A new amber deposit from the Cretaceous (uppermost Albian-lowermost Cenomanian) of southwestern France   总被引：1，自引：0，他引：1  

Didier Nraudeau  Vincent Perrichot  Jean-Paul Colin  Vincent Girard  Bernard Gomez  Franois Guillocheau  Edwige Masure  Daniel Peyrot  Florent Tostain  Blaise Videt  Romain Vullo 《Cretaceous Research》2008,29(5-6):925

A Cretaceous amber deposit has recently been discovered in a quarry of Charente-Maritime (southwestern France), at Cadeuil. This paper presents the sedimentary and palaeoenvironmental settings of the uppermost Albian-lowermost Cenomanian series including the amber deposit. A preliminary analysis of the amber samples reveals diverse fossil arthropods (a few mites and at least 20 insect families within 9 orders), as well as numerous micro-organisms, mainly algae and mycelia. A myceloid colony of bacteria, a flagellate algae and four especially well preserved insects are illustrated (Diptera Dolichopodidae, Diptera Chironomidae, Hymenoptera Parasitica, and Heteroptera Tingidae). The abundance of the limnic micro-organisms is discussed in terms of bloom events. Their relative scarcity in almost all the amber pieces containing fossil arthropods is attributed to differences in the origin of resin: production along trunk and branches for amber with arthropods; production by aquatic roots for amber rich in algae. The absence of pollen and spores in amber is attributed to differences in the respective periods of resin and palynomorph production, which may be related to a seasonal climate during the Albian-Cenomanian transition in Western Europe.  相似文献   

阿尔金索尔库里地区元古代流纹岩锆石SHRIMP U-Pb定年及其地质意义   总被引：2，自引：1，他引：1  

张志诚  郭召杰  冯志硕  李建锋 《岩石学报》2010,26(2):597-606

阿尔金索尔库里北山彩虹沟塔什达坂群卓阿布拉克组流纹岩锆石SHRIMP U-Pb 年龄为920±20Ma (MSWD=1.50),代表流纹岩的喷出时间。岩石的SiO₂介于68.33%~70.60%,K₂O>Na₂O,K₂O/Na₂O平均值6.42,属弱过铝质(ACNK平均为1.25)钙碱性系列(σ平均为2.76),为一套典型的壳源流纹岩岩石系列。稀土元素含量高(平均为211.3×10^-6),轻稀土富集(L/H平均为6.57),Eu亏损中等(δEu平均为0.30)。微量元素以富集Rb、Th、K、Zr,而相对亏损Ba、Sr、Eu、Ti、Nb、Ta为特征。岩石微量及稀土元素具有典型的板内火山岩特征,而岩石显著的低Sr特征(25.0×10^-6~65.3×10^-6,平均值为36.8×10^-6))表明其并非源自加厚的地壳,而是起源于斜长石稳定的正常地壳。阿尔金流纹岩是由进入上地壳高位岩浆房的拉斑玄武岩浆的底侵作用直接使上地壳部分熔融,形成酸性火山岩的原始岩浆。该岩浆体系沿区域断裂构造体系上升,并经历了较强的结晶分异和演化,最终形成阿尔金索尔库里北山流纹岩系列。  相似文献   

Oxygen isotope study of Cayenne duricrust paleosurfaces: implications for past climate and laterization processes over French Guiana     

Jean-Pierre Girard 《Chemical Geology》2002,191(4):329-343

Oxygen isotopic compositions of weathering goethite, hematite, kaolinite and gibbsite in duricrust paleosurfaces of the Cayenne region, northeastern French Guiana, were investigated. Samples were microdrilled from different horizons and different pedogenetic microfacies of three well-characterized duricrust units of Eocene (unit 1) and Miocene (units 2 and 3) age. The results provided valuable information on duricrust formation processes and on climate change over French Guiana.The pristine original isotopic signal, suited for reconstruction of past climates, appears to be best preserved in the massive duricrust facies (middle part of the duricrust). In the overlying pisolotic duricrust and in the underlying mottled zone, the isotopic signal is affected by subsequent re-activation of weathering processes. Oxygen isotope data from massive duricrust indicate that Cayenne duricrusts formed from meteoric waters increasingly depleted in ¹⁸O with age. The youngest duricrust paleosurface (unit 3) formed under humid climate similar to present-day, while the two older paleosurfaces formed from meteoric paleo-water distinctly depleted in ¹⁸O, reflecting a “moonsonal” contrasted ancient climate for unit 2 added to the ¹⁸O-depleted nature of the pre-Miocene ocean for unit 1. The results further suggest that the major climatic change, from tropical wet-and-dry to present-day humid regime, recorded in Amazonia most likely occurred in the Late Miocene, and that Miocene laterization events may be responsible for the secondary bauxitization of the Eocene duricrust paleosurface.The oxygen isotopic composition of weathering minerals occurring in massive duricrust horizons, and in particular in hematite nodules and matrix, may be used as a tool to discriminate among the different duricrust paleosurfaces encountered in Amazonia and constrain the evolution of past climates.  相似文献   

Modeling of Nitrogen Cycle and Nitrate Transfer in Regional Hydrogeologic Systems   总被引：8，自引：0，他引：8  

Q. Z. Geng  G. Girard  E. Ledoux 《Ground water》1996,34(2):293-304

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Extension of the "Pore Tree" Model to Describe Transport in Soil     

Girard A. Simons 《Ground water》1996,34(4):683-690

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Spectroscopy of Mars from 2.04 to 2.44 micrometers during the 1993 opposition: absolute calibration and atmospheric vs mineralogic origin of narrow absorption features     

Bell JF rd  Pollack JB  Geballe TR  Cruikshank DP  Freedman R 《Icarus》1994,111(1):106-123

We present moderate-resolution (lambda/delta lambda = 300 to 370) reflectance spectra of Mars from 2.04 to 2.44 micrometers that were obtained at UKIRT during the 1993 opposition. Seven narrow absorption features were detected and found to have a Mars origin. By comparison with solar and Mars atmospheric spectra, five of these features were attributed all or in part to Mars atmospheric CO2 or CO(2.052 +/- 0.003, 2.114 +/- 0.002, 2.150 +/- 0.003, 2.331 +/- 0.001, and 2.357 +/- 0.002 micrometers). Two of the bands (2.331 +/- 0.001 and 2.357 +/- 0.002 micrometers) appear to have widths and depths that are consistent with additional, nonatmospheric absorptions, although a solar contribution cannot be entirely ruled out. Two other weak bands centered at 2.278 +/- 0.002 and 2.296 +/- 0.002 micrometers may be at least partially mineralogic in origin. The data provide no conclusive identification of the mineralogy responsible for these absorption features. However, examination of terrestrial spectral libraries and previous moderate spectral resolution mineral studies indicates that the most likely origin of these features is either (bi)carbonate or (bi)sulfate anions in framework silicates or (Fe, Mg)-OH bonds in sheet silicates. If the bands are caused by phyllosilicate minerals, then an explanation must be found for the extremely narrow widths of the cation-OH features in the Mars spectra as compared to terrestrial minerals.  相似文献   

Evaluation of an ensemble of Arctic regional climate models: spatiotemporal fields during the SHEBA year     

A. Rinke  K. Dethloff  J. J. Cassano  J. H. Christensen  J. A. Curry  P. Du  E. Girard  J.-E. Haugen  D. Jacob  C. G. Jones  M. Køltzow  R. Laprise  A. H. Lynch  S. Pfeifer  M. C. Serreze  M. J. Shaw  M. Tjernström  K. Wyser  M. Žagar 《Climate Dynamics》2006,27(4):433-435

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Impact of the Quadrupole Moment of the Sun on the Dynamics of the Earth-Moon System     

E. Bois  J.F. Girard 《Celestial Mechanics and Dynamical Astronomy》1999,73(1-4):329-338

Range of values of the Sun's mass quadrupole moment of coefficient J₂ arising both from experimental and theoretical determinations enlarge across literature on two orders of magnitude, from around 10^-7 until to 10^-5. The accurate knowledge of the Moon's physical librations, for which the Lunar Laser Ranging data reach an outstanding precision level, prove to be appropriate to reduce the interval of J₂ values by giving an upper bound of J₂. A solar quadrupole moment as high as 1.1 10^-5 given either from the upper bounds of the error bars of the observations, or from the Roche's theory, is not compatible with the knowledge of the lunar librations accurately modeled and observed with the LLR experiment. The suitable values of J₂ have to be smaller than 3.0 10^-6. As a consequence, this upper bound of 3.0 10^-6 is accepted to study the impact of the Sun's quadrupole moment of mass on the dynamics of the Earth-Moon system. Such as effect (with J₂ = 5.5±1.3 × 10^-6) has been already tested in 1983 by Campbell & Moffat using analytical approximate equations, and thus for the orbits of Mercury, Venus, the Earth and Icarus. The approximate equations are no longer sufficient compared with present observational data and exact equations are required. As if to compute the effect on the lunar librations, we have used our BJV relativistic model of solar system integration including the spin-orbit coupled motion of the Moon. The model is solved by numerical integration. The BJV model stems from general relativity by using the DSX formalism for purposes of celestial mechanics when it is about to deal with a system of n extended, weakly self-gravitating, rotating and deformable bodies in mutual interactions. The resulting effects on the orbital elements of the Earth have been computed and plotted over 160 and 1600 years. The impact of the quadrupole moment of the Sun on the Earth's orbital motion is mainly characterized by variations of , , and . As a consequence, the Sun's quadrupole moment of mass could play a sensible role over long time periods of integration of solar system models. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Characterizing the vadose zone and a perched aquifer near the Vosges ridge at the La Soutte experimental site,Obernai, France     

Pascal Sailhac  Maksim Bano  Mickael Behaegel  Jean-François Girard  Ester Falgàs Para  Juanjo Ledo  Guy Marquis  Pierre-Daniel Matthey  José Ortega-Ramírez 《Comptes Rendus Geoscience》2009,341(10-11):818-830

We consider a series of hydrogeophysical techniques that provide a multiscale investigation of the water content in the vadose zone and of the perched aquifer at the experimental site of “La Soutte” in the Vosges Mountains (France). It is located in a catchment area where several springs and streams occur along fractured volcanic and weathered plutonic rocks. The site is the object of a long-term study that uses both continuous and repeated measurements to monitor hydrogeological processes. The main results from AMT and DC resistivity techniques allow the determination of a high-resolution 3D resistivity model over a large range of depths (from 10⁰ to 10³ m). We discuss their use and propose a hydrogeological model (porosity, water conductivity and water content). We also use MRS and GPR for a detailed investigation of the shallow part of the catchment that consists of soil and weathered rocks of highly varying thickness (0 to 15 m). MRS is used to map the thickness and total water volume content by unit surface of the saturated weathered zone. It also yields estimates of the vadose zone thickness through the depth to the top of the saturated zone. Moreover, we show results from GPR CMP measurements that yield estimates of the water content and porosity in the shallowest layer (0–30 cm) by simple interpretation of the ground direct wave.  相似文献   

Numerical study of the variations of magnetic resonance signals caused by surface slope   总被引：1，自引：0，他引：1  

J.-F. Girard  A. Legchenko  M. Boucher  J.-M. Baltassat 《Journal of Applied Geophysics》2008,66(3-4):94

When performing forward modelling and inversion of Magnetic Resonance Sounding (MRS) data, the water-content distribution is typically assumed to be horizontal (1D case). This assumption is fully justified because MRS is often used for characterizing continuous aquifers in a nearly flat environment. However, MRS can also be used in areas with sharp topographical variations. Following a review of the standard MRS equations when using a coincident transmitter/receiver loop, the mathematical terms potentially affected by tilting of the loop are discussed. We present the results of a numerical modelling exercise, studying a case where the surface is not horizontal and the loop cannot be considered to be parallel to the top of the aquifer. This shows that maximum variations in the MRS-signal amplitude are caused mainly by north- or south-dipping slopes. Slope effects depend on the loop size (a larger loop produces a larger error) especially in the presence of shallow water. With a geomagnetic-field inclination of 65° and a slope angle ≤ 10°, the topography causes a maximum variation in amplitude of less than 10%. Near magnetic poles and equator, the slope effect is lower and undetectable in most cases. It was found that within a 10% range of variation in the amplitude, errors introduced into inversions are within the typical uncertainty for MRS inversion and hence no topographic corrections are necessary. Thus, a significant effect from non-horizontal topography might be expected only when data uncertainty is lower than the slope effect (the slope effect is lower than equivalence when data quality is poor). Today, most field data sets are inverted using the modulus of the MRS signal, but some new developments consider the complex signal (both modulus and phase). However, inversion of complex MRS signals, which would provide a higher sensitivity to groundwater distribution, may be affected by slope effect. Thus, the slope orientation and dip angle should be accurately measured in the field when the phase of MRS signals is inverted too.  相似文献