Effet de l'agrégation sur le transport de la kaolinite recouverte d'acide humique à travers un sable de quartz d'origine naturelleAggregation effect on the transport of humic-coated kaolinite colloids through a natural quartz sand     

Rachid Ait Akbour  Jamaâ Douch  Mohamed Hamdani  Philippe Schmitz 《Comptes Rendus Geoscience》2002,334(13):981-985

To evaluate the risk of contaminant transport by mobile colloids, it is necessary to understand how colloids and associated pollutants behave during their migration through uncontaminated soil or groundwater. In this study, we investigated the influence of aggregation induced by Ca²⁺ and trace metals (Pb²⁺, Cu²⁺) concentrations on the transport of humic-coated kaolinite colloids through a natural quartz sand at pH=4. Adsorbed divalent cations reduce the colloids surface charge and thereby induce aggregation and deposition in porous media. To cite this article: R. Ait Akbour et al., C. R. Geoscience 334 (2002) 981–985.  相似文献   

Environmental changes over the past 25 000 years in the southern Middle Atlas,Morocco          下载免费PDF全文

Jalal Tabel  Carla Khater  Ali Rhoujjati  Laurent Dezileau  Ilham Bouimetarhan  Matthieu Carre  Laurence Vidal  Abdelfattah Benkaddour  Majda Nourelbait  Rachid Cheddadi 《第四纪科学杂志》2016,31(2):93-102

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Hydrochemical and isotopic investigations as indicators of recharge processes of the Continental Intercalaire aquifer (eastern piedmont of Dahar,southern Tunisia)     

Zahra Dhaoui  Kamel Zouari  Jean-Denis Taupin  Rachid Farouni 《Environmental Earth Sciences》2016,75(16):1186

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Inter-season and interannual variations in fish and macrocrustacean community structure on a eastern English Channel sandy beach: Influence of environmental factors     

Jonathan Selleslagh  Rachid Amara 《Estuarine, Coastal and Shelf Science》2008,77(4):721-730

The intertidal zone of an exposed sandy beach on the French coast of the English Channel was sampled with a 1.5 m beam-trawl over five years (2000 and 2003–2006) at weekly intervals. The fish and macrocrustacean catches were analysed to determine the inter-season and interannual variation in community structure and relate these variations to changes in the major environmental variables. Only six species (plaice Pleuronectes platessa, common goby Pomatoschistus microps, sprat Sprattus sprattus, sand eel Ammodytes tobianus, brown shrimp Crangon crangon and shore crab Carcinus maenas) from the 27 species captured can be considered as dominant species of the intertidal zone, and they accounted for >90% of total numbers. Most individuals caught were young-of-the-year or juvenile. Analysis of similarities (ANOSIM) and similarities percentage (SIMPER) indicated that inter-season variability of community structure (mean average similarity = 47%) was more pronounced than interannual variability (mean average similarity = 65%). Canonical correspondence analysis (CCA) indicates that a substantial component (32.2%) of the measured inter-season variation in community structure can be explained by environmental factors (mainly water temperature). The main inter-season changes in the abundance and community structure were due to the variation of the six key species and reflect the different times of their recruitment. During the five years of the study, the structure of the fish and macrocrustacean spring community persisted from year to year, with the dominant species reappearing consistently even though their abundances fluctuated from year to year. This interannual variation probably reflects variable recruitment success influenced by physico-chemical conditions. In spite of the considerable interannual variation (40 times) in the spring bloom of the prymnesiophyte alga Phaeocystis globosa we found no effect of this bloom on either fish and macrocrustacean species densities or diversity index.  相似文献   

Controlling the collimation and rotation of hydromagnetic disc winds     

Ralph E. Pudritz  Conrad S. Rogers  Rachid Ouyed 《Monthly notices of the Royal Astronomical Society》2006,365(4):1131-1148

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Quark-nova remnants: application to RRATs     

Rachid Ouyed  Denis Leahy  Brian Niebergal  Youling Yue 《Monthly notices of the Royal Astronomical Society》2009,396(2):1058-1065

This is the third paper of a series of papers where we explore the evolution of iron-rich ejecta from quark-novae. In the first paper, we explored the case where a quark-nova ejecta forms a degenerate shell, supported by the star's magnetic field, with applications to SGRs. In the second paper, we considered the case where the ejecta would have sufficient angular momentum to form a degenerate Keplerian torus and applied such a system to two AXPs, namely 1E2259+586 and 4U0142+615. Here, we explore the late evolution of the degenerate torus and find that it can remain unchanged for  ∼10⁶ yr  before it becomes non-degenerate. This transition from a degenerate torus (accretion-dominated) to a non-degenerate disc (no accretion) occurs about 10⁶ yr following the quark-nova, and exhibits features that are reminiscent of observed properties of Rotation RAdio Transients (RRATs). Using this model, we can account for the duration of both the radio bursts and the quiet phase, as well as the observed radio flux from RRATs. We discuss a connection between XDINs and RRATs and argue that some XDINs may be 'dead RRATs' that have already consumed their non-degenerate disc.  相似文献   

Chromothermal oscillations and collapse of strange stars to black holes: astrophysical implications     

Manjari Bagchi  Rachid Ouyed  Jan Staff  Subharthi Ray  Mira Dey †  Jishnu Dey ‡ 《Monthly notices of the Royal Astronomical Society》2008,387(1):115-120

We study the effects of temperature on strange stars. It is found that the maximum mass of the star decreases with the increase of temperature, as at high temperatures the equations of state become softer. Moreover, if the temperature of a strange star increases, keeping its baryon number fixed, its gravitational mass increases and its radius decreases. This leads to a limiting temperature, where it turns into a black hole. These features are the result of a combined effect of the change of gluon mass and the quark distribution with temperature. We report on a new type of radial oscillation of strange stars, driven by what we call 'chromothermal' instability. We also discuss the relevance of our findings in the astrophysics of core collapse supernovae and gamma-ray bursts.  相似文献   

Supernova SN2006gy as a first ever Quark Nova?     

Denis Leahy  Rachid Ouyed 《Monthly notices of the Royal Astronomical Society》2008,387(3):1193-1198

The most luminous Supernova SN2006gy (more than 100 times brighter than a typical supernova) has been a challenge to explain by standard models. For example, pair-instability supernovae which are luminous enough seem to have too slow a rise, and core-collapse supernovae do not seem to be luminous enough. We present an alternative scenario involving a Quark Nova (an explosive transition of the newly born neutron star to a quark star) in which a second explosion (delayed) occurs inside the ejecta of a normal supernova. The reheated supernova ejecta can radiate at higher levels for longer periods of time primarily due to reduced adiabatic-expansion losses, unlike the standard supernova case. We find an encouraging match between the resulting light curve and that observed in the case of SN2006gy suggesting that we might have at hand the first ever signature of a Quark Nova. Successful application of our model to SN2005gj and SN2005ap is also presented.  相似文献   

New data on the Lower Mesozoic basal series of the Traras mounts (Tlemcen,northwestern Algeria)     

Menad Ferhat  Rachid Ait Ouali 《Arabian Journal of Geosciences》2017,10(15):338

The lower Mesozoic of the Traras mount starts with the so-called Red Series, which lays uncomformably on the folded and granitized Paleozoic basement. This series is overlain by Middle Liassic limestones. On the basis of its lower and upper limits and the lack of dating evidence, former authors attribute a Permian to lower Liassic (Sinemurian) age for this series. Palynological results allow to range it in the upper Triassic probably Norian-Rhetian. The Red Series is studied from five sections that depict important thickness and facies variations from southwest to the northeast, inferring the irregularities of the Hercynian erosional surface. In the Central Traras, this series shows over 130-m-thick micaceous sandy conglomeratic units, deposited within alluvial fans, where the bedrock source corresponds to granite of Nedroma or its equivalent. In the southern and eastern Traras, where the series’ thickness respectively does not exceed 30 m and averages 40–80 m, besides alluvial deposits issued from hercynian basement erosion, it exhibits volcanic evidences interbedded by lacustrine deposits. Vertical and spatial distribution depicts synsedimentary infilling of narrow elongated rift basins, typically half-grabens, bounded on one side by a normal fault or a series of normal faults trending NNE-SSW to NW-SE, inherited from the hercynian event. The study of tectonostratigraphic units permitted to put forward geodynamics of the infilling basins.  相似文献   

失水对海洋沉积物磁学性质的影响     

李明坤  欧阳婷萍  田成静  朱照宇  唐志华  彭学超  邱燕  钟和贤． 《热带地理》2016,36(3):438-447

为了探究沉积物的干燥过程及方式对其磁学性质的影响,选取含水率高的南海沉积物样品,对其中685个样品在自然条件下逐步晾干,并每间隔40 d测量1次低频磁化率（κlf）、高频磁化率（κhf）、饱和等温剩磁（SIRM）、S-300和频率磁化率系数（κfd）,共测量5次;对另外60个样品进行冷冻干燥,并在干燥前后测量相同的磁学参数。结果表明：1）自然晾干过程中,除少数异常点（约7%）外,大多数样品的κlf和κhf呈减小趋势,少数样品呈增大趋势,S-300和κfd均呈减小趋势,SIRM先减后增,整体上呈增大趋势;2）冷冻干燥过程中,样品的κlf、κhf、S-300和κfd呈增大趋势,SIRM呈减小趋势;3）2种干燥方法均不影响κlf、κhf、SIRM和S-300的剖面变化趋势,但对κfd的影响较大,这在磁学指标的古环境研究中具有关键的指示意义。磁学参数的变化,可能是由于失水过程发生的微弱氧化作用、失水导致水的抗磁性“负贡献”降低、细粒磁铁矿和磁赤铁矿在湿润状态下转变成顺磁性和不完全反铁磁性等综合因素造成的。建议对同一批次的样品采取相同的干燥方法。  相似文献