粘土矿物在气候环境变化研究中的应用进展   总被引：1，自引：0，他引：1  

孙庆峰  陈发虎  张家武 《矿物学报》2011,31(1):146-152

在古环境和古气候的重建中,粘土矿物和碳-氧同位素、孢粉、树轮、冰芯等代用指标一样具有同等重要的地位。在没有地质构造运动影响时,气候是影响粘土矿物形成的主要因素,沉积物中的粘土矿物可用来分析古气候和古环境。粘土矿物及其组合可以独立或作为主要指标反映气候和环境变化,并已应用于高分辨率的晚第四纪地层的气候环境研究中。粘土矿物在很短的时间内也会发生明显地变化,不仅可以反映千年-百年尺度的气候环境变化,而且也可以反映几十年尺度的古气候环境变化过程。粘土矿物与其它指标对同一气候环境响应的相位差有待深入研究。不同的半定量分析方法测量出的同一剖面中粘土矿物的含量变化趋势和特征具有一致性。  相似文献   

2000 ans de colmatage du port antique de Fréjus (Forum Julii), France : une double métamorphose littorale     

Guénaëlle Bony  Christophe Morhange  Hélène Bruneton  Pierre Carbonel  Chérine Gébara 《Comptes Rendus Geoscience》2011,343(10):701-715

The ancient harbour of Fréjus, located in a Holocene ria, has been the subject of a research program in archaeology and, notably with regards to the sedimentary environment at its foundation. A core was extracted in the middle of the basin of Fréjus harbour. The objective is to understand the paleogeographical evolution of the pre-harbour and Roman harbour environments. The sedimentological and biostratigraphical proxies enabled us to: (1) confirm Texier's (1849) hypothesis in which the pre-harbour environment comprised a marine bay blocked by an artificial quay (Gébara and Morhange, 2010). Excoffon et al., 2006 and Devillers et al., 2007, demonstrate the presence of a rocky coast (butte Saint-Antoine), at the time of the harbour's foundation, which it has been progressively transformed into a sandy coast due to the sedimentary input of Argens delta. This study permitted: (2) to confirm the date of foundation of Fréjus’ harbor; and (3) to show different phases of protection. Indeed, the harbour facies attests to a euryhaline lagoon (B1 and B3) which was gradually transformed into a freshwater lake (B4) due to the progradation of the Argens. Low sedimentation rates (ca. 0.5 mm/year), between the end of the last century BC until seventh century AD is consistent with the dredging of the harbour basin.  相似文献   

Morphotectonic and fault�Cearthquake relationships along the northern Ligurian margin (western Mediterranean) based on high resolution, multibeam bathymetry and multichannel seismic-reflection profiles     

Christophe Larroque  Bernard Mercier de L��pinay  S��bastien Migeon 《Marine Geophysical Researches》2011,32(1-2):163-179

We present here new data from the MALISAR surveys that focus on two areas of the northern Ligurian margin where we reveal recent and active deformation. A set of N60°E scarps that are oblique to the margin is seen at the foot of the continental slope. These correspond to cumulated reverse-strike slip faulting that is consistent with the present-day kinematics of earthquakes. At the north-western margin, the Marcel Fault appears at the surface as a 10-km-long scarp trending N60°E. Several earthquakes of moderate magnitude (3.8 < M_L < 4.6) have focal mechanisms consistent with the geometry and the kinematics of, and have been located around, the Marcel Fault. At the north-eastern margin, offshore of Imperia, the major feature is a large promontory that is bound by a network of N60°E faults on its southern side. The structures and the deflection of the drainage network are consistent with a recent uplift of the Imperia Promontory. No surface ruptures have been identified in the epicentre area of the 1887 Ligurian earthquake (the major historical regional event: M_W ~6.5?C6.7), although the Imperia Fault network has the necessary characteristics to account for this earthquake. Therefore, from the present study, we propose that the rupture, as a reverse-strike slip faulting of a few or all of the segments belonging to the Imperia Fault network, was the source of the 1887 event. These MALISAR data have allowed identification of an 80-km-long transpressive system of Plio-Quaternary faults. The question of the potential activation of all of these faults during a single event is now of major concern, which has led to reappraisal of the regional seismic hazard as moderate to high.  相似文献   

Use of inhibitors for coastal bacteria and phytoplankton: Application to nitrogen uptake measurement     

Aurore Trottet  Eric Fouilland  Christophe Leboulanger  Elodie Lanouguère  Marc Bouvy 《Estuarine, Coastal and Shelf Science》2011

For several decades, prokaryotic and eukaryotic inhibitors have been used to exclude bacteria from microalgal cultures and for investigating prey-predator relationships. Recently there has been considerable interest in using specific inhibitors for studying the interactions between bacteria and phytoplankton, by selective repression of either organism’s activity. The effectiveness of chemical inhibitors must be tested before applying them to natural communities to partition metabolic activities between functional groups. Six different antibiotics selected from the most commonly reported in the literature were tested, at concentrations varying from 12.5 to 100 mg L⁻¹, for their effect on bacterial growth and functional diversity of natural communities from Mediterranean coastal waters. Penicillin and streptomycin each at a final concentration of 100 mg L⁻¹ significantly reduced bacterial growth within 2 h. There was a greater impact on bacterial functional diversity when both antibiotics were mixed together. This mixture did not have any significant effect on the growth of selected cultured phytoplankton strains, whereas the eukaryote inhibitor cycloheximide at 100 mg L⁻¹ reduced growth within 2 h of incubation. The penicillin–streptomycin mixture and cycloheximide alone successfully partitioned NH₄⁺ and NO₃⁻ uptake between bacteria and phytoplankton bi-weekly sampled in a coastal lagoon in Autumn, where bacterial contribution to total NH₄⁺ and NO₃⁻ uptake averaged 46 and 41%, respectively. The use of specific inhibitors may be a valuable method for studying interactions, such as competition and mutualism, or lack of interaction between the different components of microbial communities and could be used to study their relative importance in biogeochemical fluxes.  相似文献   

Dissipation of Titan's north polar cloud at northern spring equinox     

Stéphane Le Mouélic  Pascal Rannou  Sébastien Rodriguez  Christophe Sotin  Caitlin A. Griffith  Lucille Le Corre  Jason W. Barnes  Robert H. Brown  Kevin H. Baines  Bonnie J. Buratti  Roger N. Clark  Philip D. Nicholson  Gabriel Tobie 《Planetary and Space Science》2012,60(1):86-92

Saturn's Moon Titan has a thick atmosphere with a meteorological cycle. We report on the evolution of the giant cloud system covering its north pole using observations acquired by the Visual and Infrared Mapping Spectrometer onboard the Cassini spacecraft. A radiative transfer model in spherical geometry shows that the clouds are found at an altitude between 30 and 65 km. We also show that the polar cloud system vanished progressively as Titan approached equinox in August 2009, revealing at optical wavelengths the underlying sea known as Kraken Mare. This decrease of activity suggests that the north-polar downwelling has begun to shut off. Such a scenario is compared with the Titan global circulation model of Rannou et al. (2006), which predicts a decrease of cloud coverage in northern latitudes at the same period of time.  相似文献   

Analytic theory of Titan’s Schumann resonance: Constraints on ionospheric conductivity and buried water ocean     

Christian Béghin  Orélien Randriamboarison  Michel Hamelin  Erich Karkoschka  Christophe Sotin  Robert C. Whitten  Jean-Jacques Berthelier  Réjean Grard  Fernando Simões 《Icarus》2012,218(2):1028-1042

This study presents an approximate model for the atypical Schumann resonance in Titan’s atmosphere that accounts for the observations of electromagnetic waves and the measurements of atmospheric conductivity performed with the Huygens Atmospheric Structure and Permittivity, Wave and Altimetry (HASI–PWA) instrumentation during the descent of the Huygens Probe through Titan’s atmosphere in January 2005. After many years of thorough analyses of the collected data, several arguments enable us to claim that the Extremely Low Frequency (ELF) wave observed at around 36 Hz displays all the characteristics of the second harmonic of a Schumann resonance. On Earth, this phenomenon is well known to be triggered by lightning activity. Given the lack of evidence of any thunderstorm activity on Titan, we proposed in early works a model based on an alternative powering mechanism involving the electric current sheets induced in Titan’s ionosphere by the Saturn’s magnetospheric plasma flow. The present study is a further step in improving the initial model and corroborating our preliminary assessments. We first develop an analytic theory of the guided modes that appear to be the most suitable for sustaining Schumann resonances in Titan’s atmosphere. We then introduce the characteristics of the Huygens electric field measurements in the equations, in order to constrain the physical parameters of the resonating cavity. The latter is assumed to be made of different structures distributed between an upper boundary, presumably made of a succession of thin ionized layers of stratospheric aerosols spread up to 150 km and a lower quasi-perfect conductive surface hidden beneath the non-conductive ground. The inner reflecting boundary is proposed to be a buried water–ammonia ocean lying at a likely depth of 55–80 km below a dielectric icy crust. Such estimate is found to comply with models suggesting that the internal heat could be transferred upwards by thermal conduction of the crust, while convective processes cannot be ruled out.  相似文献   

Quantitative evaluation of soil processes using in situ-produced cosmogenic nuclides     

Erik Thorson Brown  Fabrice Colin  Didier L. Bourls 《Comptes Rendus Geoscience》2003,335(16):1161-1171

In situ-produced cosmogenic nuclides provide a means for quantitative evaluation of a wide range of weathering and sediment transport processes. Although these nuclides have received attention for their power as geochronometers of surface exposure, it may be argued that they are more broadly suited for study of surface processes. In many environments, they may be used to evaluate collapse, erosion, burial, bioturbation, and creep, as well as providing a qualitative basis for distinguishing allochthonous from autochthonous materials. In addition, these nuclides can provide quantitative information on rates of erosion on scales of landforms and drainage basins. Here, we review the systematics of cosmogenic nuclide production within the Earth's surface, and present field examples demonstrating the utilization of in situ-produced cosmogenic nuclides distributions for evaluation of a range of soil evolution processes. To cite this article: E.T. Brown et al., C. R. Geoscience 335 (2003).  相似文献   

Biogéographie des ammonites jurassiques et reconstitution palinspastique de la Téthys     

Jean-Louis Dommergues  Didier Marchand  Jacques Thierry 《Geodinamica Acta》2013,26(4-5):273-281

Résumé

— La distribution géographique des ammonites jurassiques est régie par deux causes fondamentales : l’écologie et l’histoire évolutive (événements vicariants). L’analyse conjointe de ces deux facteurs permet de reconnaître : d’une part des taxons dont la distribution est essentiellement contrôlée par des contraintes écologiques (Phylloce-ratinae et Lytoceratinae, liés à des environnements océaniques profonds; Clydoniceratidae et Proplanulitinae liés à des plates-formes assez superficielles); d’autre part des taxons dont l’histoire évolutive est associée à des événements vicariants (Ammonitina liasiques euro-boréales et Cardioceratidae-Kosmoceratidae boréaux du Jurassique moyen).

Les exemples développés ici permettent d’analyser en terme de paléobiogéographie la position de l’Europe centro-méridionale (Bulgarie, Hongrie, Roumanie) incluse au Jurassique dans la bordure nord-téthy-sienne. Il est montré que Phylloceratinae et Lytoceratinae sont très abondants dans les régions supposées profondes à cette époque (sphéno-chasme des monts d’Apuseni, sillon Dobrogeo-Caucasien), alors qu’elles sont très rares sur la plate-forme moësienne. La même remarque est valable pour les plates-formes moyennes-orientales de la marge sud (Israël, Arabie Saoudite).

Lorsque l’on tente d’établir des reconstructions palinspastiques basées sur la paléobiogéographie, on constate que les taxons qui ont une histoire évolutive originale fournissent de meilleures informations paléogéographiques que les formes ubiquistes ou celles à préférences écologiques accusées. Les données brutes de répartition des faunes d’ammonites ne sont donc pas des arguments absolus pour corroborer les reconstructions. Les analyses fauniques, conduites avec une approche qualitative et quantitative, doivent tenir compte de données extra-biologiques telles que la distribution des faciès et des unités structurales; enfin, le niveau d’intervention — local, régional, global — conditionne fortement les possibilités d’interprétation des résultats.  相似文献   

Evolution of mass-transfer during progressive oblique under-thrusting of the Variscan foreland: eastern Bohemian Massif     

Andrea Kolaříková  Didier Marquer  Karel Schulmann 《Geodinamica Acta》2013,26(3):81-93

Abstract

Four ductile shear zones were sampled in the autochthonous Thaya basement and the Upper Bíte? nappe (Moravian unit) at the Eastern margin of the Bohemian massif. In both studied units, the tectono-metamorphic evolution and the chemical mass transfer are different. Two deformational events are recognised: the first deformation stage under amphibolite facies conditions is overprinted by a second event under greenschist facies conditions.

The first deformation affected the western margin of the Thaya basement and the whole Bíte? nappe: microstructures are characterised by dynamic recrystallisation of feldspars and quartz, and occurrence of myrmekites and grain-boundary migration of quartz. None or weak chemical mass transfer is related to this medium to high temperature deformation. This deformation corresponds to the thrusting of Moldanubdian units on the Brunovistulian units (Moravian nappes and autochthonous Thaya basement).

The second deformation generated shear zones in the until then preserved Thaya basement and reactivated both shear zones of the western margin of the Thaya basement and those of the Bíte? nappe. This deformation is retrograde and mainly associated with chemical mass transfer: a decrease of CaO, FeO, FeO/Fe₂O₃ and an increase of MgO, K₂O and H₂O. These chemical changes are related to greenschist metamorphic reactions leading to the destabilisation of feldspars and the crystallisation of white micas and Ca-silicates. The large chemical mass transfer is associated with the circulation of a large volume of fluids. A model of progressive fluid circulation correlated with Variscan prograde and retrograde metamorphism during the collision of Moldanubian and Brunovistulian units is proposed.  相似文献   

Impact of environmental parameters on coral reef development and drowning: Forward modelling of the last deglacial reefs from Tahiti (French Polynesia; IODP Expedition #310)     

Claire Seard  Jean Borgomano  Didier Granjeon  Gilbert Camoin 《Sedimentology》2013,60(6):1357-1388

The sedimentological and chronological analysis of the last deglacial reef sequences of Tahiti (French Polynesia), drilled during the Integrated Ocean Drilling Program Expedition 310, provide a high‐resolution data set allowing a well‐constrained forward modelling study. This study represents the first attempt to model in three dimensions the coral reef development of Tahiti during the last deglacial sea‐level rise (23 000 to 6000 cal yr bp ) using the software dionisos developed by IFP Energies nouvelles. It allows the testing of the reconstructed last deglacial sea‐level curve and the different environmental parameters (for example, wave energy and sediment fluxes) that could have influenced the reef development. These last deglacial reef sequences form two prominent ridges occurring seaward of the living barrier reef that consist of successive submerged reefs. These reefs have been prone to drowning because the window of maximum carbonate production rate is inhibited by high water turbidity (sediment supply from a nearby river), shallow depth of wave action and substrate availability. These factors, combined with rapid sea‐level rise, have driven the growth of retrograding reef pinnacles. Local factors (substratum nature, sediment supply and wave energy) were the main processes that induced the drowning of the inner ridge, whereas interplay of local and global factors (acceleration of the sea‐level rise) was responsible for the drowning of the outer ridge. This particular acceleration of sea‐level rise of 16 m between 14·6 ka and 14 ka bp corresponds to meltwater pulse 1A.  相似文献