The Einstein polarization interferometer for cosmology (EPIC) and the millimeter-wave bolometric interferometer (MBI)     

P.T. Timbie  G.S. Tucker  P.A.R. Ade  S. Ali  E. Bierman  E.F. Bunn  C. Calderon  A.C. Gault  P.O. Hyland  B.G. Keating  J. Kim  A. Korotkov  S.S. Malu  P. Mauskopf  J.A. Murphy  C. O&#x;Sullivan  L. Piccirillo  B.D. Wandelt 《New Astronomy Reviews》2006,50(11-12):999

We provide an overview of a mission concept study underway for the Einstein Inflation Probe (EIP). Our study investigates the advantages and tradeoffs of using an interferometer (EPIC) for the mission. We also report on the status of the millimeter-wave bolometric interferometer (MBI), a ground-based pathfinder optimized for degree-scale CMB polarization measurements at 90 GHz.  相似文献   

山东诸城晚白垩世王氏群恐龙化石层碎屑锆石定年和物源示踪   总被引：2，自引：0，他引：2  

安伟  旷红伟  柳永清  彭楠  许克民  许欢  章朋  王克柏  陈树清  张艳霞 《地质论评》2016,62(2):423-471

山东东部诸城晚白垩世王氏群大面积、高密度集群埋藏的恐龙化石是近年研究的热点,但其沉积物源与精确沉积时限目前尚不明确。本文通过对山东诸城王氏群恐龙化石层中6个砂岩样品的碎屑锆石U-Pb定年表明,样品090414-24-D中最年轻的单颗粒锆石年龄(YSG)为77.3 Ma,应代表王氏群恐龙化石层的最大沉积时限(下限),结合前人对王氏群红土崖组的年代学研究表明,其沉积时限应老于73.5 Ma(上限),也说明赋存恐龙化石层的王氏群上部红土崖组为Campanian期沉积;碎屑锆石定年揭示物源的锆石年龄组成分布在100～130 Ma之间,6个样品的年龄主峰值多在110 Ma或120 Ma左右,与下伏的早白垩世青山群火山岩年龄主峰较为吻合。王氏群恐龙化石层砾岩的砾石成分和古水流研究显示,其中3组砾石统计表明砾岩层砾石成分主要由火山岩或火山碎屑岩组成,3组古水流数据表明,诸城地区王氏群红土崖组砾岩层的古流向以南和南东方向为主,尚有1组显示古流向为向北,表明王氏群物源主要来自盆地北侧莱阳和北西侧沂沭断裂带的青山群火山岩,其次为盆地南缘。本研究为诸城王氏群化石层沉积时限的限定和沉积物源的判断,以及胶莱盆地王氏群时期古地理格局的恢复等提供了重要的依据。  相似文献   

Mitigating depletion of a porous geothermal aquifer in the Pannonian sedimentary basin     

Nina Rman  Andrej Lapanje  Joerg Prestor  Michael J. O’Sullivan 《Environmental Earth Sciences》2016,75(8):723

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Geophysical applications across the US Critical Zone Observatories (CZO) and future CZOs for the pan-Canadian EON-ROSE research initiative     

Katherine Boggs  Nicole West  Pamela Sullivan  Edward Johnson 《《地质学报》英文版》2018,92(Z1):154-155

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Shallow groundwater response to rainfall on a forested headwater catchment in northern coastal California: implications of topography,rainfall, and throughfall intensities on peak pressure head generation          下载免费PDF全文

Amod S. Dhakal  Kate Sullivan 《水文研究》2014,28(3):446-463

The pore water pressure head that builds in the soil during storms is a critical factor for the prediction of potential slope instability. We report findings from a 3‐year study of pressure head in 83 piezometers distributed within a 13‐ha forested catchment on the northern coast of California. The study's primary objective was to observe the seasonal and storm‐based dynamics of pressure head at a catchment scale in relation to observed rainfall characteristics and in situ topography to better understand landscape patterns of pressure head. An additional goal was to determine the influence of the interaction between rainfall and forest canopy in altering delivery of water and pressure head during the large storms necessary to induce landsliding. We found that pressure head was highly variable in space and time at the catchment scale. Pore pressures peaked close to maximum rainfall intensity during the largest storms measured. The difference between rainfall and throughfall delivered through the canopy was negligible during the critical landslide‐producing peak rainfall periods. Pore pressure was spatially variable within the catchment and did not strongly correlate with surficial topographic features. Only 23% of the piezometers located in a variety of slope positions were found to be highly responsive to rainfall. Topographic index statistically explained peak pressure head at responsive locations during common storms, but not during the larger storms with potential to produce landslides. Drainage efficiency throughout the catchment increased significantly in storms exceeding 2 to 7 months peak pressure head return period indicated by slowing or cessation of the rate of increase of pressure head with increasing storm magnitude. This asymptotic piezometric pattern persisted through the largest storm measured during the study. Faster soil drainage suppressed pressure head response in larger storms with important process implications for pore pressure development and landslide hazard modelling. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

Spatial and temporal changes in estuarine water quality during a post-flood hypoxic event     

Vanessa N.L. Wong  Scott G. Johnston  Richard T. Bush  Leigh A. Sullivan  Christina Clay  Edward D. Burton  Peter G. Slavich 《Estuarine, Coastal and Shelf Science》2010

A major fish kill occurred in the Richmond River estuary in January 2008 due to oxygen depletion following extensive overbank flooding. This paper examines spatial and temporal changes in the chemistry of main channel waters, thereby identifying the primary sources of deoxygenating water. Over 40 km of the mid- to lower estuary main channel was deoxygenated within seven days of the flood peak. Hypoxia was confined to downstream of the confluences with mid-estuary backswamp basins and occurred during the later phase of the flood recession. Water chemistry at key locations in the estuary indicated elevated concentrations of redox sensitive species associated with acid sulfate soils (ASS) during the hypoxic period. Peak concentrations of Fe²⁺ up to 18.2 μmol L⁻¹, dissolved Mn up to 4.3 μmol L⁻¹, chemical oxygen demand (COD) up to 2052 μmol L⁻¹, dissolved organic carbon (DOC) up to 960 μmol L⁻¹ and elemental S⁰ up to 4.7 μmol L⁻¹ were found in the backswamp discharge confluences and mid-estuary main channel locations. The geochemical signature of main channel floodwaters identifies anaerobic decomposition of floodplain vegetation in ASS backswamps as a primary process leading to generation of hypoxic waters. The transport of these hypoxic floodwaters to the estuary has been accelerated and prolonged by extensive floodplain drainage, thereby enhancing the magnitude and duration of estuarine deoxygenation.  相似文献   

Early diagenesis in rapidly accumulating sediments on the Alboran slope, ODP site 976     

Stefano M. Bernasconi  Philip A. Meyers  Gerard O’Sullivan 《Geo-Marine Letters》1998,18(3):209-214

The oxidation and reduction that occur during early diagenesis of sediments has been studied in the interstitial waters of a rapidly accumulating sedimentary sequence from the Mediterranean margin of Spain. A series of reactions that are mediated by progressively lower free energy derived from oxidation of organic matter is evident in the sedimentary sequence. Iron and manganese are rapidly reduced. Phosphate and alkalinity maxima at a subbottom depth of 15?m indicate maximal organic matter degradation. Methane first appears at ～20?m subbottom after sulfate is depleted, and its concentrations quickly climb.  相似文献   

Discovering SNPs in Protein Coding Regions with StellaSNP: Illustrating the Characterization and Geographic Distribution of Polymorphisms in the Estuarine Anemone <Emphasis Type="Italic">Nematostella vectensis</Emphasis>     

Adam M. Reitzel  James C. Sullivan  John R. Finnerty 《Estuaries and Coasts》2010,33(4):930-943

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RT sculptoris: An important star for low-mass close binary research     

Timothy Banks  Denis J. Sullivan  Edwin Budding 《Astrophysics and Space Science》1990,173(1):77-92

TheUBV light curves of Duerbeck and Karimie (1979) for the southern eclipsing binary RT Sculptoris were analysed using information limit optimizing computer programs. We decide in favour of the transit primary minimum hypothesis. The system is found to be semi-detached, but in the rare primary contact configuration. This implies a fast mass transfer process. Our derived picture of the system broadly corroborates that of Hilditch and King (1986), but our analysis includes a detailed treatment of the hot spot. We also report on recent spectroscopic radial velocity data obtained at Mt. Stromlo, Canberra. The system provides an important case study for low mass close binary research.  相似文献   

The EC 14026 stars – V. The pulsation periods of PB 8783     

O'Donoghue  Koen  Solheim  Barstow  Dobbie  O'Brien  Clemens  Sullivan  & Kawaler 《Monthly notices of the Royal Astronomical Society》1998,296(2):296-305

PB 8783 is a member of the newly discovered class of pulsating sdB stars, the EC 14026 stars. The potential of the pulsations of these stars as diagnostic probes of their interiors can only be realized fully by intensive campaigns of multisite time series photometry. To this end we have undertaken a campaign spanning 2 weeks and involving data from five different sites. 183 h of data were obtained. Frequency analysis yielded at least 11 pulsation periods in seven discrete groups between 94 and 136 s. Three of the periods in one specific group are equally spaced in frequency, with a spacing of 0.94 μHz. The frequency spacings amongst the members of other groups are similar to this. A rotation period of ∼12 d is implied. A general scheme for identifying the observed modes is suggested. The periods from a detailed model are in good overall agreement with the observed periods, but some difficulties remain. Three additional periods in the range 61–63 s, and with very low amplitude, were also found. No convincing interpretation of these could be devised.  相似文献