A method for generating uniform size-segregated pyrite particle fractions     

Amy L Wolfe  Ran Liu  Brian W Stewart  Rosemary C Capo  David A Dzombak 《Geochemical transactions》2007,8(1):9

Background  

Standardized sample preparation techniques allow comparison of pyrite dissolution experiments under diverse conditions. Our objective was to assess dry and wet sieving preparation methodologies, and to develop a reproducible technique that yields uniformly size-distributed material within a limited size range of interest.  相似文献   

Predation on the rocky shores of Patagonia,Argentina     

Fernando J. Hidalgo  Brian R. Silliman  María Cielo Bazterrica  Mark D. Bertness 《Estuaries and Coasts》2007,30(5):886-894

Rocky intertidal communities of Argentinean Patagonia are exposed to harsh physical conditions caused by dry, strong southern trade winds (mean speed 45 km h^-1, gusts up to 140 km h^-1) that result in intense desiccation of intertidal organisms. Predator distributions in these communities were evaluated from April 2003 to December 2004 at two exposed headlands and six protected bays in Cabo dos Bahias (44°50′S, 65°40′W). Crabs and sea stars dominated the predator assemblage, with occasional scavenger snails and fish also present. During low tide, predators were never found in the open but were always associated with shelter (primarily within mussel beds and coralline algae), suggesting a strong predator dependency on foundation species to buffer them from physical stress. Few predators (mostly crabs) emerged from shelter at high tide. Unlike the larger predators found on Chilean rocky shores, invertebrate predators in this system are diminutive, generally < 2 cm. The lone exception was the newly discovered invasive green crab,Carcinus mamas. Feeding trials, gut content analyses, and visual surveys indicated that native predators feed primarily on small, soft-bodied prey.C. mamas fed on slow-moving and sessile animals, including the super abundant musselPerumytilus purpuratus, with much greater voracity than native predators. Because native intertidal organisms are dependent on mussel beds and coralline algae for shelter from desiccation, successful invasion ofC. mamas may lead to a significant decrease in native diversity by consuming foundation species. This study represents a preliminary survey of predator distributions and feeding habits on the rocky shores of Argentinean Patagonia and provides important baseline data to evaluate trophic linkages and predatory effects on Patagonian rocky shores.  相似文献   

Economic consequences of consideration of permanence, leakage and additionality for soil carbon sequestration projects     

Brian C. Murray  Brent Sohngen  Martin T. Ross 《Climatic change》2007,80(1-2):127-143

This paper introduces, explains, and describes methods for addressing the issues of permanence, leakage, and additionality (PLA) of agricultural soil carbon sequestration (ASCS) activities at the project level. It is important to cast these as project-level issues, because they relate to the integrity and consistency of using location-specific ASCS projects as an offset against GHG emissions generated in other sectors (e.g., energy). The underlying objective is to understand and quantify what the net carbon benefits of an ASCS project are once we account for the fact that (1) the sequestered carbon may be stored impermanently, (2) the project may displace emissions outside the project boundaries (leakage), and (3) the project’s carbon sequestration may not be entirely additional to what would have occurred anyway under business-as-usual (no project) conditions. This article evaluates methods for identifying and estimating PLA and gauges the potential magnitude of these effects on the economic returns to a project. This work reflects ongoing collaborative efforts of the authors and Bruce McCarl (Texas A&M University), Allan Sommer, Jui-Chen Yang, and Laurel Clayton (RTI International), Sandra Brown (Winrock International), Ken Andrasko and Ben DeAngelo (US EPA), and various participants in the World Resources Institute/World Business Council workgroup to develop GHG project reporting protocols. All opinions, errors and omissions are those of the authors only.  相似文献   

New Zealand and International Migration. A Digest and Bibliography Number 3 by Andrew D. Trlin and Paul Spoonley.     

Brian Heenan 《New Zealand geographer》1998,54(2):54-54

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Petrogenesis of late stage magmatism at Hold with Hope, East Greenland     

Rob M. Ellam  Brian G. J. Upton  J. Godfrey Fitton 《Contributions to Mineralogy and Petrology》1998,133(1-2):51-59

The Myggbukta caldera complex and a swarm of basic dykes constitute the latest Tertiary magmatism in the Hold with Hope region, East Greenland. The Sr and Nd isotope ratios of these rocks show coherent variations which extend to high ⁸⁷Sr/⁸⁶Sr and low ¹⁴³Nd/¹⁴⁴Nd values and require a contribution from continental lithosphere. Broad correlations with major element differentiation indices suggest that the continental component was incorporated during magmatic differentiation thereby favouring a crustal contamination process. Trace element concentrations are strongly correlated with isotopic compositions but display ranges for many incompatible elements which extend beyond likely crustal contaminant compositions. This is readily modelled by AFC processes in which the dominant cause of trace element enrichment is the concentration effect of fractional crystallisation rather than the composition of the contaminant. The simplest such models still require unrealistically high degrees of fractional crystallisation to explain the ten-fold enrichment of some trace elements. This can be overcome if the primary magmas entering the crust already had highly variable trace element compositions. Such variability is readily achieved if melts from different parts of the melting column escape without thorough homogenization. An AFC model which incorporates variability in parental magma composition is then able to simulate the range of compositions observed at Hold with Hope. This carries the implication that the variations observed are more readily attributed to changes in uncontaminated parental magma than to variations in the composition or amount of contaminant. Received: 5 March 1998 / Accepted: 16 June 1998  相似文献   

The breakdown of potassium feldspar at high water pressures   总被引：1，自引：0，他引：1  

Pauline Thompson  Ian Parsons  Colin M. Graham  Brian Jackson 《Contributions to Mineralogy and Petrology》1998,130(2):176-186

The equilibrium position of the reaction between sanidine and water to form “sanidine hydrate” has been determined by reversal experiments on well characterised synthetic starting materials in a piston cylinder apparatus. The reaction was found to lie between four reversed brackets of 2.35 and 2.50 GPa at 450 °C, 2.40 and 2.59 GPa at 550 °C, 2.67 and 2.74 GPa at 650 °C, and 2.70 and 2.72 GPa at 680 °C. Infrared spectroscopy showed that the dominant water species in sanidine hydrate was structural H₂O. The minimum quantity of this structural H₂O, measured by thermogravimetric analysis, varied between 4.42 and 5.85 wt% over the pressure range of 2.7 to 3.2 GPa and the temperature range of 450 to 680 °C. Systematic variation in water content with pressure and temperature was not clearly established. The maximum value was below 6.07 wt%, the equivalent of 1 molecule of H₂O per formula unit. The water could be removed entirely by heating at atmospheric pressure to produce a metastable, anhydrous, hexagonal KAlSi₃O₈ phase (“hexasanidine”) implying that the structural H₂O content of sanidine hydrate can vary. The unit cell parameters for sanidine hydrate, measured by powder X-ray diffraction, were a = 0.53366 (±0.00022) nm and c = 0.77141 (±0.00052) nm, and those for hexasanidine were a = 0.52893 (±0.00016) nm and c = 0.78185 (±0.00036) nm. The behaviour and properties of sanidine hydrate appear to be analogous to those of the hydrate phase cymrite in the equivalent barium system. The occurrence of sanidine hydrate in the Earth would be limited to high pressure but very low temperature conditions and hence it could be a potential reservoir for water in cold subduction zones. However, sanidine hydrate would probably be constrained to granitic rock compositions at these pressures and temperatures. Received: 6 May 1997 / Accepted: 2 October 1997  相似文献   

Resonant tidal disruption in galactic nuclei     

Kevin P. Rauch  & Brian Ingalls 《Monthly notices of the Royal Astronomical Society》1998,299(4):1231-1241

It has recently been shown by Rauch 38 Tremaine that the rate of angular momentum relaxation in nearly Keplerian star clusters is greatly increased by a process termed 'resonant relaxation'; it was also argued, via a series of scaling arguments, that tidal disruption of stars in galactic nuclei containing massive black holes could be noticeably enhanced by this process. We describe here the results of numerical simulations of resonant tidal disruption which quantitatively test the predictions made by Rauch 38 Tremaine. The simulation method is based on an N -body routine incorporating cloning of stars near the loss cone and a semirelativistic symplectic integration scheme. Normalized disruption rates for resonant and non-resonant nuclei are derived at orbital energies both above and below the critical energy, and the corresponding angular momentum distribution functions are found. The black hole mass above which resonant tidal disruption is quenched by relativistic precession is determined. We also briefly describe the discovery of chaos in the Wisdom–Holman symplectic integrator applied to highly eccentric orbits and propose a modified integration scheme that remains robust under these conditions. We find that resonant disruption rates exceed their non-resonant counterparts by an amount consistent with the predictions; in particular, we estimate the net tidal disruption rate for a fully resonant cluster to be about twice that of its non-resonant counterpart. No significant enhancement in rates is observed outside the critical radius. Relativistic quenching of the effect is found to occur for hole masses M  >  M _Q  = (8 ± 3) × 10⁷  M . The numerical results combined with the observed properties of galactic nuclei indicate that for most galaxies the resonant enhancement to tidal disruption rates will be very small.  相似文献   

Mineralogy of sedimentary formations in the western North Atlantic Ocean: Preliminary results     

Prof. Dr. Peter Rothe  Dr. Brian E. Tucholke 《International Journal of Earth Sciences》1981,70(1):327-343

Six sedimentary formations, and two separate members recently were described byJansa, et al. (1979) from the western North Atlantic Ocean basin. We have investigated the mineralogical composition of these lithostratigraphic units by qualitative X-ray diffraction analyses of about five hundred samples from DSDP Sites 105, 106, 386, 387, and 391. The sedimentary section studied, from bottom to top, consists of: argillaceous limestones (Cat Gap Formation); limestones (Blake-Bahama Formation); claystones and shales (Hatteras Formation); zeolitic claystones (Plantagenet Formation); nannofossil marls (Crescent Peaks Member); siliceous oozes, clays, and cherts (Bermuda Rise Formation), and hemipelagic muds (Blake Ridge Formation) that locally contain redeposited shallow-water carbonates (Great Abaco Member). The section ranges in age from Oxfordian at the base to Quaternary at the sea-floor.Most of the formations and members described byJansa, et al. (1979) have a characteristic mineralogical composition. Thus it is possible to recognize boundaries between formations and members by changes in mineral components, although these changes range from sharp to transitional. Within the same formation local differences in mineral spectra between sites can be explained by changing distance from terrigenous sources, lateral changes in surface paleoproductivity, and varying diagenetic conditions.

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Zusammenfassung Sechs sedimentäre Formations und zwei dazugehörige Members wurden vor kurzem durchJansa, et al. (1979) aus dem Ozeanboden des westlichen Nordatlantik beschrieben. Wir haben die Mineralzusammensetzung dieser lithostratigraphischen Einheiten anhand von etwa 500 qualitativen röntgenographischen Analysen untersucht; die Proben dazu entstammen den DSDP-Bohrungen 105, 106, 386, 387 und 391. Vom Liegenden zum Hangenden lassen sich folgende Einheiten unterscheiden: Tonige Kalksteine (Cat Gap Formation); Kalksteine (Blake-Bahama Formation); Tonsteine und shales (Hatteras Formation); Zeolithische Tonsteine (Plantagenet Formation); Nannofossil-Mergel (Crescent Peaks Member); Kieselige Schlamme, Tone und Hornsteine (Bermuda Rise Formation) und Hemipelagische Schlamme (Blake Ridge Formation), die lokal umgelagerte Flachwasser-Karbonate (Great Abaco Member) enthalten. Das Gesamtprofil reicht altersmäßig von Oxfordium an der Basis bis zum Quartär.Die meisten der vonJansa, et al. (1979) beschriebenen Formations und Members haben eine charakteristische Mineralzusammensetzung; es ist daher möglich, Grenzen sowohl zwischen Formations als auch zwischen Formations und Members anhand ihrer Mineralkomponenten zu erkennen; der entsprechende Wechsel kann scharf sein oder fließende Übergänge aufweisen. Lokale Unterschiede in den Mineralspektren einer Formation zwischen einzelnen Bohrpunkten lassen sich auf wechselnde Entfernungen vom Liefergebiet bzw. unterschiedliche Liefergebiete selbst, auf laterale Wechsel in der oberflächennahen Paläo-Produktivität und/oder auf unterschiedliche diagenetische Bedingungen zurückführen.

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Résumé Six »formations« sédimentaires ainsi que deux »members« séparés ont été ré cemment décrits parJansa, et al. (1979) dans la partie nordouest du bassin de l'océan Atlantique. Nous avons étudié, d'un point de vue qualitatif, la composition minéralogique de ces unités lithostratigraphiques à partir de l'analyse diffractométrique d'environ 500 échantillons provenant des sites DSDP 105, 106, 386, 387 et 391. Les sections sédimentaires examinées comprennent de bas en haut: Des calcaires argileux (Cat Gap Formation); des calcaires (Blake-Bahama Formation); des argilites et des argiles schisteuses (Hatteras Formation); des argilites zéolitiques (Plantagenet Formation); de la marne aux nannofossiles (Crescent Peaks Member); des boues silicieuses, des argiles et du silex (Bermuda Rise Formation), ainsi que des boues hémipélagiques (Blake Ridge Formation) qui contiennent par endroits des carbonates resédimentaires provenant d'un milieu peu profond (Great Abaco Member). Leur âge s'échelonne de l'Oxfordien à la base jusqu'au Quaternaire au fond océanique.La plupart des »formations« et des »members« décrits parJansa, et al. (1979) ont une composition minéralogique caractéristique. Il est donc possible de reconnaître les limites entre des »formations« et des »members« à partir des changements de la composition minéralogique, bien que ces changements varient du net au transitoire. Dans une même formation on peut expliquer les différences locales des spectres minéraux entre les sites, par la variation de distance des sources terrigènes, des changements latéraux de la paléoproductivité de surface et des conditions diagénétiques variables.

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Jansa . (1979) 6 2 . 500 . 105, 106, 386, 387, 391. : — Cat Gap —, — Blake-Bahama —, — Hatteras'a —, — Plantagenet —, - — Crescent Peaks —, , — Bermuda Rise — — Blake Ridge —, — Great Abaco. . Jansa ; , , , . , ., , / .

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Sorting benthic samples     

Brian E. Barnett 《Marine pollution bulletin》1979,10(8):241-242

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An archaean granulite-grade tonalite-trondhjemite-granite suite from scourie,NW Scotland: Geochemistry and origin     

Hugh R. Rollinson  Brian F. Windley 《Contributions to Mineralogy and Petrology》1980,72(3):265-281

The Lewisian complex of the Scourie-Badcall area is composed predominantly of banded tonalitic gneiss which intrudes layered gabbro-ultramafic complexes. Intrusive into both gabbro and tonalitic gneiss are homogeneous acid sheets which are trondhjemitic to granitic in composition. All rocks were subjected to granulite facies metamorphism. Smooth continuous trends on chemical variation diagrams suggest that the evolution of these rocks was dominated by fractional crystallisation. A scheme is proposed whereby a tonalitic melt was parental to trondhjemite and granite. Variation within tonalites was a function of the fractional crystallisation of hornblende and plagioclase, and trondhjemite was derived from tonalite by the fractional crystallisation of hornblende and/or plagioclase. Granite and granodiorite represent residual liquids which evolved along the quartz-feldspar cotectic surface; they were derived by the fractional crystallisation of plagioclase from a trondhjemite liquid. Some trondhjemitic sheets are quartz-plagioclase residues from which a granitic melt was removed. The associated gabbros and ultramafic rocks are not directly related to the proposed fractional crystallisation scheme and are not crystal residues removed from the tonalitic melt. Tonalites were probably derived from a basaltic source by partial melting or fractional crystallisation with either hornblende and/or garnet as residual phases.  相似文献