Gaussianity of cosmic velocity fields and linearity of the velocity–gravity relation     

Pawe&#; Cieciel&#;g  Micha&#; J. Chodorowski  Marcin Kiraga  Michael A. Strauss  rzej Kudlicki  François R. Bouchet 《Monthly notices of the Royal Astronomical Society》2003,339(3):641-651

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The restoration of hazardous waste sites in Alpine regions     

Franois Veuthey 《Engineering Geology》1993,34(3-4):145-150

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Relation of the fluctuations of some of the solar activity indices     

T. Ataç 《Astrophysics and Space Science》1989,159(1):173-176

In this Letter we obtained the fluctuation curves from the differences of unsmoothed and smoothed values of the different solar activity indices. We compared the pattern of fluctuations of these curves. Also using monthly mean values of each index we studied the degree of correlation between the pairs of indices during the selected time intervals.  相似文献   

78-Day periodicity in the solar 1–8 Å X-ray index during the ascending branch of cycle 21     

Atila Özgüç 《Astrophysics and Space Science》1989,162(1):123-127

In the present paper, the time series of 1–8 Å X-ray index for the time interval between January 1977 to September 1981 has been analyzed by carrying out power spectrum using Discrete Fourier Transform. The 78-day periodicity which is one-half of the period found from various solar parameters of cycles 20 and 21 by various authors, was found. This periodicity is thought to be related to the 152-day periodicity.  相似文献   

Accumulation of heavy metals by flounder, Platichthys flesus (Linnaeus 1758), in a heterogeneously contaminated nursery area     

Vinagre C  França S  Costa MJ  Cabral HN 《Marine pollution bulletin》2004,49(11-12):1109-1113

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Prediction of heavy metal solubility in agricultural topsoils around two smelters by the physico-chemical parameters of the soils   总被引：1，自引：0，他引：1  

Matthieu?Fran?oisEmail author  Henri-Charles?Dubourguier  Dongyan?Li  Francis?Douay 《Aquatic Sciences - Research Across Boundaries》2004,66(1):78-85

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Non-conservative behavior of bromide in surface waters and brines of Central Andes: A release into the atmosphere?     

François Risacher  Bertrand Fritz 《Geochimica et cosmochimica acta》2006,70(9):2143-2152

The transfer of reactive bromine into the atmosphere was recently observed by Hönninger et al. [Hönninger, G., Bobrowski, N., Palenque, E.R., Torrez, R., Platt, U., 2004. Reactive bromine and sulfur emission at salar de Uyuni, Bolivia. Geophys. Res. Lett.31, doi:10.1029/2003GL018818] in a large salt pan of the Bolivian Altiplano: the salar de Uyuni. However, bromide is considered to be an excellent conservative tracer, which leads to the questioning of its actual conservation in surficial geochemical processes. The relation between bromide and lithium, thought to be a conservative component in waters and brines of the Central Andes, points to a depletion of Br relative to Li in Uyuni brines of about 50-300 kg/day, a flux close to that measured by Hönninger et al. (2004): ?200 kg/day. Such values are very low in regard to the size of the salar (5-30 g/km²/day). Salt efflorescences have a much higher surface area than a flat salt crust, which should enhance the release of bromine. Leach solutions of salt efflorescences in closed basins of northern Chile are compared to their parent waters. Conservative components should have the same concentration ratios in both solutions. Actually, a strong depletion in Br is observed in the leach solutions, which could suggest a significant release of Br from the salt into the atmosphere. During the rainy season, efflorescences are leached and their dissolved components brought in saline lakes and salars. Evaporative profiles show a slight but noticeable fractionation between Li and Br which could be due to the contribution of Br-depleted leach solutions of salt efflorescences. Therefore, bromide does not behave conservatively in surface waters and brines of the Central Andes. If the loss of Br is really due to its transfer into the atmosphere, then the flux would be much higher than that estimated for the salar de Uyuni alone. Numerous salt pans, saline lakes, and widespread efflorescences covering large land surfaces would contribute significantly more reactive bromine into the atmosphere.  相似文献   

Li and B isotopic variations in an Allende CAI: Evidence for the in situ decay of short-lived Be and for the possible presence of the short-lived nuclide Be in the early solar system     

Marc Chaussidon  François Robert 《Geochimica et cosmochimica acta》2006,70(1):224-245

The concentrations and isotopic compositions of lithium, beryllium, and boron, analyzed in situ by ion microprobe in 66 spots of a type B1 Ca-Al-rich inclusion (CAI 3529-41) from the Allende meteorite, are reported. Large variations are observed for both the Li and the B isotopic ratios with ⁷Li/⁶Li ranging from 9.2 ± 0.22 to 12.22 ± 0.43 (a ≈250‰ range in δ⁷Li values) and ¹⁰B/¹¹B ranging from 0.2468 ± 0.0057 to 0.4189 ± 0.0493 (a 410‰ range in δ¹¹B values). The very low Li concentrations (<1 ppb) observed in several anorthite and fassaite grains require that a correction for the contribution of spallogenic Li produced during irradiation of the Allende meteoroid by galactic cosmic rays (GCR) be made (after this correction ⁷Li/⁶Li ranges from 9.2 ± 0.22 to 13.44 ± 0.56, i.e., a ≈350‰ range in δ⁷Li values). In 3529-41, the ¹⁰B/¹¹B ratios are positively correlated with ⁹Be/¹¹B in a manner indicating the in situ decay of short-lived ¹⁰Be (half-life = 1.5 Ma) with a ¹⁰Be/⁹Be ratio at the time of formation of the CAI of 8.8 ± 0.6 × 10⁻⁴, which is in agreement with previous findings [McKeegan, K.D., Chaussidon, M., Robert, F., 2000. Incorporation of short-lived ¹⁰Be in a calcium-aluminum-rich inclusion from the Allende meteorite. Science289, 1334-1337]. The present detailed investigation demonstrates that only minor perturbations of the ¹⁰Be-¹⁰B system are present in 3529-41, contrary to the ²⁶Al/²⁶Mg system for which numerous examples of isotopic redistribution following crystallization were observed [Podosek, F.A., Zinner, E.K., MacPherson, G.J., Lundberg, L.L., Brannon, J.C., Fahey, A.J., 1991. Correlated study of initial ⁸⁷Sr/⁸⁶Sr and Al-Mg systematics and petrologic properties in a suite of refractory inclusions from the Allende meteorite. Geochim. Cosmochim. Acta55, 1083-1110]. Petrographically based criteria were developed to identify within the 66 analyzed spots in 3529-41, those where post-magmatic perturbation of the Li and Be distributions occurred. Li and Be concentrations measured in different analytical spots are compared with those predicted by using experimentally determined partition coefficients according to a model of closed-system crystallization of the CAI melt. These criteria show that 56% of the spots in melilite, 38% in anorthite, and 8% in fassaite suffered post-crystallization perturbations of Li and/or Be distributions. In the remaining spots, which do not show obvious indication of redistribution of Li or Be, the ⁷Li/⁶Li isotopic variations (corrected for GCR exposure) are positively correlated with⁹Be/⁶Li suggesting the in situ decay of now-extinct ⁷Be. The derived isochron implies that at the time of its formation, the CAI melt had a ⁷Be/⁹Be ratio of 0.0061 ± 0.0013 and a ⁷Li/⁶Li ratio of 11.49 ± 0.13. In contrast, all the spots in 3529-41, which do show evidence for post-magmatic redistribution of Li and Be, have relatively constant ⁷Li/⁶Li, averaging 11.72 ± 0.56, which is consistent with mass balance calculations for Li isotopic homogenization in the CAI after the decay of ⁷Be. The incorporation of live ⁷Be in 3529-41 requires, because of the very short half-life of this nuclide (53 days), that it be produced essentially contemporaneously with the formation of the CAI. Therefore, the irradiation processes responsible for production of ⁷Be must have occurred within the solar accretion disk. Calculations developed in the framework of the x-wind model [Gounelle, M., Shu, F.H., Shang, H., Glassgold, A.E., Rehm, E.K., Lee, T., 2004. The origin of short-lived radionuclides and early Solar System irradiation (abstract). Lunar Planet. Sci.35, 1829] reproduce the ⁷Be and ¹⁰Be abundances observed in 3529-41. The correlated presence of ⁷Be and ¹⁰Be in 3529-41 is thus a strong argument that ¹⁰Be, which is observed rather ubiquitously in CAIs, is also a product of irradiation in the early solar system, as might be a significant fraction of other short-lived radionuclides observed in early solar system materials.  相似文献   

Expériences de drainage et estimation de paramètres en milieu poreux non saturé     

Hussein Beydoun  François Lehmann 《Comptes Rendus Geoscience》2006,338(3):180-187

Two drainage experiments were carried out to identify the hydraulic parameters of a quartz sand by using inverse modelling. Our results, based on sensitivity and error analyses, show that (i) water content measurements are essential to estimate the parameters of the van Genuchten–Mualem retention curve, (ii) the saturated conductivity ($K_{\mathrm{s}}$) has a low sensitivity to pressure data and is not sensitive to other measures (water content and measured outflow), (iii) the inverse approach can be verified by comparing the simulated outflow to the measured one. To cite this article: H. Beydoun, F. Lehmann, C. R. Geoscience 338 (2006).  相似文献   

Coupling statistical and dynamical methods for spatial downscaling of precipitation   总被引：1，自引：0，他引：1  

Jie Chen  Fran?ois P. Brissette  Robert Leconte 《Climatic change》2012,114(3-4):509-526

The resolution of General Circulation Models (GCMs) is too coarse for climate change impact studies at the catchment or site-specific scales. To overcome this problem, both dynamical and statistical downscaling methods have been developed. Each downscaling method has its advantages and drawbacks, which have been described in great detail in the literature. This paper evaluates the improvement in statistical downscaling (SD) predictive power when using predictors from a Regional Climate Model (RCM) over a GCM for downscaling site-specific precipitation. Our approach uses mixed downscaling, combining both dynamic and statistical methods. Precipitation, a critical element of hydrology studies that is also much more difficult to downscale than temperature, is the only variable evaluated in this study. The SD method selected here uses a stepwise linear regression approach for precipitation quantity and occurrence (similar to the well-known Statistical Downscaling Model (SDSM) and called SDSM-like herein). In addition, a discriminant analysis (DA) was tested to generate precipitation occurrence, and a weather typing approach was used to derive statistical relationships based on weather types, and not only on a seasonal basis as is usually done. The existing data record was separated into a calibration and validation periods. To compare the relative efficiency of the SD approaches, relationships were derived at the same sites using the same predictors at a 300km scale (the National Center for Environmental Prediction (NCEP) reanalysis) and at a 45km scale with data from the limited-area Canadian Regional Climate Model (CRCM) driven by NCEP data at its boundaries. Predictably, using CRCM variables as predictors rather than NCEP data resulted in a much-improved explained variance for precipitation, although it was always less than 50?% overall. For precipitation occurrence, the SDSM-like model slightly overestimated the frequencies of wet and dry periods, while these were well-replicated by the DA-based model. Both the SDSM-like and DA-based models reproduced the percentage of wet days, but the wet and dry statuses for each day were poorly downscaled by both approaches. Overall, precipitation occurrence downscaled by the DA-based model was much better than that predicted by the SDSM-like model. Despite the added complexity, the weather typing approach was not better at downscaling precipitation than approaches without classification. Overall, despite significant improvements in precipitation occurrence prediction by the DA scheme, and even going to finer scales predictors, the SD approach tested here still explained less than 50?% of the total precipitation variance. While going to even smaller scale predictors (10–15?km) might improve results even more, such smaller scales would basically transform the direct outputs of climate models into impact models, thus negating the need for statistical downscaling approaches.  相似文献