Petrography and geochemistry of ejecta from the Sudbury impact event     

Matthew S. Huber  Iain McDonald  Christian Koeberl 《Meteoritics & planetary science》2014,49(10):1749-1768

Ejecta from the Connors Creek site in Michigan (500 km from the Sudbury Igneous Complex [SIC]), the Pine River site in western Ontario (650 km from the SIC), and the Coleraine site in Minnesota (980 km from the SIC) were petrographically and geochemically analyzed. Connors Creek was found to have approximately 2 m of ejecta, including shocked quartz, melt droplets, and accretionary lapilli; Pine River has similar deposits about 1 m in thickness, although with smaller lapilli; Coleraine contains only impact spherules in a 20 cm‐thick layer (impact spherules being similar to microkrystites or microtektites). The ejecta transition from chaotic deposits of massively bedded impactoclastic material with locally derived detritus at Connors Creek to a deposit with apparently very little detrital material that is primarily composed of melt droplets at Pine River to a deposit that is almost entirely composed of melt spherules at Coleraine. The major and trace element compositions of the ejecta confirm the previously observed similarity of the ejecta deposits to the Onaping Formation in the SIC. Platinum‐group element (PGE) concentrations from each of the sites were also measured, revealing significantly elevated PGE contents in the spherule samples compared with background values. PGE abundances in samples from the Pine River site can be reproduced by addition of approximately 0.2 wt% CI chondrite to the background composition of the underlying sediments in the core. PGE interelement ratios indicate that the Sudbury impact event was probably caused by a chondritic impactor.  相似文献   

River network travel time is correlated with dissolved organic matter composition in rivers of the contiguous United States     

Jacob D. Hosen  George H. Allen  Giuseppe Amatulli  Sara Breitmeyer  Matthew J. Cohen  Byron C. Crump  YueHan Lu  Jérôme P. Payet  Brett A. Poulin  Aron Stubbins  Byungman Yoon  Peter A. Raymond 《水文研究》2021,35(5):e14124

Most terrestrial allochthonous organic matter enters river networks through headwater streams during high flow events. In headwaters, allochthonous inputs are substantial and variable, but become less important in streams and rivers with larger watersheds. As allochthonous dissolved organic matter (DOM) moves downstream, the proportion of less aromatic organic matter with autochthonous characteristics increases. How environmental factors converge to control this transformation of DOM at a continental scale is less certain. We hypothesized that the amount of time water has spent travelling through surface waters of inland systems (streams, rivers, lakes, and reservoirs) is correlated to DOM composition. To test this hypothesis, we used established river network scaling relationships to predict relative river network flow-weighted travel time (FWTT) of water for 60 stream and river sites across the contiguous United States (3090 discrete samples over 10 water years). We estimated lentic contribution to travel times with upstream in-network lake and reservoir volume. DOM composition was quantified using ultraviolet and visible absorption and fluorescence spectroscopy. A combination of FWTT and lake and reservoir volume was the best overall predictor of DOM composition among models that also incorporated discharge, specific discharge, watershed area, and upstream channel length. DOM spectral slope ratio (R² = 0.77) and Freshness Index (R² = 0.78) increased and specific ultraviolet absorbance at 254 nm (R² = 0.68) and Humification Index (R² = 0.44) decreased across sites as a function of FWTT and upstream lake volume. This indicates autochthonous-like DOM becomes continually more dominant in waters with greater FWTT. We assert that river FWTT can be used as a metric of the continuum of DOM composition from headwaters to rivers. The nature of the changes to DOM composition detected suggest this continuum is driven by a combination of photo-oxidation, biological processes, hydrologically varying terrestrial subsidies, and aged groundwater inputs.  相似文献   

The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations     

Vivienne Wild  John A. Peacock  Ofer Lahav  Edward Conway  Steve Maddox  Ivan K. Baldry  Carlton M. Baugh  Joss Bland-Hawthorn  Terry Bridges  Russell Cannon  Shaun Cole  Matthew Colless  Chris Collins  Warrick Couch  Gavin Dalton  Roberto De Propris  Simon P. Driver  George Efstathiou  Richard S. Ellis  Carlos S. Frenk  Karl Glazebrook  Carole Jackson  Ian Lewis  Stuart Lumsden  Darren Madgwick  Peder Norberg  Bruce A. Peterson  Will Sutherland  Keith Taylor 《Monthly notices of the Royal Astronomical Society》2005,356(1):247-269

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The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z= 0.6     

David A. Wake  Robert C. Nichol  Daniel J. Eisenstein  Jon Loveday  Alastair C. Edge  Russell Cannon  Ian Smail  Donald P. Schneider  Ryan Scranton  Daniel Carson  Nicholas P. Ross  Robert J. Brunner  Matthew Colless  Warrwick J. Couch  Scott M. Croom  Simon P. Driver  José da Ângela  Sebastian Jester  Roberto de Propris  Michael J. Drinkwater  Joss Bland-Hawthorn  Kevin A. Pimbblet  Isaac G. Roseboom  Tom Shanks  Robert G. Sharp  Jon Brinkmann 《Monthly notices of the Royal Astronomical Society》2006,372(2):537-550

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The GLARE Survey – II. Faint z≈ 6 Lyα line emitters in the HUDF     

Elizabeth R. Stanway †  rew J. Bunker  Karl Glazebrook  Roberto G. Abraham  James Rhoads  Sangeeta Malhotra  David Crampton  Matthew Colless  Kuenley Chiu 《Monthly notices of the Royal Astronomical Society》2007,376(2):727-738

The galaxy population at   z ≈ 6  has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) – the deepest imaging survey yet. A large number of high-redshift galaxy candidates have been identified within the HUDF, but until now analysis of their properties has been hampered by the difficulty of obtaining spectroscopic redshifts for these faint galaxies. Our 'Gemini Lyman-Alpha at Reionization Era' (GLARE) project has been designed to undertake spectroscopic follow-up of faint  ( z ' < 28.5)  i '-drop galaxies at   z ≈ 6  in the HUDF. In a previous paper we presented preliminary results from the first 7.5 h of data from GLARE. In this paper we detail the complete survey. We have now obtained 36 h of spectroscopy on a single GMOS slitmask from Gemini-South, with a spectral resolution of  λ/Δλ_FWHM≈ 1000  . We identify five strong Lyα emitters at   z > 5.5  , and a further nine possible line emitters with detections at lower significance. We also place tight constraints on the equivalent width of Lyα emission for a further ten i '-drop galaxies and examine the equivalent width distribution of this faint spectroscopic sample of   z ≈ 6  galaxies. We find that the fraction of galaxies with little or no emission is similar to that at   z ≈ 3  , but that the   z ≈ 6  population has a tail of sources with high rest-frame equivalent widths. Possible explanations for this effect include a tendency towards stronger line emission in faint sources, which may arise from extreme youth or low metallicity in the Lyman-break population at high redshift, or possibly a top-heavy initial mass function.  相似文献   

Studying reionization with Lyα emitters     

Matthew McQuinn  Lars Hernquist  Matias Zaldarriaga  Suvendra Dutta 《Monthly notices of the Royal Astronomical Society》2007,381(1):75-96

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Use of fused airborne scanning laser altimetry and digital map data for urban flood modelling     

David C. Mason  Matthew S. Horritt  Neil M. Hunter  Paul D. Bates 《水文研究》2007,21(11):1436-1447

Flood modelling of urban areas is still at an early stage, partly because until recently topographic data of sufficiently high resolution and accuracy have been lacking in urban areas. However, digital surface models (DSMs) generated from airborne scanning laser altimetry (LiDAR) having sub‐metre spatial resolution have now become available, and these are able to represent the complexities of urban topography. This paper describes the development of a LiDAR post‐processor for urban flood modelling based on the fusion of LiDAR and digital map data. The map data are used in conjunction with LiDAR data to identify different object types in urban areas, though pattern recognition techniques are also employed. Post‐processing produces a digital terrain model (DTM) for use as model bathymetry, and also a friction parameter map for use in estimating spatially distributed friction coefficients. In vegetated areas, friction is estimated from LiDAR‐derived vegetation height, and (unlike most vegetation removal software) the method copes with short vegetation less than ～1 m high, which may occupy a substantial fraction of even an urban floodplain. The DTM and friction parameter map may also be used to help to generate an unstructured mesh of a vegetated urban floodplain for use by a two‐dimensional finite element model. The mesh is decomposed to reflect floodplain features having different frictional properties to their surroundings, including urban features (such as buildings and roads) and taller vegetation features (such as trees and hedges). This allows a more accurate estimation of local friction. The method produces a substantial node density due to the small dimensions of many urban features. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

Mid-Holocene vertebrate bone Concentration-Lagerstätte on oceanic island Mauritius provides a window into the ecosystem of the dodo (Raphus cucullatus)     

Kenneth F. Rijsdijk  Julian P. Hume  Frans Bunnik  F.B. Vincent Florens  Claudia Baider  Beth Shapiro  Johannes van der Plicht  Anwar Janoo  Owen Griffiths  Lars W. van den Hoek Ostende  Holger Cremer  Tamara Vernimmen  Perry G.B. De Louw  Assenjee Bholah  Salem Saumtally  Nicolas Porch  James Haile  Mike Buckley  Matthew Collins  Edmund Gittenberger 《Quaternary Science Reviews》2009,28(1-2):14-24

Although the recent history of human colonisation and impact on Mauritius is well documented, virtually no records of the pre-human native ecosystem exist, making it difficult to assess the magnitude of the changes brought about by human settlement. Here, we describe a 4000-year-old fossil bed at Mare aux Songes (MAS) in south-eastern Mauritius that contains both macrofossils (vertebrate fauna, gastropods, insects and flora) and microfossils (diatoms, pollen, spores and phytoliths). With >250 bone fragments/m² and comprising 50% of all known extinct and extant vertebrate species (n_s = 44) of Mauritius, MAS may constitute the first Holocene vertebrate bone Concentration-Lagerstätte identified on an oceanic volcanic island. Fossil remains are dominated by extinct giant tortoises Cylindraspis spp. (63%), passerines (～10%), small bats (7.8%) and dodo Raphus cucullatus (7.1%). Twelve radiocarbon ages [four of them duplicates] from bones and other material suggest that accumulation of fossils took place within several centuries. An exceptional combination of abiotic conditions led to preservation of bones, bone collagen, plant tissue and microfossils. Although bone collagen is well preserved, DNA from dodo and other Mauritian vertebrates has proved difficult. Our analysis suggests that from ca 4000 years ago (4 ka), rising sea levels created a freshwater lake at MAS, generating an oasis in an otherwise dry environment which attracted a diverse vertebrate fauna. Subsequent aridification in the south-west Indian Ocean region may have increased carcass accumulation during droughts, contributing to the exceptionally high fossil concentration. The abundance of floral and faunal remains in this Lagerstätte offers a unique opportunity to reconstruct a pre-human ecosystem on an oceanic island, providing a key foundation for assessing the vulnerability of island ecosystems to human impact.  相似文献   

Lieutenant-Colonel Delmé-Radcliffe's report on the 1906 eruption of Vesuvius,Italy: Some further comments and some corrections of an historical nature     

Matthew S. Seligmann 《Journal of Volcanology and Geothermal Research》2009,179(3-4):270-271

The report on the 1906 eruption of Vesuvius by Lieutenant-Colonel Charles Delmé-Radcliffe was reproduced with comments in a 2007 edition of this journal. This article supplies additional details about this report, explaining that the report is, in fact, incomplete and why this is the case. It also corrects some of the comments about the accessibility and previous publication of this report made in the 2007 article.  相似文献   

The missing metals problem – III. How many metals are expelled from galaxies?     

Nicolas Bouché  Matthew D. Lehnert  Anthony Aguirre  Céline Péroux  Jacqueline Bergeron 《Monthly notices of the Royal Astronomical Society》2007,378(2):525-540

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