SIMS studies of Allende projectiles fired into Stardust‐type aluminum foils at 6 km/sec     

Peter Hoppe  Frank J. Stadermann  Thomas Stephan  Christine Floss  Jan Leitner  Kuljeet K. Marhas  Friedrich Hrz 《Meteoritics & planetary science》2006,41(2):197-209

Abstract— We have explored the feasibility of C, N, and O isotopic measurements by NanoSIMS and of elemental abundance determinations by time‐of‐flight secondary ion mass spectrometry (TOF‐SIMS) on residues of Allende projectiles that impacted Stardust‐type aluminum foils in the laboratory at 6 km/sec. These investigations are part of a consortium study aimed at providing the foundation for the characterization of matter associated with microcraters that were produced during the encounter of the Stardust space probe with comet 81P/Wild‐2. Eleven experimental impact craters were studied by NanoSIMS and eighteen by TOF‐SIMS. Crater sizes were between 3 and 190 μm. The NanoSIMS measurements have shown that the crater morphology has only a minor effect on spatial resolution and on instrumental mass fractionation. The achievable spatial resolution is always better than 200 nm, and C and O isotopic ratios can be measured with a precision of several percent at a scale of several 100 nm, which is the typical size of presolar grains. This clearly demonstrates that presolar matter, provided it survives the impact into the aluminum foil partly intact, is recognizable even if embedded in material of solar system origin. TOF‐SIMS studies are restricted to materials from the crater rim. The element ratios of the major rock‐forming elements in the Allende projectiles are well‐characterized by the TOF‐SIMS measurements, indicating that fractionation of those elements during impact can be expected to be negligible. This permits chemical information on the type of impactor material to be obtained. For any more detailed assignments to specific chondrite groups, however, information on the abundances of the light elements, especially C, is crucial. This information could not be obtained in the present study due to unavoidable contamination during impact experiments.  相似文献   

Modelled impact of global warming on ENSO-driven precipitation changes in the tropical Pacific     

Christine T. Y. Chung  Scott B. Power 《Climate Dynamics》2016,47(3-4):1303-1323

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Application of Genetic Algorithm (GA) in History Matching of the Vapour Extraction (VAPEX) Heavy Oil Recovery Process     

Suxin Xu  Min Zhang  Fanhua Zeng  Christine Chan 《Natural Resources Research》2015,24(2):221-237

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Local perceptions in climate change debates: insights from case studies in the Alps and the Andes     

Christine Jurt  Maria Dulce Burga  Luis Vicuña  Christian Huggel  Ben Orlove 《Climatic change》2015,133(3):511-523

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Vegetation and climate history in the Laptev Sea region (Arctic Siberia) during Late Quaternary inferred from pollen records     

Andrei A. Andreev  Lutz Schirrmeister  Pavel E. Tarasov  Andrey Ganopolski  Viktor Brovkin  Christine Siegert  Sebastian Wetterich  Hans-Wolfgang Hubberten 《Quaternary Science Reviews》2011,30(17-18):2182-2199

Paleoenvironmental records from a number of permafrost sections and lacustrine cores from the Laptev Sea region dated by several methods (¹⁴C-AMS, TL, IRSL, OSL and ²³⁰Th/U) were analyzed for pollen and palynomorphs. The records reveal the environmental history for the last ca 200 kyr. For interglacial pollen spectra, quantitative temperature values were estimated using the best modern analogue method. Sparse grass-sedge vegetation indicating arctic desert environmental conditions existed prior to 200 kyr ago. Dense, wet grass-sedge tundra habitats dominated during an interstadial ca 200–190 kyr ago, reflecting warmer and wetter summers than before. Sparser vegetation communities point to much more severe stadial conditions ca 190–130 kyr ago. Open grass and Artemisia communities with shrub stands (Alnus fruticosa, Salix, Betula nana) in more protected and moister places characterized the beginning of the Last Interglacial indicate climate conditions similar to present. Shrub tundra (Alnus fruticosa and Betula nana) dominated during the middle Eemian climatic optimum, when summer temperatures were 4–5 °C higher than today. Early-Weichselian sparse grass-sedge dominated vegetation indicates climate conditions colder and dryer than in the previous interval. Middle Weichselian Interstadial records indicate moister and warmer climate conditions, for example, in the interval 40–32 kyr BP Salix was present within dense, grass-sedge dominated vegetation. Sedge-grass-Artemisia-communities indicate that climate became cooler and drier after 30 kyr BP, and cold, dry conditions characterized the Late Weichselian, ca 26–16 kyr BP, when grass-dominated communities with Caryophyllaceae, Asteraceae, Cichoriaceae, Selaginella rupestris were present. From 16 to 12 kyr BP, grass-sedge communities with Caryophyllaceae, Asteraceae, and Cichoriaceae indicate climate was significantly warmer and moister than during the previous interval. The presence of Salix and Betula reflect temperatures about 4 °C higher than present at about 12–11 kyr BP, during the Allerød interval, but shrubs were absent in the Younger Dryas interval, pointing to a deterioration of climate conditions. Alnus fruticosa, Betula nana, Poaceae, and Cyperaceae dominate early Holocene spectra. Reconstructed absolute temperature values were substantially warmer than present (up to 12 °C). Shrubs gradually disappeared from coastal areas after 7.6 kyr BP when vegetation cover became similar to modern. A comparison of proxy-based paleoenvironmental reconstructions with the simulations performed by an Earth system model of intermediate complexity (CLIMBER-2) show good accordance between the regional paleodata and model simulations, especially for the warmer intervals.  相似文献   

A simple time-dependent solution of the geomagnetic ring-current problem     

Christine M. Davies 《Geophysical Journal International》1977,50(1):23-28

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Preliminary Results on the 3-dimensional Seismic Structure of the Lithosphere under the USGS Central California Seismic Array     

Eystein S. Husebye  ers Christoffersson  Keiiti Aki  Christine Powell 《Geophysical Journal International》1976,46(2):319-340

About 1500 readings of teleseismic P -time residuals obtained from the US Geological Survey seismograph network in central California have been used to obtain a three-dimensional image of seismic velocity anomalies for this area by the method of Aki, Christoffersson & Husebye We found that the California network is less suitable than the LASA and NORSAR arrays for this kind of studies because of its greater proportion of peripheral blocks in which the resolution is very poor for the stochastic inverse solution and the random error effect is severe for the generalized inverse solution. Nevertheless, the resultant velocity anomalies show a remarkable correlation with the San Andreas fault zone to a depth of 75 km. The anomaly pattern changes drastically as the depth exceeds 75 km, suggesting that the asthenosphere has been reached.  相似文献   

Aperture synthesis observations of individual molecular clouds in M33     

Christine D. Wilson  Nick Scoville 《Astrophysics and Space Science》1989,156(1-2):269-273

Aperture synthesis maps of six fields in the nearby spiral galaxy M33 have revealed the presence of a population of molecular clouds whose masses, sizes, velocity widths, and brightness temperatures are similar to Galactic giant molecular clouds. The masses of the clouds obtained from the virial theorem and from the integrated CO flux are in relatively good agreement, suggesting that the conversion factor from CO flux to molecular mass in M33 is unlikely to be much different from the value measured in our own Galaxy. The star formation properties of these regions are under study with deep optical CCD imaging and near-infrared data.  相似文献   

Environmental aspects of child growth and nutrition: A case study from Ibadan,Nigeria     

Christine E. Rossington Dr. 《GeoJournal》1981,5(4):347-356

Protein-energy malnutrition, especially among young children, is a major health problem in many developing areas. Its causes are complex and inadequately understood. The paper outlines a pilot survey designed to investigate the impact of economic, demographic and socio-cultural factors on growth and nutrition among a small group of children aged between one and five years from urban poor families living in Ibadan, Nigeria. Field surveys were undertaken between July 1971 and August 1972 using 51 children from the Oje area of the city who formed part of a larger longitudinal study of child growth and development. Records of child growth patterns were compiled from monthly anthropometric measurements and enquiries made into the socio-economic and demographic status of the sample families.Basic analysis identified periods of growth retardation and seasonal fluctuations in somatic attainments. Multiple correlation analyses attempted to define statistically some of the aspects of the environment which significantly influenced somatic achievements. Relatively low levels of explanation were obtained, emphasising data deficiencies and the complexity of the nutrition problem, but small groups of economic and demographic causative variables were isolated.The research for this paper was funded by the Social Science Research Council, when the author was a postgraduate student, Department of Geography, University of Liverpool.  相似文献   

Continental growth and volatile exchange during Earth''s evolution     

Siegfried Franck  Christine Bounama 《Physics of the Earth and Planetary Interiors》1997,100(1-4):189-196

We investigate the thermal and degassing history of the Earth with the help of a parameterized mantle convection model including the volatile exchange between mantle and surface reservoirs. The weakening of mantle silicates by dissolved volatiles is described by a functional relationship between creep rate and water fugacity. We use flow law parameters of diffusion creep in olivine under dry and wet conditions. The mantle degassing rate is considered as directly proportional to the seafloor spreading rate, which is also dependent on the mantle heat flow and the continental area. To calculate the spreading rate, we assume three different continental growth models: constant growth, delayed growth, and the one proposed by Reymer and Schubert (1984, Tectonics, 3: 63–77). The rate of regassing also depends on the seafloor spreading rate, as well as on other factors. Both mechanisms (degassing and regassing) are coupled self-consistently with the help of a parameterized convection model under implementation of a temperature and volatile-content dependent mantle viscosity. We calculate time series for the Earth's evolution over 4.6 Gyr for the average mantle temperature, the mantle heat flow, the mantle viscosity, the Rayleigh number, the Urey ratio, the volatile loss, and the seafloor spreading rate. In those numerical simulations with continental growth from the beginning and a high initial average mantle temperature water is outgassed rapidly. In the delayed continental growth model there is a very early outgassing event and the delayed continental growth has no remarkable influence on the thermal and outgassing history. A similar situation is found for the linear continental growth model but not for the Reymer and Schubert (1984) model.  相似文献