Further classification of ordinary chondrites from the Monnig Collection     

Arthur J. Ehlmann  Klaus Keil 《Meteoritics & planetary science》1994,29(1):71-73

Abstract— Four ordinary chondrites from the Oscar Monnig Meteorite Collection were classified into compositional groups, petrologic types, and shock stages: Wray (b), Colorado, L5S2; Round Top (a), Texas, L5S3; Round Top (b), Texas, H4S3; Hassayampa, Arizona, H4S3.  相似文献   

Reply to comments by G. Gust on ‘mean flow and turbulence scaling in a tidal boundary layer’     

Thomas F. Gross  Arthur R.M. Nowell 《Continental Shelf Research》1985,4(5):541-545

  相似文献   

Detailed data for 259 fireballs from the Canadian camera network and inferences concerning the influx of large meteoroids     

Ian Halliday  Arthur A. Griffin  Alan T. Blackwell 《Meteoritics & planetary science》1996,31(2):185-217

Abstract— We present data for 259 meteoric fireballs observed with the Canadian camera network, including velocities, heights, orbits, luminosities along each trail, estimates of preatmospheric masses and surviving meteorites (if any) as well as membership in meteor showers. Some 213 of the events comprise an unbiased sample of the 754 fireballs observed in a total of 1.51 × 10¹⁰ km² h of clear-sky observations. The number of fireballs and the amount of clear sky in which they were recorded are given for each day of the year. We find at least 37% of the unbiased sample are members of some 15 recognized meteor showers. Preatmospheric masses, based on an assumed luminous efficiency of 0.04 for velocities >10 km s^?1, range from 1 g for some very fast fireballs up to hundreds of kilograms for the largest events. We present plots and equations for the flux, as a function of initial mass, for the entire group of fireballs and for some subgroups: meteorite-dropping objects; meteor shower members; groups that appear to be mainly of asteroidal or cometary origin; and for very fast objects. For masses of a few kilograms, asteroidal objects outnumber cometary ones. Cometary objects attain greater peak brightness than asteroidal ones of equal mass largely due to higher velocity, but also because they fragment more severely. For 66 fireballs, we estimate the meteoroid density using photometric and dynamic masses. Presumed cometary objects have typical densities near 1.0, while asteroidal values show two groups that suggest meteoroids similar to carbonaceous and ordinary chondrites. Our basic data may be used by others for further studies or to reexamine our results using assumptions different from those employed in this paper.  相似文献   

Classification of Six Ordinary Chondrites from Texas     

Arthur J. Ehlmann  Klaus Keil 《Meteoritics & planetary science》1988,23(4):361-364

Abstract— Based on optical microscopy, modal and electron microprobe analyses, six ordinary chondrites from Texas preserved in the Monnig Meteorite Collection at Texas Christian University, Fort Worth, Texas, were classified in compositional groups, petrologic types, and shock facies. These meteorites are Comanche (stone), L5c; Haskell, L5c; Deport (a), H4b; Naruna (a), H4b; Naruna (b), H4b; and Clarendon (b), H5d.  相似文献   

Quantification of co-occurring reaction rates in deep subseafloor sediments     

Guizhi Wang  Arthur J. Spivack  Uri Manor  Steven D’Hondt 《Geochimica et cosmochimica acta》2008,72(14):3479-3488

Net rates of biogeochemical reactions in subseafloor sediments can be quantified from concentration profiles of dissolved reactants or products and physical properties of the sediment. To study net rates of microbial activities in deep sediments, we developed a robust approach that is well suited to use over a broad range of sediment depths. Our approach is based on a finite-difference solution to a continuity equation that considers molecular diffusion, sediment burial, fluid advection, and reaction under the assumption of steady state. Numerical procedures are adopted to identify the maximum number of depth intervals with statistically different reaction rates. The approach explicitly considers downcore variation in physical properties and sample spacing. Uncertainties in the rate estimates are quantified using a Monte Carlo technique. We tested our approach using synthetic concentration profiles generated from analytical solutions to the continuity equation. We then applied the approach to concentration profiles of dissolved sulfate, sulfide, methane, and manganese in the 420-m thick sediment column of eastern equatorial Pacific Ocean Drilling Program Site 1226. Our results indicate that (i) sulfate reduction and iron reduction occur at most sediment depths, (ii) net methane production occurs in discrete depth intervals and (iii) manganese reduction occurs near the seafloor and deep in the sediments. These results provide quantitative evidence that multiple respiration pathways co-exist in the same depth intervals of these deep subseafloor sediments.  相似文献   

A study of two mid-crustal bright spots from southeast Georgia (USA)     

Arthur E. Barnes  Timothy J. Reston 《Geophysical Journal International》1992,108(2):683-691

  相似文献   

Palynofacies, coal petrographic facies and depositional environments: Amphitheatre formation (Eocene to Oligocene) and Ravenscrag Formation (Maastrichtian to Paleocene), Canada     

Arthur R. Sweet  Alexander R. Cameron 《International Journal of Coal Geology》1991,19(1-4)

Low rank coals from two disparate geological settings have been subjected to petrographic and palynological analysis. The stratigraphic units studied and their locations are the Amphitheatre Formation, St Elias Mountains, Yukon Territory, of Eocene to Oligocene age; and the base of the Ravenscrag Formation, south-central Saskatchewan, of latest Cretaceous to earliest Paleocene age.The depositional setting of the Amphitheatre Formation ranges from distal sand-dominated braided stream and lacustrine environments to proximal gravel-dominated fluvial environments. The coals are low in inertinite (< 6%) and mostly high in huminite (> 85%). In localities with a dominance of angiosperm pollen the relative abundance of eu-ulminite B and densinite is greatest whereas in the ones with a dominantly coniferous pollen assemblage eu-ulminite A is the most prominent maceral. These observations suggest as an immediate cause/effect relationship, an at least partial dependance of present maceral content on floral precursors. This in turn probably reflects a certain combination of depositional environment conditions (pH, Eh, temperature, etc.), that likely controlled the plant community and the preservation of vegetal matter.The depositional environment of coals from the basal part of the Ravenscrag Formation contrasts sharply with that of the Amphitheatre. The Ravenscrag coals formed within a low energy, stable, floodplain environment. Palynological and coal maceral profiles for the basal Ravenscrag Formation coal, which spans the Cretaceous-Tertiary boundary, indicates that the environment of deposition progressed from an open canopied swamp forest with areas of open water, through a phase of low-lying to open water swamps with herbaceous, pterophytic vegetation to, at least locally, raised bogs. The change in coal petrography across the Cretaceous-Tertiary boundary is shown to be relatively minor in comparison to subsequent changes in coal petrography in the earliest Paleocene and to changes that occur in the palynological assemblages across the boundary interval.  相似文献   

Fumarolic activity of Avachinsky and Koryaksky volcanoes, Kamchatka, from 1993 to 1994   总被引：1，自引：0，他引：1  

Yuri A. Taran  Charles B. Connor  Vyacheslav N. Shapar  Alexandre A. Ovsyannikov  Arthur A. Bilichenko 《Bulletin of Volcanology》1997,58(6):441-448

 Volcanic gas and condensate samples were collected in 1993–1994 from fumaroles of Koryaksky and Avachinsky, basaltic andesite volcanoes on the Kamchatka Peninsula near Petropavlovsk–Kamchatsky. The highest-temperature fumarolic discharges, 220  °C at Koryaksky and 473  °C at Avachinsky, are water-rich (940–985 mmol/mol of H₂O) and have chemical and isotopic characteristics typical of Kamchatka–Kurile, high- and medium-temperature volcanic gases. The temperature and chemical and water isotopic compositions of the Koryaksky gases have not changed during the past 11 years. They represent an approximate 2 : 1 mixture of magmatic and meteoric end members. Low-temperature, near-boiling-point discharges of Avachinsky Volcano are water poor (≈880 mmol/mol); Their compositions have not changed since the 1991 eruption, and are suggested to be derived from partially condensed magmatic gases at shallow depth. Based on a simple model involving mixing and single-step steam separation, low water and high CO₂ contents, as well as the observed Cl concentration and water isotopic composition in low-temperature discharges, are the result of near-surface boiling of a brine composed of the almost pure condensed magmatic gas. High methane content in low-temperature Avachinsky gases and the 220  °C Koryaksky fumarole, low C isotopic ratio in CO₂ at Koryaksky (–11.8‰), and water isotope data suggest that the "meteoric" end member contains considerable amounts of the regional methane-rich thermal water discovered in the vicinity of both volcanoes. Received: 2 May 1996 / Accepted: 5 November 1996  相似文献   

Multi-fidelity meta-modeling for reservoir engineering - application to history matching     

Arthur Thenon  Véronique Gervais  Mickaële Le Ravalec 《Computational Geosciences》2016,20(6):1231-1250

Defining representative reservoir models usually calls for a huge number of fluid flow simulations, which may be very time-consuming. Meta-models are built to lessen this issue. They approximate a scalar function from the values simulated for a set of uncertain parameters. For time-dependent outputs, a reduced-basis approach can be considered. If the resulting meta-models are accurate, they can be called instead of the flow simulator. We propose here to investigate a specific approach named multi-fidelity meta-modeling to reduce further the simulation time. We assume that the outputs of interest are known at various levels of resolution: a fine reference level, and coarser levels for which computations are faster but less accurate. Multi-fidelity meta-models refer to co-kriging to approximate the outputs at the fine level using the values simulated at all levels. Such an approach can save simulation time by limiting the number of fine level simulations. The objective of this paper is to investigate the potential of multi-fidelity for reservoir engineering. The reduced-basis approach for time-dependent outputs is extended to the multi-fidelity context. Then, comparisons with the more usual kriging approach are proposed on a synthetic case, both in terms of computation time and predictivity. Meta-models are computed to evaluate the production responses at wells and the mismatch between the data and the simulated responses (history matching error), considering two levels of resolution. The results show that the multi-fidelity approach can outperform kriging if the target simulation time is small. Last, its potential is evidenced when used for history matching.  相似文献   

Metamorphic assemblages and the direction of flow metamorphic fluids in four instances of serpentinization     

Dr. I. Barnes  John B. Rapp  James R. O'Neil  Richard A. Sheppard  Arthur J. Gude III 《Contributions to Mineralogy and Petrology》1973,38(1):80-80

  相似文献