Essai sur la structure des domaines émergés autour de la Méditerranée occidentale     

Prof. Dr. Michel Durand Delga 《International Journal of Earth Sciences》1964,53(2):534-535

Résumé De travaux menés dans les zones littorales de l'Afrique du Nord et dans tout le S de l'Espagne, l'auteur tire une nouvelle définition des grands ensembles structuraux péri-méditerranéens. Ces ensembles sont, dans les Cordillères bétiques, du N au S: zones externes (Prébétique, Subbétiques, Pénibétiques), zones internes (Flyschs gaditans, Malaguides, Alpujarrides, Nevadides 1). Dans le Rif marocain, symétriquement, on rencontre du S au N: zones externes (Autochtone de l'Atlas, nappes prérifaines et intrarifaines), zones internes (Flyschs nord-rifains, Tétouanides 2), Ghomarides 3), Sebtides 4); la plupart de ces zones se poursuivent vers l'E, jusqu'en Tunisie et en Sicile.Le fait majeur, à souligner au départ, est la parfaite symétrie de la chaîne alpine de la Méditerranée occidentale: les nappes rifaines ne le cèdent pas en importance aux nappes bétiques. Les diverses unités des deux systèmes se raccordent de manière évidente par la courbure de Gibraltar. L'âge du paroxysme tectonique paraît entièrement compris entre Oligocène supérieur et Miocène supérieur, aucune preuve objective n'existant de nappes plus anciennes.La remise en place des divers ensembles structuraux dépend de l'hypothèse générale définie au départ. Il est d'abord fait allusion à l'interprétation classique, par charriages modérés, ne faisant pas appel à des modifications importantes dans l'emplacement des bassins sédimentaires, actuellement visibles en plan. Les objections à ce premier schéma paraissent déterminantes.Une deuxième interprétation, que l'auteur a déjà partiellement esquissée auparavant, sera envisagée: les unités externes (s'empilant sur elles-mêmes) et leurs socles s'enfonceraient sous les zones internes qui, par réaction, seraient poussées vers l'extérieur de la chaîne: chacune des nappes dépasserait la nappe plus basse, au cours de ce mouvement. Dans le cas de l'Espagne, avant les charriages, les domaines sédimentaires des zones internes se placeraient à l'inverse de la disposition actuelle, soit du N au S: Nevadides, Alpujarrides, Malaguides, Pénibétique et Flyschs gaditans (ultras). Du côté marocain, nous aurions de même du S au N: Sebtides, Ghomarides, Tétouanides, Flyschs nord-rifains (ultras). Cela obligerait, au total, à faire rapprocher l'un de l'autre, en profondeur, les bâtis de la Meseta ibérique et de l'Atlas marocain, d'environ 300 à 500 km, l'actuelle largeur de la mer d'Alboran (150 km) ne permettant pas de reloger les domaines de toutes les nappes. Un axe d'enfouissement serait à rechercher sous l'actuelle Méditerranée.Une troisième interprétation, proposée aujourd'hui par l'auteur, considère que la chaîne péri-méditerranéenne montre une cicatrice structurale fondamentale, qui séparerait domaines internes bétiques et rifains, d'une part, domaines bétiques et rifains plus externes, de l'autre. Cette cicatrice se couderait au niveau de Gibraltar. Les nappes internes seraient comme aspirées vers la cicatrice ainsi que, en sens inverse, les nappes externes. La reconstitution paléogéographique finale est fort satisfaisante et l'ampleur des rétrécissements sensiblement diminuée.La position du domaine des Flyschs kabyles, nord-rifains et gaditans, fait enfin l'objet d'un examen nouveau: sans rejeter l'origine ultra, déjà proposée, l'auteur envisage d'autres solutions, qui auraient l'avantage de mieux s'intégrer dans l'image proposée aujourd'hui.  相似文献   

Geographic structure of European anchovy: A nuclear-DNA study     

Yanis Bouchenak-Khelladi  Jean-Dominique Durand  Antonios Magoulas  Philippe Borsa   《Journal of Sea Research》2008,59(4):269-278

Atlantic–Mediterranean anchovies were genetically characterized at two polymorphic nuclear loci (intron 6 of two creatine-kinase genes) and compared to reference Engraulis albidus and E. encrasicolus samples from the northern Western Mediterranean to provide new insights into their geographic structure. Northeastern Atlantic anchovy, represented by one sample from the Canary archipelago and one sample from the Alboran Sea, were genetically distinct from Mediterranean E. encrasicolus (Weir and Cockerham's ^θ = 0.027–0.311), indicating geographic isolation from either side of the Almería–Oran oceanographic front. Generally smaller genetic differences were evident among anchovy populations from different sub-basins in the Mediterranean (^θ = − 0.019–0.116), the genetic differences between Black Sea and Ionian Sea/Aegean Sea anchovies being the strongest (^θ = 0.002–0.116). There was no evidence of the presence of E. albidus in our samples outside Camargue (northern shore of the Western Mediterranean). However, a sample from the southern Western Mediterranean appeared to be genetically intermediate between E. albidus and Mediterranean E. encrasicolus, indicating possible hybridization. Anchovy from the Benguela current system off southern Africa possessed allele frequencies characteristic of E. albidus at one locus and Northeastern Atlantic anchovy at the other locus, suggesting past introgression.  相似文献   

AMRVAC and relativistic hydrodynamic simulations for gamma-ray burst afterglow phases     

Zakaria Meliani  Rony Keppens  Fabien Casse  Dimitrios Giannios 《Monthly notices of the Royal Astronomical Society》2007,376(3):1189-1200

We apply a novel adaptive mesh refinement (AMR) code, AMRVAC (Adaptive Mesh Refinement version of the Versatile Advection Code), to numerically investigate the various evolutionary phases in the interaction of a relativistic shell with its surrounding cold interstellar medium (ISM). We do this for both 1D isotropic and full 2D jet-like fireball models. This is relevant for gamma-ray bursts (GRBs), and we demonstrate that, thanks to the AMR strategy, we resolve the internal structure of the shocked shell–ISM matter, which will leave its imprint on the GRB afterglow. We determine the deceleration from an initial Lorentz factor  γ= 100  up to the almost Newtonian     phase of the flow. We present axisymmetric 2D shell evolutions, with the 2D extent characterized by their initial opening angle. In such jet-like GRB models, we discuss the differences with the 1D isotropic GRB equivalents. These are mainly due to thermally induced sideways expansions of both the shocked shell and shocked ISM regions. We found that the propagating 2D ultrarelativistic shell does not accrete all the surrounding medium located within its initial opening angle. Part of this ISM matter gets pushed away laterally and forms a wide bow-shock configuration with swirling flow patterns trailing the thin shell. The resulting shell deceleration is quite different from that found in isotropic GRB models. As long as the lateral shell expansion is merely due to ballistic spreading of the shell, isotropic and 2D models agree perfectly. As thermally induced expansions eventually lead to significantly higher lateral speeds, the 2D shell interacts with comparably more ISM matter and decelerates earlier than its isotropic counterpart.  相似文献   

The pattern of Ni and Co abundances in lunar olivines     

John Longhi  Sedelia R. Durand  David Walker 《Geochimica et cosmochimica acta》2010,74(2):784-3045

Near liquidus experiments on peridotite and other olivine normative compositions from 1.7 to 6 GPa confirm the applicability of exchange-based empirical models of Ni and Co partitioning between olivine and silicate liquids with compositions close to the liquidus of peridotite. Given that most estimates of lunar bulk composition are peridotitic, the partitioning models thus lend themselves to calculation of olivine compositions produced during the early stages of magma ocean crystallization. Calculation of olivine compositions produced by fractional crystallization of a model lunar magma ocean, initially 700 km deep, reveals a prominent maximum in Ni concentration versus fraction crystallized or Mg’ (molar MgO/(MgO + FeO)), but a pattern of monotonically increasing Co concentration. These patterns qualitatively match the puzzling patterns of Ni and Co concentrations observed in lunar rocks in which forsteritic olivines in magnesian suite cumulates have lower Ni and Co abundances than do less magnesian olivines from low-Ti mare basalts, and olivines from the ferroan anorthosite suite (FAS) have lower Ni, but similar Co to mare basalt olivines.The Ni and Co abundances in olivines from the magnesian suite cumulates can be reconciled in terms of fractional crystallization of a deep magma ocean which initially produces a basal dunite comprised of the hottest and most magnesian olivine overlain by an olivine-orthopyroxene (harzburgite) layer that is in turn overlain by an upper zone of plagioclase-bearing cumulates. The ultramafic portion of the cumulate pile overturns sending the denser harzburgite layer, which later becomes a portion of the green glass source region, to the bottom of the cumulate pile with Ni- and Co-rich olivine. Meanwhile, the less dense, but hottest, most magnesian olivines with much lower Ni and Co abundances are transported upward to the base of the plagioclase-bearing cumulates where subsequent heat transfer leads to melting of mixtures of primary dunite, norite, and gabbronorite with KREEP (a K-REE-P enriched component widely believed to be derived from the very latest stage magma ocean liquid). These hybrid melts have Al₂O₃, Ni, and Co abundances and Mg’ appropriate for parent magmas of the magnesian suite. Ni and Co abundances in the FAS are consistent with either direct crystallization from the magma ocean or crystallization of melts of primary dunite-norite mixtures without KREEP.  相似文献   

The recording of floods and earthquakes in Lake Chichój,Guatemala during the twentieth century     

Gilles Brocard  Thierry Adatte  Olivier Magand  Hans-Rudolf Pfeifer  Albedo Bettini  Fabien Arnaud  Flavio S. Anselmetti  Sergio Moran-Ical 《Journal of Paleolimnology》2014,52(3):155-169

Laguna Chichój (Lake Chichój) is the only deep permanent lake in the central highlands of Guatemala. The lake is located in the boundary zone between the North American and Caribbean plates. The lake has been struck by devastating earthquakes and tropical cyclones in historical times. We investigated the imprint of twentieth century extreme events on the sedimentary record of this tropical lake using a bathymetric survey of the lake, coring the lake floor, and providing a chronology of sediment accumulation. The lake occupies a series of circular depressions likely formed by the rapid dissolution of a buried body of gypsum. ²¹⁰Pb and ¹³⁷Cs inventories and varve counting indicate high rates of sedimentation (1–2 cm year^?1). The annually layered sediment is interrupted by turbidites of two types: a darker-colored turbidite, enriched in lake-derived biogenic constituents, and interpreted as a seismite, and a lighter-colored type, enriched in catchment-derived constituents, interpreted as a flood layer. Comparison of our ¹³⁷Cs-determined layer ages with a catalog of twentieth century earthquakes shows that an earthquake on the Motagua fault in 1976 generated a conspicuous darker-colored turbidite and slumped deposits in separate parts of the lake. The entire earthquake inventory further reveals that mass movements in the lake are triggered at Modified Mercalli Intensities higher than V. Tropical cyclonic depressions known to have affected the lake area had limited effect on the lake, including Hurricane Mitch in 1998. One storm however produced a significantly thicker flood layer in the 1940s. This storm is reportedly the only event to have generated widespread slope failures in the lake catchment. It is thus inferred that abundant landsliding provided large amounts of concentrated sediment to the lake, through hyperpycnal flows.  相似文献   

Observed intra-seasonal to interannual variability of the upper ocean thermal structure in the southeastern Arabian Sea during 2002–2008     

V.V. Gopalakrishna  F. Durand  K. Nisha  M. Lengaigne  T.P. Boyer  J. Costa  R.R. Rao  M. Ravichandran  S. Amrithash  L. John  K. Girish  C. Ravichandran  V. Suneel 《Deep Sea Research Part I: Oceanographic Research Papers》2010,57(6):739-754

The southeastern Arabian Sea (SEAS), located in the Indian Ocean warm pool, is a key-region of the regional climate system. It is suspected to play an important role in the dynamics of the Asian summer monsoon system. The present study reports the salient features derived from a newly harvested observational dataset consisting of repeated fortnightly XBT transects in the SEAS over the period 2002–2008. The fortnightly resolution of such a multi-year record duration is unprecedented in this part of the world ocean and provides a unique opportunity to examine the observed variability of the near-surface thermal structure over a wide spectrum, from intra-seasonal to interannual timescales. We find that most of the variability is trapped in the thermocline, taking the form of upwelling and downwelling motions of the thermal stratification. The seasonal variations are consistent with past studies and confirm the role of the monsoonal wind forcing through linear baroclinic waves (coastally-trapped Kelvin and planetary Rossby waves). Sub-seasonal variability takes the form of anomalous events lasting a few weeks to a few months and occurs at two preferred timescales: in the 30–110 day band, within the frequency domain of the Madden–Julian oscillation and in the 120–180 day band. While this sub-seasonal variability appears fairly barotropic in the offshore region, the sign of the anomaly in the upper thermocline is opposite to that in its lower part on many occasions along the coast. Our dataset also reveals relatively large interannual temperature variations of about 1 °C from 50 to 200 m depth that reflect a considerable year-to-year variability of the magnitude of both upwelling and downwelling events. This study clearly demonstrates the necessity for sustained long-term temperature measurements in the SEAS.  相似文献   

Simulating stochastically excited oscillations: The mode lifetime of ξ Hya     

Dennis Stello  Hans Kjeldsen  Timothy R. Bedding  Joris De Ridder  Conny Aerts  Fabien Carrier  SØren Frandsen 《Solar physics》2004,220(2):207-228

The discovery of solar-like oscillations in the giant star ξ Hya (G7 III) was reported by Frandsen et al. (2002). Their frequency analysis was very limited due to alias problems in the data set (caused by single-site observations). The extent to which the aliasing affected their analysis was unclear due to the unknown damping time of the stellar oscillation modes. In this paper we describe a simulator created to generate time series of stochastically excited oscillations, which takes as input an arbitrary window function and includes both white and non-white noise. We also outline a new method to compare a large number of simulated time series with an observed time series to determine the damping time, amplitude, and limited information on the degree of the stochastically excited modes. For ξ Hya we find the most likely amplitude to be ∼ 2 m s⁻¹, in good agreement with theory (Houdek and Gough, 2002), and the most likely damping time to be ∼ 2 days, which is much shorter than the theoretical value of 15–20 days calculated by Houdek and Gough (2002).  相似文献   

Multiproxy approach for determination of nature and origin of carbonate micro-particles so-called “micarb” in pelagic sediments     

Catherine Beltran  Marc de Rafélis  Alain Person  Fabien Stalport  Maurice Renard 《Sedimentary Geology》2009,213(1-2):64-76

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Ab initio quantum mechanical study of γ-AlOOH boehmite: structure and vibrational spectrum     

Yves Noel  Raffaella Demichelis  Fabien Pascale  Piero Ugliengo  Roberto Orlando  Roberto Dovesi 《Physics and Chemistry of Minerals》2009,36(1):47-59

The structure and vibrational spectrum of boehmite have been investigated at the quantum-mechanical level with the CRYSTAL code, using a Gaussian-type basis set and the B3LYP Hamiltonian. Three space groups are considered in this study: Cmcm, Cmc2₁, P2₁/c. Cmcm turns out to correspond to a transition state, whereas Cmc2₁ and P2₁/c are minimum energy structures. The difference among them is the position of H atoms only, the Al-O frame being essentially the same. Harmonic frequencies at the Γ point have been computed. The comparison between calculated and experimental frequencies shows a good agreement for the Al-O part of the spectrum (under 790 cm⁻¹). For the Al-OH bending modes (800–1,300 cm⁻¹) an absolute differences of 50–100 cm⁻¹ is observed; for the OH stretching modes (3,200–3,500 cm⁻¹) it increases to 120–200 cm⁻¹: anharmonicity is large because OH groups are involved in strong hydrogen bonds.  相似文献   

Contamination and Sources Identification of Polycyclic Aromatic Hydrocarbons in Water and Sediments of Annaba Bay Basin,Algeria     

Soumeya Khaled-Khodja  Cheraitia  Hassen  Durand  Gaël  Cherif  Semia 《Water Resources》2021,48(1):111-123

Water Resources - Annaba gulf is a coastal area (southwestern Mediterranean Sea) that receives large diffuse inputs from Fertial plant, Seybouse wadi and Boujemaâ wadi, which are influenced by...  相似文献