of organic carbon and nutrients between leaf and root compartments were seasonally variable and were critical for survival of submersed plants. The amount of root-rhizome material available for regrowth could control the outcome of nutrient reduction strategies. Consequently, model predictions of plant restoration success were highly dependent on initial conditions. The model is being used successfully as a research tool to interpret ecological relationships in the ongoing re-evaluation of management alternatives for submersed plant restoration. 相似文献
103.
John Kemp 《Journal of African Earth Sciences》1998,26(4):551-572
Volcanic formations of the ca 630-620 Ma old Shammar Group in the Tuluhah area in the northern Arabian Shield occupy an oval area some 8×12 km. They overlie sedimentary rift-fill of the Kuara Formation and are interpreted as related to the formation of a caldera, here named the Awad Caldera. The earliest of the volcanic formations, the Dabsah Tuff, is more than 450 m thick in the south and wedges out in the north. It is composed of silicic, medial to proximal pyroclastic flow rocks that record an eruption during which an initial caldera is interpreted to have formed by probably trapdoor-style collapse. The Nijab Basalt, more than 200 m thick and present as flows overlying the Kuara Formation to the north of the caldera, is presumed to have originated outside the study area during an interval between periods of silicic volcanic activity, and to have flowed onto the Dabsah Tuff in the first-stage caldera. The succeeding Mindassa Megabreccia contains large rafts of the older Shammar rocks, mainly Nijab Basalt, in a tuff matrix, and is regarded as probably a caldera collapse and fallback megabreccia formed during a silicic eruption that led to the second stage of caldera development. The megabreccia is overlain by the post-collapse Sutayih Tuff, more than 450 m thick, composed of proximal pyroclastic flow units. 相似文献
104.
Hillier Michael Wellmann Florian Brodaric Boyan de Kemp Eric Schetselaar Ernst 《Mathematical Geosciences》2021,53(8):1725-1749
Mathematical Geosciences - Three-dimensional structural geomodels are increasingly being used for a wide variety of scientific and societal purposes. Most advanced methods for generating these... 相似文献
105.
Thomas?AngererEmail authorView authors OrcID profile Anthony?I.?S.?Kemp Steffen?G.?Hagemann Walter?K.?Witt Jo?o?O.?Santos Christian?Schindler Carlos?Villanes 《Contributions to Mineralogy and Petrology》2018,173(5):36
Mississippian arc magmatic suites of the Au-rich Pataz and Cu-dominated Montañitas regions in Peru reveal distinct modes of magmatic-hydrothermal petro- and metallogenesis. The distinction is remarkable due to their broad contemporaneity (336–322 Ma), arc-parallel position, and close distance (<?50 km) to each other. In both arc regions, petrography, geochemistry, and the tectonic setting of magmatic suites suggest a rapid switch from syn-collisional/compressional to post-collisional/extensional (with ‘A2-type’ signature) emplacement regime. Rocks of the Au-rich Pataz region originate from mixed sources with a contribution from the mantle (εHf?>?0 and δ18O of ~?5.3‰) and assimilated old crust (variously low εHf and δ18O >?5.3‰). The ultimate source of Au in the mineralised Pataz batholith was oxidised (fO2 at FMQ buffer; based on zircon trace chemistry) and alkali-, LILE- and HFSE-enriched, most likely represented by the metasomatised mantle. The syn-extensional emplacement of the relatively reduced (ΔFMQ?<?0), but unmineralised, A2-type suite involved assimilation of reduced crust. Associated, reduced, magmatic-hydrothermal fluids infiltrated the Au-bearing batholith suite and effectively mobilised and transported and concentrated Au. In the Montañitas region, rocks are oxidised (ΔFMQ?>?0) and dominantly mantle derived without significant incorporation of crustal material. Samples from the Cu-mineralised suites indicate the additional contribution of a δ18O <?5.3‰ source, potentially melted layer-2 gabbro. In addition, the elevated whole-rock La/Yb and Sr/Y ratios are compatible with minor addition of slab-derived material, which may have enhanced Cu endowment in this region. Late-magmatic, oxidised fluids derived from the younger A2-type suite controlled Cu mobilisation and concentration, while Au behaved largely refractory. In general terms, it is postulated that source mixing in continental arcs is a first-order control of contrasting Cu and Au endowment and that sequential intrusion processes facilitate late-magmatic-hydrothermal mobilisation and concentration of specific metal assemblages. 相似文献
106.
Peter?A.?StaehrEmail author Jeremy?M.?Testa W.?Michael?Kemp Jon?J.?Cole Kaj?Sand-Jensen Stephen?V.?Smith 《Aquatic Sciences - Research Across Boundaries》2012,74(1):15-29
Measurements of the production and consumption of organic material have been a focus of aquatic science for more than 80 years.
Over the last century, a variety of approaches have been developed and employed for measuring rates of gross primary production
(Pg), respiration (R), and net ecosystem production (Pn = Pg − R) within aquatic ecosystems. Here, we reconsider the range of approaches and applications for ecosystem metabolism measurements,
and suggest ways by which such studies can continue to contribute to aquatic ecology. This paper reviews past and contemporary
studies of aquatic ecosystem-level metabolism to identify their role in understanding and managing aquatic systems. We identify
four broad research objectives that have motivated ecosystem metabolism studies: (1) quantifying magnitude and variability
of metabolic rates for cross-system comparison, (2) estimating organic matter transfer between adjacent systems or subsystems,
(3) measuring ecosystem-scale responses to perturbation, both natural and anthropogenic, and (4) quantifying and calibrating
models of biogeochemical processes and trophic networks. The magnitudes of whole-system gross primary production, respiration
and net ecosystem production rates vary among aquatic environments and are partly constrained by the chosen methodology. We
argue that measurements of ecosystem metabolism should be a vital component of routine monitoring at larger scales in the
aquatic environment using existing flexible, precise, and durable sensor technologies. Current and future aquatic ecosystem
studies will benefit from application of new methods for metabolism measurements, which facilitate integration of process
measurements and calibration of models for addressing fundamental questions involving ecosystem-scale processes. 相似文献
107.
This paper examines the weathering processes that have combined to produce the distribution of soil‐regolith (SR) thickness across the Triassic Sherwood Sandstone Group outcrop (750 km2) in Nottinghamshire, UK. Archive borehole logs (n = 282) taken across the outcrop showed that SR thickness had mean and median depths of ~1·8 and 1·5 m, respectively. Cores were taken from a forested site to depths ~3 m for geochemical analysis. At this site the SR thickness was ~1·7 m. Analysis of the loss of elements, compared to bedrock using mass balance calculations (τ) showed that all the calcite and gypsum cement had been removed to depths of >3 m. Thus the major difference between the SR and the underlying saprolite was that the former exists as loose sand as opposed to a semi‐durable rock. Scanning electron microscopy (SEM) analysis of core samples suggested that the non‐durable rock or saprolite had greater cementation of clay particles. We propose that the mechanism through which the clay cement (and other interlocking grain bonds) was eased apart was through freeze–thaw processes associated with the summer ‘active layer development (ALD)’ during the last glacial activity in the UK. We tested this theory by developing a Monte Carlo simulation based on a simplified version of the Stefan equation. Current Arctic datasets of air and ground temperatures were obtained to provide reasonable starting conditions for input variables. These were combined with known data for thermal conductivity, bulk density and moisture content of the Sherwood Sandstone regolith. Model predictions (n = 1000) of the distribution of SR thickness accurately reflect the observed distribution thickness from the borehole logs. This is strong evidence that freeze–thaw and ‘ALD’ processes are major factors in determining the thickness of SR across this outcrop. British Geological Survey © NERC 2012 相似文献
108.
We evaluated two digital data sources that might be helpful in characterizing grasshopper habitat using plant and grasshopper species composition data collected at 128 sites in three areas of Montana. A GIS was used to associate each sampling site with Omernik's ecoregions and the Montana State Soil Geographic Database (MTSTATSGO). Detrended Correspondence Analysis (DCA) and statistical analyses were used to test for correlations among grasshopper species, available water capacity, and soil permeability across sampling areas and ecoregions. Four grasshopper species were correlated with soil permeability and six were correlated with available water capacity. MTSTATSGO plant cover percentages did not correlate with cover measured in the field, indicating inadequate resolution for the scale of this study. Ecoregions were useful in distinguishing grasshopper community gradients across Montana, from mountains to plains. These georeferenced data should be considered as input for grasshopper forecasting and decision-making models. Our results show how GIS can be used to evaluate relationships between digital data sets and ecological data gathered in the field. 相似文献
109.
A. Fassia W. P. S. Meikle W. D. Vacca S. N. Kemp N. A. Walton D. L. Pollacco S. Smartt A. Oscoz A. Aragón-Salamanca S. Bennett T. G. Hawarden A. Alonso D. Alcalde A. Pedrosa J. Telting M. J. Arevalo H. J. Deeg F. Garzón A. Gómez-Roldán G. Gómez C. Gutiérrez S. López M. Rozas M. Serra-Ricart M. R. Zapatero-Osorio 《Monthly notices of the Royal Astronomical Society》2000,318(4):1093-1104
We present contemporaneous optical and infrared (IR) photometric observations of the Type IIn SN 1998S covering the period between 11 and 146 d after discovery. The IR data constitute the first ever IR light curves of a Type IIn supernova. We use blackbody and spline fits to the photometry to examine the luminosity evolution. During the first 2–3 months, the luminosity is dominated by the release of shock-deposited energy in the ejecta. After ∼100 d the luminosity is powered mostly by the deposition of radioactive decay energy from 0.15±0.05 M⊙ of 56 Ni which was produced in the explosion. We also report the discovery of an astonishingly high IR excess, K − L '=2.5, that was present at day 130. We interpret this as being due to thermal emission from dust grains in the vicinity of the supernova. We argue that to produce such a high IR luminosity so soon after the explosion, the dust must be pre-existing and so is located in the circumstellar medium of the progenitor. The dust could be heated either by the UV/optical flash (IR echo) or by the X-rays from the interaction of the ejecta with the circumstellar material. 相似文献
110.
Records of Australian palaeoclimate beyond the last glacial cycle are rare, limiting detailed analysis of long-term climate trends and associated ecosystem responses. This study analyses a discontinuous pollen and charcoal record from Fern Gully Lagoon, North Stradbroke Island (Minjerribah), subtropical Queensland, Australia, which covers much of the last ~210 ,000 years. Climate variation is inferred from changes in vegetation, while analysis of micro- and macrocharcoal is used to infer fire activity. Pollen assemblages consist of ~40% rainforest taxa during marine isotope stage (MIS) 7a–c and early MIS 5. These are inferred to result from high rainfall in the Australian subtropics, which was also evident in north-east and central Australia. Human impact from 21 ,000 years ago likely supressed post-MIS 2 rainforest expansion to some extent. However, the increased Holocene abundance of herbs and grasses and reduced representation of aquatic taxa suggest that the Holocene was relatively dry when compared with early MIS 5 and MIS 7a–c. Similar MIS 5 and early MIS 7a–c climates, in contrast to a notably drier Holocene, suggest that the progressive interglacial drying trend most strongly recorded in central Australia was not a major feature of subtropical eastern Australian climates. 相似文献