Ecological energetics of the tropical sea urchin Diadema antillarum Philippi in Barbados, West Indies     

Christopher M. Hawkins  John B. Lewis 《Estuarine, Coastal and Shelf Science》1982,15(6)

The common tropical sea urchin Diadema antillarum Philippi is the dominant herbivore on fringing coral reefs in Barbados, West Indies. The biological importance of Diadema as an agent of energy transfer was evaluated from energy budgets constructed for the population and for individuals of 10 size groups. Monthly energy budgets for urchins of various size groups balance within 1 kcal except for urchins of the largest size group examined. Approximately 20% of the monthly net benthic primary production of the fringing coral reef is consumed by Diadema. This percentage is considerably larger than the 7% reported for the consumption of benthic algal production by a population of the temperate water sea urchin, Strongylocentrotus droebachiensis, feeding in kelp beds but is lower than the 47% reported for the consumption of sea grass by the tropical urchin Lytechinus variegatus. Higher rates of secondary production of Diadema compared to that of Strongylocentrotus may be in part due to higher net and gross growth efficiencies exhibited by Diadema. It is apparent that Diadema is more efficient at converting its algal food resources into urchin biomass than is Strongylocentrotus of similar size. In comparison to Strongylocentrotus and Lytechinus, Diadema releases as much energy to the benthos in the form of fecal pellet detritus as do the other two species. The production of fecal pellet detritus is the most important pathway of energy transfer on the fringing coral reef. Fecal pellet detritus contributes approximately 26 kcal m⁻² month⁻¹ to the benthic community. This amount is equivalent to 7·4% of the monthly net primary production of the benthic algae or approximately 37% of the caloric intake of the urchin population. In addition fecal pellet detritus produced by Diadema contains about 10 times the caloric content of surface sediments found to the north and south of the fringing reef and approximately 1·7 times the caloric content of sediments within the reef. The utilization of this energy-rich fecal pellet detritus by other reef organisms is discussed briefly.  相似文献   

Excursion to Newbury and Boxford: Saturday,May 17th, 1924     

H.L. Hawkins 《Proceedings of the Geologists' Association. Geologists' Association》1924,35(4):395-400

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鲁西新太古代济宁群含铁岩系形成时代——SHRIMP U-Pb锆石定年   总被引：12，自引：7，他引：5  

王伟  王世进  刘敦一  李培远  董春艳  颉颃强  马铭株  万渝生 《岩石学报》2010,26(4):1175-1181

济宁群以隐伏的地质体分布于华北克拉通鲁西地区,以往被划归古元古代。近年来在济宁群的钻探和地球物理研究中,发现存在较大规模条带状硅铁建造,其形成时代引起地学界极大关注。本文对济宁群变质碎屑沉积岩和长英质火山岩进行了锆石SHRIMP年龄测定。含砾绿泥绢云千枚岩的碎屑锆石年龄主要集中在～2.7Ga,可靠的最年轻碎屑锆石年龄为2.61±0.01Ga。变质长英质火山岩岩浆锆石年龄为2.56±0.02Ga。研究表明,济宁群形成于新太古代晚期,而不是以往认为的古元古代。华北克拉通条带状铁建造主要形成于新太古代晚期。济宁群在岩石组合、变质作用方面与鞍山、冀东以及五台地区同时代含硅铁建造的表壳岩系有差别,但是与本溪南芬铁矿的岩石组合有相似之处。这些可能为我国的隐伏太古宙BIF铁矿的研究与勘探提供了重要依据。  相似文献   

Reviews     

Richard Darling  John C. Davis  D. M. Hawkins 《Mathematical Geosciences》1980,12(6):617-620

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Robust estimation of the variogram: I   总被引：9，自引：0，他引：9  

Noel Cressie  Douglas M. Hawkins 《Mathematical Geology》1980,12(2):115-125

It is a matter of common experience that ore values often do not follow the normal (or lognormal) distributions assumed for them, but, instead, follow some other heavier-tailed distribution. In this paper we discuss the robust estimation of the variogram when the distribution is normal-like in the central region but heavier than normal in the tails. It is shown that the use of a fourth-root transformation with or without the use of M-estimation yields stable robust estimates of the variogram.Visiting Scientist, NRIMS, during the period in which this work was carried out.  相似文献   

Diffuse magnetic anomalies in marginal basins: Their possible tectonic and petrologic significance     

L.A. Lawver  J.W. Hawkins 《Tectonophysics》1978,45(4):323-339

Marginal basins, areas of oceanic lithosphere peripheral to large ocean basins, may be formed by several processes, but the young active marginal basins have the geophysical and geochemical characteristics of young normal oceanic lithosphere. We recognize two distinct tectonic settings in which new oceanic lithosphere may be formed in areas which would be termed marginal basins:

1. (1) Upwelling of fractional melts of mantle material from the region above subducted lithospheric slabs leads to the generation of new oceanic lithosphere behind island arcs. The general case for this tectonic setting involves random location of magma leaks and does not produce correlatable magnetic anomalies. In special cases, an orthogonal ridge—transform system may duplicate the magnetic patterns found on ocean-basin crust.

2. (2) The second tectonic setting develops on very long “leaky” transform faults separating spreading ridges. In areas where the transform has dislocated a block of continental crust, or an island arc, the map view of the resulting marginal basin may resemble the setting of a basin behind an active island arc. However, the “leaky” transform setting is unrelated to active plate convergence or to Benioff zones.

At “normal” ridge-crests, and possibly in some marginal basins, basalt is erupted on long linear magma leaks and rapid cooling forms thick lithosphere with correlatable linear magnetic anomalies. Some marginal basins have high thermal flux, spread slowly and may have thick sediment cover. Slow cooling, numerous point-source magma leaks and extensive hydrothermal alteration diminish magnetic intensities and cause diffuse magnetic patterns. The correlation problems caused by diffuse magnetic anomalies make interpretations of spreading rates and directions in young marginal basins a difficult, if not futile, task.It is likely that fragments of marginal-basin lithosphere form some of the ophiolite complexes; their recognition is critical to paleo-tectonic interpretations. The geochemical characteristics of marginal-basin basalts do not appear to be useful criteria for distinguishing them from ocean-ridge basalts. However, the abundance of short ridges and seamounts in many young marginal basins suggests that an abundance of seamount material, as well as differentiated volcanic and plutonic rocks, in ophiolites may be an indication of derivation from marginal-basin lithosphere.  相似文献   

The Role of a PhD Field Exam in Preparing Graduate Students for Academic Careers*     

Alex P. Oberle  Wendy Bigler  Timothy W. Hawkins 《The Professional geographer》2005,57(3):452-461

The Department of Geography at Arizona State University implemented a field exam as part of its PhD program requirements. This field exam requires students to develop an independent field‐based research project based on a general question in the student's specialty area. A survey of current and former PhD students and faculty members document how the field exam assists students in developing skills necessary for continuing graduate research and for preparing them for the rigors of academic employment. The outcomes of the exam include both long‐term, process‐related benefits and more immediate tangible rewards. For some students, the preliminary fieldwork and results redirect student interests and form the basis for their eventual dissertation. The field exam is adaptable to a diversity of geography research methods, subject areas, and graduate degree programs, while remaining grounded in the discipline's vibrant, widely respected fieldwork tradition.  相似文献   

Cross polarization, magic-angle spinning C nuclear magnetic resonance spectroscopy of soil humic fractions     

C. Saiz-Jimenez  Bruce L. Hawkins  Gary E. Maciel   《Organic Geochemistry》1986,9(6)

Cross polarization, magic-angle spinning ¹³C nuclear magnetic resonance spectroscopy was used to characterize humic fractions isolated from different soils. The acid fractions are more aromatic than the humin fractions, probably due to the higher polyssaccharide content of humins. However, fulvic acid fractions are more aromatic than the corresponding humic acid and humin fractions. These results can be interpreted in terms of the isolation procedure, because the high affinity of Polyclar AT for phenols results in higher aromaticities as compared with other isolation methods (e.g. charcoal).  相似文献   

Petrology and geochemistry of boninite series volcanic rocks from the Mariana trench   总被引：4，自引：0，他引：4  

Sherman H. Bloomer  James W. Hawkins 《Contributions to Mineralogy and Petrology》1987,97(3):361-377

Boninite series volcanic rocks have been recovered from three dredge hauls on the inner slope of the Mariana Trench. These hauls included olivine boninites, boninites, boninitic andesites and boninitic dacites, as well as island arc tholeiitic basalts and andesites. The boninite series volcanics range from 52 to 68% SiO₂, and are characterized by very low abundances of high-field-strength cations and heavy-rare-earth elements. Boninites and olivine boninites have phenocrysts of olivine and orthopyroxene, the andesites phenocrysts of orthopyroxene and clinopyroxene, and the dacites orthopyroxene, clinopyroxene, and plagioclase. Most of the major and trace element variation in the series from boninite to boninitic dacite can be modelled by fractionation of olivine, orthopyroxene, clinopyroxene, and plagioclase in the proportions 2.5412, leaving 47% residual liquid. The fractionation must be in part open-system: reverse zoned phenocrysts, resorbed olivine and plagioclase xenocrysts, and bulk rock compositions which cannot be fit by simple closed system crystallization indicate some magma mixing and phenocryst accumulation. Two boninitic magma stems can be identified, with similar high-field-strength element abundances, but different amounts of Ca, Na, Al and light-rare-earth elements. There is also evidence for a magma stem transitional in chemistry from the boninites to arc tholeiites. The compositions of these boninites are consistent with hypotheses for boninite formation by partial melting of a depleted mantle mixed with an incompatible element enriched fluid. The Mariana forearc boninite series lacks a strong iron enrichment, but produces andesites with lower Ti, Al and Y/Zr, and higher Mg, Ni and Cr than typical calcalkaline arc andesites and dacites. Boninites in the Mariana system were erupted only in the earliest phases of subduction zone activity.  相似文献   

Planetary rings,by Larry W. Esposito     

Guy Consolmagno SJ 《Meteoritics & planetary science》2007,42(2):301-302

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