珠江三角洲三水盆地早全新世以来 孢粉分析与古环境重建

为了深入探讨珠江三角洲的沉积古环境和古气候历史,在三水市区获取了2个高取芯率的钻孔岩芯,进行了12个AMS 14C测年,并结合孢粉、硅藻等分析结果探讨三水地区全新世的海平面与河流水动力变化,以及古植被演替过程。结果表明：钻孔所在区域全新世沉积总体从9 000 cal. a B.P.左右开始,呈现河流相―河湾相―河口湾相―潮坪相―河口湾相―河漫滩相的演变过程。三水区的早全新世沉积阶段年代最早为9 000 cal. a B.P.左右,表现为河口湾相的淤泥质粉砂沉积,硅藻以淡水种类为主,最高沉积速率为1.6 cm/a。海侵初始时间为8 700 cal. a B.P.左右,最高海平面时间为7 600 cal. a B.P.左右,此时海岸带发育红树林,丘陵山地发育较茂盛的亚常绿热带常绿阔叶林;中―晚全新世阶段（6 500―2 200 cal. a B.P.）,以泥炭粉砂沉积为主,沉积速率为0.2~0.5 cm/a,河口区高潮线附近及河流弯道低洼滩地在5 000 cal. a B.P.前后形成淡水沼泽、河口三角洲边缘区洼地水松林发育。在晚全新世（2 200 cal. a B.P.左右）以来,陆相黏土质沉积指示河口泥沙快速堆积,三角洲平原迅速扩大,沉积速率高达1.7 cm/a。孢粉结果显示次生的芒箕孢子剧增,陆地植被稀疏,人类活动显著增强。     

失水对海洋沉积物磁学性质的影响

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。     

西方乡村性研究进展

在梳理20世纪60年代以来乡村性研究的社会、学术背景的基础上,聚焦于乡村性的社会建构流派及其对中国乡村转型与乡村地理研究的启示。社会建构流派将乡村性看作是社会、文化建构的过程与产物而非先存的事实,重点关注乡村转型过程中的权力关系与差异性。由描述性流派、乡土流派向社会建构流派的过渡可以看作是从关注乡村性物质层面转向想象层面,由追求乡村性的本体、核心机制向探索乡村性的认识论问题,也就是从追求“乡村性是什么”到研究“不同社会群体如何认识乡村性”“不同社会群体多样化的乡村性话语和体验”。而目前的中国乡村性研究主要关注乡村性指标及其模型建构,相关研究对于各级政府全面地了解现存的乡村问题并合理地制定乡村发展、复兴政策规划具有重要的实践意义。在西方乡村研究中,乡村性指标由于暗含线性发展观、无法解读乡村变迁的机制和过程而饱受批判。在中国乡村急剧变迁的今天,现代化乡村发展话语占据着主导地位,而在这一过程中不公平的权力关系和霸权话语对部分农村、农民的边缘化基本没有提及。在这种社会与学术背景下,乡村性社会建构流派对于解构乡村性主导话语、揭示乡村变迁过程中的权力关系及不同社会群体间利益冲突与协商具有重要意义。     

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

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.     

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

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.     

SN 2009ip and SN 2010mc as dual-shock Quark-Novae

In recent years a number of double-humped supernovae （SNe） have been discovered. This is a feature predicted by the dual-shock Quark-Nova （QN） model where an SN explosion is followed （a few days to a few weeks later） by a QN explo- sion. SN 2009ip and SN 2010mc are the best observed examples of double-humped SNe. Here, we show that the dual-shock QN model naturally explains their light curves including the late time emission, which we attribute to the interaction between the mixed SN and QN ejecta and the surrounding circumstellar matter. Our model applies to any star （O-stars, luminous blue variables, Wolf-Rayet stars, etc.） provided that the mass involved in the SN explosion is ~ 20 Mo which provides good conditions for forming a QN.     

Quark-nova remnants: application to RRATs

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.     

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

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.