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排序方式: 共有103条查询结果,搜索用时 31 毫秒
71.
Nadia Vogel Heinrich Baur Addi Bischoff Ingo Leya Rainer Wieler 《Meteoritics & planetary science》2004,39(5):767-778
Abstract— Calcium‐aluminum‐rich inclusions (CAIs) were among the first solids in the solar system and were, similar to chondrules, created at very high temperatures. While in chondrules, trapped noble gases have recently been detected, the presence of trapped gases in CAIs is unclear but could have important implications for CAI formation and for early solar system evolution in general. To reassess this question, He, Ne, and Ar isotopes were measured in small, carefully separated and, thus, uncontaminated samples of CAIs from the CV3 chondrites Allende, Axtell, and Efremovka. The 20Ne/22Ne ratios of all CAIs studied here are <0.9, indicating the absence of trapped Ne as, e.g., Ne‐HL, Ne‐Q, or solar wind Ne. The 21Ne/22Ne ratios range from 0.86 to 0.72, with fine‐grained, more altered CAIs usually showing lower values than coarse‐grained, less altered CAIs. This is attributed to variable amounts of cosmogenic Ne produced from Na‐rich alteration phases rather than to the presence of Ne‐G or Ne‐R (essentially pure 22Ne) in the samples. Our interpretation is supported by model calculations of the isotopic composition of cosmogenic Ne in minerals common in CAIs. The 36Ar/38Ar ratios are between 0.7 and 4.8, with fine‐grained CAIs within one meteorite showing higher ratios than the coarse‐grained ones. This agrees with higher concentrations of cosmogenic 36Ar produced by neutron capture on 35Cl with subsequent β?‐decay in finer‐grained, more altered, and thus, more Cl‐rich CAIs than in coarser‐grained, less altered ones. Although our data do not strictly contradict the presence of small amounts of Ne‐G, Ne‐R, or trapped Ar in the CAIs, our noble gas signatures are most simply explained by cosmogenic production, mainly from Na‐, Ca‐, and Cl‐rich minerals. 相似文献
72.
Nadia?ImtiazEmail author Johnathan?Burchill Richard?Marchand 《Astrophysics and Space Science》2015,355(1):23-32
We model the particle velocity distribution functions around the entrance window of the Suprathermal Ion Imager (SII). The SII sensor was mounted on a 1 m boom carried by the scientific payload of NASA rocket 36.234 as part of Joule II mission to investigate Joule heating in the E-region ionosphere. The rocket flew above Northern Alaska on 19 January 2007. The payload was spin-stabilized with a period of 1.6 s, giving an apparent rotation of the ion flow velocity in the frame of reference of the payload. The SII sensor is an electrostatic analyzer that measures two dimensional slices of the distribution of the kinetic energies and arrival-angles of low energy ions. The study is concerned with the interpretation of data obtained from the SII sensor. For this purpose, we numerically investigate ram velocity effects on ions velocity distributions in the vicinity of the SII sensor aperture at an altitudes of approximately 150 km. The electrostatic sheath profiles surrounding the SII sensor, boom and payload are calculated numerically with the PIC code PTetra. It is observed that the direction of the ion flow velocity modifies the plasma sheath potential profile. This in turn impacts the velocity distributions of NO+ and \(\mathrm{O}_{2}^{+}\) ions at the aperture of the particle sensor. The velocity distribution functions at the sensor aperture are calculated by using test-particle modeling. These particle distribution functions are then used to inject particles in the sensor, and calculate the fluxes on the sensor microchannel plate (MCP), from which comparisons with the measurements can be made. 相似文献
73.
Multiscale modeling of coastal, shelf, and global ocean dynamics 总被引:1,自引:1,他引:0
Pierre F. J. Lermusiaux Jens Schröter Sergey Danilov Mohamed Iskandarani Nadia Pinardi Joannes J. Westerink 《Ocean Dynamics》2013,63(11-12):1341-1344
74.
Recent developments in the application of x-ray micro-tomography in laboratory geomechanics have allowed all the individual
grains of sand in a test sample to be seen and identified uniquely in 3D. Combining such imaging capabilities with experiments
carried out “in situ” within an imaging set-up has led to the possibility of directly observing the mechanisms of deformation
as they happen. The challenge has thus become extracting pertinent, quantified information from these rich time-lapse 3D images
to elucidate the mechanics at play. This paper presents a new approach (ID-Track) for the quantification of individual grain
kinematics (displacements and rotations) of large quantities of sand grains (tens of thousands) in a test sample undergoing
loading. With ID-Track, grains are tracked between images based on some geometrical feature(s) that allow their unique identification
and matching between images. This differs from Digital Image Correlation (DIC), which makes measurements by recognising patterns
between images. Since ID-Track does not use the image of a grain for tracking, it is significantly faster than DIC. The technique
is detailed in the paper, and is shown to be fast and simple, giving good measurements of displacements, but suffering in
the measurement of rotations when compared with Discrete DIC. Subsequently, results are presented from successful applications
of ID-track to triaxial tests on two quite different sands: the angular Hostun sand and the rounded Caicos Ooids. This reveals
details on the performance of the technique for different grain shapes and insight into the differences in the grain-scale
mechanisms occurring in these two sands as they exhibit strain localisation under triaxial loading. 相似文献
75.
Nadia Solovieva Vivienne J. Jones Larisa Nazarova Stephen J. Brooks H. J. B. Birks John-Arvid Grytnes Peter G. Appleby Tommi Kauppila Boris Kondratenok Ingemar Renberg Vasily Ponomarev 《Journal of Paleolimnology》2005,33(4):463-482
The recent sediments from two deep arctic lakes, Mitrofanovskoe and Vanuk-ty, situated in the permafrost belt within the Bolshezemelskaya Tundra in the northern Ural region, were studied for diatoms, chironomids, spheroidal carbonaceous particles and stable lead isotopes. The magnitudes and rates-of-change in diatom and chironomid assemblages were numerically estimated. Instrumental climate records were used to assess statistically the amount of variance in diatom and chironomid data explained by temperature. August and September air temperatures have a statistically significant effect on diatom composition at both lakes. At Mitrofanovskoe Lake, major compositional changes in diatom and chironomid assemblages occurred at the turn of the 20th century and might be related to the regional increase in temperature. Chironomid-inferred air temperature also increased by approximately 1 °C since the early 1900s. At both lakes diatom compositional changes, coincident with the increase in June and September temperatures, also occurred in the late 1960s. These compositional changes are correlated with the increase in diatom production, sediment organic content and diatom species richness, and are likely to be a diatom response to the lengthening of the growing season. These changes are also correlated with the circum-Arctic temperature increase from the 1960s. A chironomid response to the late 1960s temperature increase was less pronounced at both lakes. Pollution levels are relatively low and pollution history is unrelated to ecological changes. Both lead isotopes and spheroidal carbonaceous particles show a clear atmospheric pollution signal, peaking in the 1980s. 相似文献
76.
Kaarina Sarmaja-Korjonen Seija Kultti Nadia Solovieva Minna Väliranta 《Journal of Paleolimnology》2003,30(4):415-426
Mid-Holocene changes in vegetation, palaeohydrology and climate were investigated from the sediments of Lake Vankavad in the northern taiga of the Usa Basin, NE European Russia, through the analysis of pollen, plant macrofossils, Cladocera and diatoms. Lake Vankavad was probably formed at ca. 5000 BP (ca. 5600 cal. BP) and initially it was shallow with a littoral cladoceran fauna. Macrofossil and pollen results suggest that dense Betula-Picea forests grew in the vicinity and the shore was close to the sampling point. At ca. 4600 BP (ca. 5400 cal. BP) the water level rose coincident with the decrease in the density and area of forests, probably caused by cooling climate and accelerated spread of mires. There was also a further rise in the water level at ca. 3500 BP (ca. 3800 cal. BP). The initiation of the lake, followed by two periods of rising water-level, as well as the increase in mire formation, was a consequence of a rise in groundwater level. This probably reflects lower evapotranspiration in a cooling mid-Holocene climate and/or higher precipitation in the lowland area. Also the decreased forest density and area may have contributed to the lower evapotranspiration. It is also possible that permafrost aggradation or changes in peat ecosystems might have affected the hydrological conditions in the area. 相似文献
77.
We compare insolation results calculated from two well-known empirical formulas (Seckel and Beaudry’s SB73 formula and the
original Smithsonian (SMS) formula) and a radiative transfer model using input data predicted from meteorological weather-forecast
models, and review the accuracy of each method. Comparison of annual mean daily irradiance values for clear-sky conditions
between the two formulas shows that, relative to the SMS, the SB73 underestimates spring values by 9 W m-2 in the northern Adriatic Sea, although overall there is a good agreement between the annual results calculated with the two
formulas. We also elucidate the effect on SMS of changing the ‘Sun-Earth distance factor (f)’, a parameter which is commonly
assumed to be constant in the oceanographic context. Results show that the mean daily solar radiation for clear-sky conditions
in the northern Adriatic Sea can be reduced as much as 12 W m-2 during summer due to a decrease in thef value. Lastly, surface irradiance values calculated from a simple radiative transfer model (GM02) for clear-sky conditions
are compared to those from SB73 and SMS. Comparison within situ data in the northern Adriatic Sea shows that the GM02 estimate gives more realistic surface irradiance values than SMS, particularly
during summer. Additionally, irradiance values calculated by GM02 using the buoy meteorological fields and ECMWF (The European
Centre for Medium Range Weather Forecasts) meteorological data show the suitability of the ECMWF data usage. Through tests
of GM02 sensitivity to key regional meteorological factors, we explore the main factors contributing significantly to a reduction
in summertime solar irradiance in the Adriatic Sea. 相似文献
78.
79.
80.
The present study employed a modified Fenton system that aims to extend the optimum pH range towards neutral conditions for studying the oxidation of benzene, toluene, ethyl benzene, xylenes (BTEX) using glutamic acid (Glu) as an iron chelator. Addition of 20 mM Glu greatly enhanced the oxidation rate of BTEX in modified Fenton system at pH 5–7. A rapid mass destruction (>97% after 1 h) of BTEX as a water contaminant carried out in the presence of 500 mM H2O2, 10 mM Fe2+, and 20 mM Glu at pH 5 could be shown. The efficiency of this modified Fenton's system for mass destruction of BTEX in contaminated water was measured to estimate the impact of the major process variables that include initial concentrations of soluble Fe, H2O2, Glu (as metal chelating agent), and reaction time. 相似文献