Fish stocks and their management: The changing face of fisheries in South Africa     

George M. Branch  Barry M. Clark 《Marine Policy》2006

Transformation of South African marine fisheries over the past 10 years has had to balance economic stability, equity and sustainability. This is being done in three ways. First, access rights have been redistributed, increasing the number of rights holders 20-fold and the participation of historically disadvantaged individuals from 0.75% to 62%. Second, established companies have undergone internal transformation. Third, subsistence fishers have formally been recognised. New focuses include co-management, ecosystem-based management and marine protected areas. Further necessary steps include parity in salaries, attention to artisanal fishers, embracement of co-management, expansion of subsistence management and effective enforcement. Most stocks are healthy or recovering but exceptions, such as abalone, warn how quickly stocks can be decimated if co-operation is not achieved.  相似文献   

Dietary change of the rock lobster Jasus lalandii after an ‘invasive’ geographic shift: Effects of size,density and food availability     

C.N. Haley  L.K. Blamey  L.J. Atkinson  G.M. Branch 《Estuarine, Coastal and Shelf Science》2011,93(2):160-170

During the 1990s the rock lobster Jasus lalandii shifted its focus of distribution south-eastwards along the coast of South Africa, to establish a dense population in an area where it was previously rare. This coincided with a marked decrease in the sea urchin Parechinus angulosus, a preferred prey item of J. lalandii and a vital source of shelter for juveniles of the abalone Haliotis midae. The range expansion of lobsters has thus economic and ecological ripple effects. We determined the diets of small (50–65 mm carapace length) and large (>69 mm CL) rock lobsters from gut content analyses, and compared them between three ‘lobster invaded’ sites and three adjacent ‘non-invaded’ sites where densities are still low. At the non-invaded sites, diets were collectively heterogeneous but the dietary breadth of individual lobsters was narrow (in contradiction to generally accepted ecological theory), and the lobsters fed mainly on large, individual, mobile, high-energy prey such as sea urchins and large winkles. Conversely, at invaded sites where lobster densities were high, they consumed predominantly small, colonial or sessile low-energy prey such as sponges, barnacles and foliar algae, and the diet was significantly more uniform among individuals, but broader within individuals. This was a direct result of the contrasting benthic community structure of the two areas, and consequent prey availability – itself caused by differences in intensity of rock-lobster predation. Cannibalism was unexpectedly greater at non-invaded sites, possibly as a result of lobsters being larger there. The diet of small and large lobsters also differed significantly. Large rock lobsters predominantly consumed large individual prey such as lobsters, urchins and crabs, while small rock lobsters ate mainly colonial, sessile prey such as sponges and barnacles, and small prey such as tiny winkles and crustaceans. Dietary selectivity indices revealed that algae and sponges were negatively selected (avoided) in non-invaded areas but positively or neutrally selected in invaded areas. These dietary differences have important ramifications not only for the lobster populations but also for the structure and functioning of the radically different communities that have developed in invaded areas, reflecting a regime shift induced by lobster predation.  相似文献   

三维非均匀介质中真振幅地震偏移算子研究   总被引：31，自引：6，他引：25       下载免费PDF全文

崔兴福  张关泉  吴雅丽 《地球物理学报》2004,47(3):509-513

利用三维非均匀介质中的波动方程,进行振幅保真波场偏移算子分解,得到用于真振幅偏移的单程波方程. 经过数学推理,导出裂步Fourier法真振幅偏移和Fourier有限差分法真振幅偏移的算子方程,并给出其具体的实现过程.  相似文献   

川东北飞仙关组鲕滩天然气地球化学特征与成因   总被引：29，自引：3，他引：26  

谢增业  田世澄  李剑  胡国艺  李志生  马成华 《地球化学》2004,33(6):567-573

四川盆地东北部下三叠统飞仙关组鲕滩气藏天然气烃类气体以甲烷为主,含量主要分布在75%～90%之间,C2 含量很少,为0%～0.15%,干燥系数为0.997 0～0.999 8,是典型的干气;非烃气体以H2S和CO2为主,含量分别为4.21%～16.24%和0.97%～10.41%.天然气δ13C1值为-29.0‰～-31.5‰,δ13C2值为-29.4‰～-32.4‰.多参数表明鲕滩气藏天然气是以腐泥型为主的高过成熟天然气.高含H2S的天然气分布区域与含石膏地层分布基本一致,这些H2S为飞仙关组气藏附近的石膏经热化学硫酸盐还原作用(TSR)而生成,CO2是其主要的副产物.在TSR过程中,C2 重烃气体比甲烷更容易与硫酸盐发生反应,也就是C2 重烃气体的消耗速率大于甲烷,从而导致发生TSR反应的天然气C2 含量低、H2S和CO2含量高.天然气δ13C1值与甲烷含量之间具有很好的负相关关系,而与天然气酸性系数[H2S/(H2S CnH2n 2)]具有正相关关系.根据同位素动力学的分馏效应,随着TSR的进行,烃类分子中的12C损耗速率大于13C,残留下来的烃类分子中则更加富集13C,也就是TSR反应使天然气碳同位素变重.  相似文献   

准噶尔盆地腹部超压顶面附近深层砂岩碳酸盐胶结作用和次生溶蚀孔隙形成机理   总被引：2，自引：1，他引：1  

何生  杨智  何治亮  武恒志  王芙蓉  孟闲龙 《地球科学》2009,34(5):759-768

准噶尔盆地腹部深层超压顶面附近(现今埋深4400~6200m, 温度105~145℃) 砂岩中广泛出现的碳酸盐胶结作用和次生溶蚀孔隙与超压流体活动关系密切.由于超压封闭和释放引起其顶面附近砂岩中的孔隙压力和水化学环境的周期性变化可导致碳酸盐沉淀和易溶矿物溶解过程交替出现.根据腹部地区超压顶面附近深埋砂岩成岩作用、碳酸盐胶结物含量、储集物性、碳酸盐胶结物碳、氧同位素和烃源岩热演化模拟等资料的综合研究表明: 含铁碳酸盐胶结物是主要的胶结成分, 长石类成分的次生溶蚀孔隙是主要的储集空间类型, 纵向上深层砂岩碳酸盐胶结物出现15%~30%含量的地层厚度范围约在邻近超压顶面之下100m至之上大于450m, 碳酸盐胶结物出现大于25%含量高值带分布在靠近超压顶面向上的250~300m的地层厚度范围, 超压顶面附近砂岩中碳酸盐胶结物含量高值的深度范围也是次生溶蚀孔隙(孔隙度10%~20%) 发育带的范围; 因晚白垩世以来深部侏罗纪煤系有机质生烃增压作用, 导致在超压顶面附近砂岩晚成岩作用阶段深部富含碳酸盐的超压流体频繁活动, 所形成的碳酸盐胶结物受到了明显的与深部生烃增压有关的超压热流体和有机脱羧作用的影响; 超压流体多次通过超压顶面排放, 使得超压顶面附近砂岩遭受了多期酸性流体溶蚀作用过程, 形成了次生溶蚀孔隙发育带.   相似文献   

准噶尔盆地腹部侏罗系超压特征和测井响应以及成因   总被引：3，自引：1，他引：2  

何生  何治亮  杨智  武恒志  王芙蓉  石万忠 《地球科学》2009,34(3):457-470

准噶尔盆地腹部地区深层钻井揭示侏罗系发育异常高压系统.根据26口井的67个钻杆测试(DST) 和电缆测试(MDT) 数据, 实测砂岩异常高压揭示深度约在4470~6160m, 剩余压力约为11~57MPa, 压力系数为1.24~2.07, 砂岩段超压实测值主要分布在侏罗系, 少数出现在白垩系底部与侏罗系邻近地层, 1个超压实测值位于下三叠统, 实测超压砂岩样品的孔隙度和渗透率范围分别为3.20%~16.00%和0.02×10-3~14.40×10-3μm2;根据钻井、测井和测试资料的综合解释, 埋深在4430~6650m的深部侏罗系流体超压带, 钻井泥浆密度明显增加, 泥页岩和砂岩共同具有相对于正常趋势的异常高声波时差和低视电阻率测井响应特征; 超压系统顶界埋深可能不浅于4400m (地温约104℃), 有些钻井超压顶界可深达约6000m (地温约140℃), 且超压带顶界深度随侏罗系埋深的增加而增大; 钻井揭示的侏罗系超压带烃源岩镜质体反射率(R_o, %) 约为0.7%~1.3%, 超压带分布深度受控于侏罗系成熟烃源岩层的埋深且两者深度分布的变化具有相关性; 研究认为腹部地区已被充分压实的侏罗系异常高压成因主要与其含煤岩系干酪根热演化及油气共生有关, 即生烃增压; 物理模拟实验表明, 由于高孔隙流体压力可导致岩石骨架颗粒间有效应力的减小, 从而直接引起通过岩石的声波速度降低, 即出现高声波时差响应; 在超压地层温度条件下, 高压液态水的电离常数可能明显增加, 从而减小地层电阻率, 进一步开展此种现象的相关探索性研究可望对超压带低电阻率异常的原因给出新的解释.   相似文献   

南海北部渐新世末的构造事件   总被引：3，自引：2，他引：1  

邵磊  庞雄  张功成  乔培军  李前裕  韦刚健  吴梦霜 《地球科学》2009,34(5):717-724

ODP1148站以及珠江口盆地沉积物均记录了渐新世末发生的重大地质构造事件, 这一构造事件在时间上与南海扩张轴发生跳跃的时间十分吻合, 是渐新世以来南海构造演化史上最为重大的构造事件, 涉及到南海扩张、盆地类型转化、沉积物源变迁等一系列相关联的重大地质事件.伴随这一地质构造事件, 南海北部沉积物成分发生剧烈改变, 出现渐新世-中新世地球化学成分上的跳跃, 在深海沉积中发生沉积间断及滑塌事件, 并使珠江口盆地由断陷型盆地转为坳陷型盆地, 白云凹陷由渐新世晚期的浅水陆架环境转为中新世以后的深水陆坡环境.可以认为, 这次构造运动奠定了我国现代的地理格局, 也标志着我国东部陆相盆地最佳烃源岩形成期的结束, 在南海乃至东亚地区影响深远.   相似文献   

Using in situ REE analysis to study the origin and diagenesis of dolomite of Lower Paleozoic,Tarim Basin     

WANG XiaoLin  JIN ZhiJun  HU WenXuan  ZHANG JunTao  QIAN YiXiong  ZHU JingQuan & LI Qing State Key Laboratory for Mineral Deposits Research  School of Earth Sciences  Engineering  Nanjing University  Nanjing  China  Petroleum Exploration  Development Institute of SINOPEC  Beijing  SINOPEC Northwest Oil Field Branch  Urumqi 《中国科学D辑(英文版)》2009,(5)

In situ REE concentrations of various dolomites from Tarim Basin were obtained by LA-ICP-MS analysis,and the data were normalized to standard seawater(Seawater Normalized=SWN).Most of the samples have a ΣREE range of less than 20 ppm.All samples show similar REESWN distributions with heavy REE depletion,and positive Ce anomaly,which indicates that they have the same dolomitization fluids(seawater).According to the origin and diagenetic process of dolomite,two types of dolomite are determined and described a...  相似文献   

Massive stars exploding in a He-rich circumstellar medium – I. Type Ibn (SN 2006jc-like) events     

A. Pastorello  S. Mattila  L. Zampieri  M. Della Valle  S. J. Smartt  S. Valenti  I. Agnoletto  S. Benetti  C. R. Benn  D. Branch  E. Cappellaro  M. Dennefeld  J. J. Eldridge  A. Gal-Yam  A. Harutyunyan  I. Hunter  H. Kjeldsen  Y. Lipkin  P. A. Mazzali  P. Milne  H. Navasardyan  E. O. Ofek  E. Pian  O. Shemmer  S. Spiro  R. A. Stathakis  S. Taubenberger  M. Turatto  H. Yamaoka 《Monthly notices of the Royal Astronomical Society》2008,389(1):113-130

We present new spectroscopic and photometric data of the Type Ibn supernovae 2006jc, 2000er and 2002ao. We discuss the general properties of this recently proposed supernova family, which also includes SN 1999cq. The early-time monitoring of SN 2000er traces the evolution of this class of objects during the first few days after the shock breakout. An overall similarity in the photometric and spectroscopic evolution is found among the members of this group, which would be unexpected if the energy in these core-collapse events was dominated by the interaction between supernova ejecta and circumstellar medium. Type Ibn supernovae appear to be rather normal Type Ib/c supernova explosions which occur within a He-rich circumstellar environment. SNe Ibn are therefore likely produced by the explosion of Wolf–Rayet progenitors still embedded in the He-rich material lost by the star in recent mass-loss episodes, which resemble known luminous blue variable eruptions. The evolved Wolf–Rayet star could either result from the evolution of a very massive star or be the more evolved member of a massive binary system. We also suggest that there are a number of arguments in favour of a Type Ibn classification for the historical SN 1885A (S-Andromedae), previously considered as an anomalous Type Ia event with some resemblance to SN 1991bg.  相似文献   

瞬变电磁场的直接时域数值分析   总被引：44，自引：9，他引：35  

闫述  陈明生  傅君眉 《地球物理学报》2002,45(2):275-284

为了深入了解瞬变电磁场的勘探原理,直接在时间域对负阶跃脉冲激发的二维瞬态场进行了数值分析.采用的方法是从反映电磁场基本规律的麦克斯韦方程组出发,导出时域电场的齐次扩散方程,对所研究的空间区域作差分离散,源作为初始条件加入,利用准静态近似处理空中边界,然后进行时间的逐步递推,由此展现瞬变电磁场在地下扩散随时间发展的全过程.通过模拟计算不同时刻瞬态电场在地下的分布形态及地面上感生电动势相应的变化,揭示了低阻异常体对感应涡流的聚集作用,低阻覆盖层对瞬变场扩散的减速作用,及瞬变场的延时效应.因此,瞬变电磁法对低阻体是敏感的,有上覆低阻层时探测同样的深度需要较长的时间,而延时效应瞬变场的晚期时段可反映埋藏较浅的异常体.  相似文献