The anatomy of Continental Flood Basalt Provinces: geological constraints on the processes and products of flood volcanism   总被引：2，自引：0，他引：2  

Dougal A. Jerram  Mike Widdowson   《Lithos》2005,79(3-4):385-405

The internal architecture of the immense volumes of eruptive products in Continental Flood Basalt Provinces (CFBPs) provides vital clues, through the constraint of a chrono-stratigraphic framework, to the origins of major intraplate melting events. This work presents close examination of the internal facies architecture and structure, duration of volcanism, epeirogenetic uplift associated with CFBPs, and the potential environmental impacts of three intensely studied CFBPs (the Parana-Etendeka, Deccan Traps and North Atlantic Igneous Province). Such a combination of key volcanological, stratigraphic and chronologic observations can reveal how a CFBP is constructed spatially and temporally to provide crucial geological constraints regarding their development.

Using this approach, a typical model can be generated, on the basis of the three selected CFBPs, that describes three main phases of flood basalt volcanism. These phases are recognized in Phanerozoic CFBPs globally. At the inception of CFBP volcanism, relatively low-volume transitional-alkaline eruptions are forcibly erupted into exposed cratonic basement lithologies, sediments, and in some cases, water. Distribution of initial volcanism is strongly controlled by the arrangement of pre-existing topography, the presence of water bodies and local sedimentary systems, but is primarily controlled by existing lithospheric and crustal weaknesses and concurrent regional stress patterns. The main phase of volcanism is typically characterised by a culmination of repeated episodes of large volume tholeiitic flows that predominantly generate large tabular flows and flow fields from a number of spatially restricted eruption sites and fissures. These tabular flows build a thick lava flow stratigraphy in a relatively short period of time (c. 1–5 Ma). With the overall duration of flood volcanism lasting 5–10 Ma (the main phase accounting for less than half the overall eruptive time in each specific case). This main phase or ‘acme’ of volcanism accounts for much of the CFBP eruptive volume, indicating that eruption rates are extremely variable over the whole duration of the CFBP. During the waning phase of flood volcanism, the volume of eruptions rapidly decrease and more widely distributed localised centres of eruption begin to develop. These late-stage eruptions are commonly associated with increasing silica content and highly explosive eruptive products. Posteruptive modification is characterised by continued episodes of regional uplift, associated erosion, and often the persistence of a lower-volume mantle melting anomaly in the offshore parts of those CFBPs at volcanic rifted margins.  相似文献   

Phase transformation of Mg-calcite to aragonite in active-forming hot spring travertines     

Heather F. Greer  Wuzong Zhou  Li Guo 《Mineralogy and Petrology》2015,109(4):453-462

  相似文献   

Electrical resistivity imaging of hydrologic flow through surface coal mine valley fills with comparison to other landforms          下载免费PDF全文

Breeyn M. Greer  Thomas J. Burbey  Carl E. Zipper  Erich T. Hester 《水文研究》2017,31(12):2244-2260

Surface coal mining has altered land cover, near‐surface geologic structure, and hydrologic processes of large areas in central Appalachia, USA. These alterations are associated with changes in water quality such as elevated total‐dissolved solids, which is usually measured via its surrogate, specific conductance (SC). The SC of valley fill effluent streams is a function of fill construction methods, materials, and age; yet hydrologic studies that relate these variables to water quality are sparse due to the difficulty of conducting traditional hydrologic studies in mined landscapes. We used electrical resistivity imaging (ERI) to visualize the subsurface geologic structure and hydrologic flow paths within a valley fill. ERI is a noninvasive geophysical technique that maps spatiotemporal changes in resistivity of the subsurface. We paired ERI with artificial rainfall experiments to track infiltrated water as it moved through the valley fill. Results indicate that ERI can be used to identify subsurface geologic structure and track advancing wetting fronts or preferential flow paths. Our results suggest that the upper portion of the fill contains significant fines, whereas the deeper profile is primarily large rocks and void spaces. Water tended to pond on the surface of compacted areas until it reached preferential flow paths, where it appeared to infiltrate quickly down to >15 m depth in 75 min. ERI applications can improve understanding of how fill construction techniques influence subsurface water movement, and in turn may aid in the development of valley fill construction methods to reduce water quality effects.  相似文献   

TRACER AND DARCY-BASED IDENTIFICATION OF SUBSURFACE FLOW, BUKIT TIMAH FOREST, SINGAPORE     

M.D. Sherlock  Nick Chappell  Tony Greer 《Singapore journal of tropical geography》1996,16(2):197-215

  相似文献   

Infrared detection techniques for space research: V. Manno and J. Ring (Eds.)(Proceedings of the 5th ESLAB/ESRIN Symposium,Noordwijk, Netherland,June 1971). Reidel,Dordrecht, Holland, 1972. xi + 344. $29.25.     

R.G.H. Greer 《Planetary and Space Science》1973,21(4):712

  相似文献   

Hydrography of the Santee River during moderate discharge conditions     

Björn Kjerfve  J. E. Greer 《Estuaries and Coasts》1978,1(2):111-119

To harness hydroelectric power, most of the flow of the Santee River, SC was diverted in 1942 into Charleston Harbor, where shoaling promptly became a major problem. For this reason, most of the diverted flow is scheduled to be rediverted to the Santee within the next decade, increasing the mean discharge of the Santee from 74 to 428 m³s^?1. To assess the present hydrogrpahy of the Santee estuary under conditions of moderate discharge, we determined 226 vertical profiles of velocity, salinity, and temperature distributed over 17 stations in February, 1975. We found that 73 and 27% of the discharge reached the ocean via the North and South distributaries, respectively. The 1 ppt isohaline was found no further than 8 km upstream from the mouth, indicating the limited extent of the estuarine zone. The Santee is a partially mixed estuary classified as type 2b. The circulation parameter is approximately 3 and the stratification parameter approximately 0.3. The bulk parameters indicate the importance of tidal, mixing and a weakly developed gravitational circulation. When rediversion is completed, the net salinity in the lower Santee River can be expected to decrease drastically, which in turn is likely to terminate the lucrative oyster and clam fishery.  相似文献   

Close encounters in young stellar clusters: implications for planetary systems in the solar neighbourhood     

Daniel Malmberg  Francesca De Angeli  Melvyn B. Davies  Ross P. Church  Dougal Mackey  Mark I. Wilkinson 《Monthly notices of the Royal Astronomical Society》2007,378(3):1207-1216

The stars that populate the solar neighbourhood were formed in stellar clusters. Through N -body simulations of these clusters, we measure the rate of close encounters between stars. By monitoring the interaction histories of each star, we investigate the singleton fraction in the solar neighbourhood. A singleton is a star which formed as a single star, has never experienced any close encounters with other stars or binaries, or undergone an exchange encounter with a binary. We find that, of the stars which formed as single stars, a significant fraction is not singletons once the clusters have dispersed. If some of these stars had planetary systems, with properties similar to those of the Solar System, the planets' orbits may have been perturbed by the effects of close encounters with other stars or the effects of a companion star within a binary. Such perturbations can lead to strong planet–planet interactions which eject several planets, leaving the remaining planets on eccentric orbits. Some of the single stars exchange into binaries. Most of these binaries are broken up via subsequent interactions within the cluster, but some remain intact beyond the lifetime of the cluster. The properties of these binaries are similar to those of the observed binary systems containing extrasolar planets. Thus, dynamical processes in young stellar clusters will alter significantly any population of Solar System-like planetary systems. In addition, beginning with a population of planetary systems exactly resembling the Solar System around single stars, dynamical encounters in young stellar clusters may produce at least some of the extrasolar planetary systems observed in the solar neighbourhood.  相似文献   

The altitude dependence of the O₂(A³Σ_u⁺) vibrational distribution in the terrestrial nightglow     

I.C. McDade  E.J. Llewellyn  R.G.H. Greer  D.P. Murtagh 《Planetary and Space Science》1982,30(11):1133-1136

A simple vibrational relaxation model which reproduces the observed altitude integrated vibrational distribution of the Herzberg I bands in the nightglow is used to derive the altitude profiles of the individual vibrational levels at 1 km intervals in the 85–115 km height range. The possible errors associated with using rocket-borne photometer measurements of a limited number of bands in the O₂(A³Σ_u⁺?X³Σ_g^?) system to infer the total Herzberg I emission profile are assessed.  相似文献   

The upper atmosphere and solar- terrestrial relations: J. K. Hargreaves: Van Nostrand Rheinhold,London. XV + 300. U.K. £15.00 (hardback), £7.00 (paperback)     

R.G.H. Greer 《Planetary and Space Science》1980,28(6):655

  相似文献   

The use of proxy chemical records in Coral skeletons to ascertain past environmental conditions in Florida Bay     

Peter Koenraad Swart  Genevieve Healy  Lisa Greer  Michael Lutz  Amel Saied  Daniel Anderegg  Richard E. Dodge  David Rudnick 《Estuaries and Coasts》1999,22(2):384-397

This paper will discuss the use of chemical proxies in coral skeletons to reconstruct the history of salinity (from the δ¹⁸O of the skeleton) and nutrients in the water (from the δ¹³C) in Florida Bay between 1824 and 1994. Monthly salinity and water temperature data collected since 1989 were used to establish a correlation between salinity, temperature, and the δ¹⁸O of the skeleton of the coralSolenastrea bournoni from Lignumvitae Basin in Florida Bay. This relationship explains over 50% of the variance in the δ¹⁸O of the skeleton. Assuming that interannual variations in the temperature of the water are small, we have applied this relationship to the δ¹⁸O measured in the coral skeleton collected from Lignumvitae Basin which has a record between 1824 and 1993. These data provide a revised estimate of salinity variation in Lignumvitae Basin for the period when historical records for salinity were not available, and show that the highest salinity events occurred in the past 30 yr. Using the relationships between the salinity in Lignumvitate Basin and other basins, obtained using a modern dataset, we are able to estimate ranges in salinity for other portions of Florida Bay. Skeletons of specimens of the coral speciesSiderastrea radians collected from other areas of Florida Bay show similar patterns in the δ¹⁸O over the past 10 yr, indicating that corals in most portions of Florida Bay are recording salinity variations in their skeletons and therefore support the idea that salinity variations in different portions of Florida Bay can be related. Fluorescence analysis of the coral from Lignumvitae Basin shows a large change in the magnitude of the 10-yr signal coincident with the construction of the railway, confirming that this event had a significant impact upon Florida Bay. The δ¹³C of the coral skeletons reveals a long-term history of the oxidation of organic material, fixation of carbon by photosynthesis (algal blooms), and the intrusion of marine water into the bay. Since the construction of the railway from Miami to Key West there has been a long-term decrease in the δ¹³C of the coral skeleton from Lignumvitae Basin, suggesting the increased oxidation of organic material in this area. This decrease in δ¹³C appears to have reached a minimum value around 1984 and has increased since this time in the western portions of Florida Bay. The increase may be related to the algal blooms prevalent in the area or alternatively could result from intrusion of more marine water. In the eastern areas, a small increase in the δ¹⁸C between 1984 and 1988 was followed by further decline suggesting more oxidation of organic material. We have also attempted to use the concentration of barium in the coral skeleton as a proxy indicator of the nutrient status in Florida Bay.  相似文献