岛屿地形对热带气旋强度影响的数值模拟研究

本文用理想数值模拟分析的方法,在MM5模式中构造对称初始涡旋,在理想的环境场中发展为成熟的TC并移动经过从台湾岛抽象出的岛屿地形,揭示岛屿对TC强度和结构影响的机理。结果表明,理想模拟试验的方法对TC强度及结构变化的模拟具有很好的可靠性和客观性;TC中心登岛至到达岛屿山顶过程中,由于岛屿地形的抬升作用使得垂直方向上产生了局地的狭管收缩效应,使得TC在通过时强度短暂加强;TC在过岛过程中,风速垂直结构以及暖心结构的对称性会因地形的抬升和扰动影响而破坏,同时二者的大值区范围缩小;TC在过岛时,暖心结构在中高层分裂成一大一小2个部分,低层暖心偏离TC低压中心而伸向地面,TC由准正压系统变为斜压系统,使得TC整体强度减弱;次生低压对翻山后的TC中心的吸引融合加速了其过山后的北折过程;TC过岛后强度减弱十分明显,这是由于岛屿地形对环流摩擦阻力较大,对水汽供应的减弱和阻断,以及对TC对称结构的破坏。     

地中海东部的早中生代俯冲——土耳其西北部三叠纪榴辉岩提供的证据

地中海东部的早中生代俯冲——土耳其西北部三叠纪榴辉岩提供的证据ＡｒａｌＯｋａｙ等晚古生代古地理再造表明现今地中海东部地区是一辽阔的海域。虽然有地质证据证明这一地区存在过这个古生代海洋——古特提斯海，但是对于这个古特提斯俯冲史的资料是缺乏的。因此，我们...     

Can turbidity caused by Corophium volutator (Pallas) activity be used to assess sediment toxicity rapidly?

The standard toxicity test organism, Corophium volutator, exhibits a behavioural response to contaminated sediments that causes increased turbidity of overlying water. We quantify the effects of this response to an estuarine sediment spiked with copper and hydrocarbon contaminated sediments from an oil installation in the North Sea. Turbidity measured 24 h after the start of a toxicity test shows a strong relationship with contaminant concentrations and with mortality after 10 days. Turbidity measurements can therefore give a rapid indication of sediment toxicity, permitting a reduction in storage time of sediments to be used in dilution series and toxicity identification evaluation (TIE) tests, reducing the likelihood of contaminants degrading prior to testing.     

Population structure of Haliotis rubra from South Australia inferred from nuclear and mtDNA analyses

1Introduction ThemajorityofAustralia’sabalonefisheryex ports(5.135kt,worth＄216millionin2002～2003,ABARE2004)consistofblacklipabalone(HaliotisrubraLeach,1814).AssuchH.rubrais consideredasanimportantmarineresourcewithin Australia.Likemanyabalonespecieswor…     

Lead contamination of small cetaceans in European waters--the use of stable isotopes for identifying the sources of lead exposure

Lead concentrations and isotopic composition have been measured in bone and teeth of small cetaceans belonging to three species (Delphinus delphis, Phocoena phocoena and Stenella coeruleoalba), to evaluate the toxicological risk and to determine sources of lead in the European waters. Lead concentrations, far lower than threshold value inducing toxic effects in human, were higher in teeth than in bones, but highly correlated between the two tissues (r=0.92, p<0.001). Large variations of 206Pb/207Pb values in bone tissue showed that cetaceans must be submitted to various atmospheric influences. No geographical differences appeared which is consistent with studies on their distribution indicating seasonal movements between Brittany waters and the Bay of Biscay. The negative correlation between 206Pb/207Pb ratios and age of the individuals reflected the decrease in the production of alkyl lead in Europe, i.e., the increasing use of unleaded gasoline.     

1nm锰矿相的金属阳离子交换能力的研究

人工合成的1nm锰矿相和铜、钴、镍等二价金属阳离子的交换实验表明,1nm锰矿相具有强烈的金属阳离子交换能力.正是这种金属阳离子的交换能力,使得大洋多金属结核大量地富集了铜、钴、镍等有价金属元素.1nm锰矿相对几种金属阳离子的交换的优先顺序为:Cu>Co>Zn≥Ni>Ca>Mg.多金属结核中镍的含量往往高于铜、钴、锌等元素,但在交换顺序中它却低于铜、钴、锌等,这种不一致性说明结核成矿后期的金属离子交换并非是有价金属结合进结核的唯一途径.多金属结核富含铜、钴、镍等有价金属可能是结核初始成矿和成矿后期金属离子交换等多种因素共同作用的结果.     

Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?

We present thermal mass loss calculations over evolutionary time scales for the investigation if the smallest transiting rocky exoplanets CoRoT-7b (∼1.68R_Earth) and Kepler-10b (∼1.416R_Earth) could be remnants of an initially more massive hydrogen-rich gas giant or a hot Neptune-class exoplanet. We apply a thermal mass loss formula which yields results that are comparable to hydrodynamic loss models. Our approach considers the effect of the Roche lobe, realistic heating efficiencies and a radius scaling law derived from observations of hot Jupiters. We study the influence of the mean planetary density on the thermal mass loss by placing hypothetical exoplanets with the characteristics of Jupiter, Saturn, Neptune, and Uranus to the orbital location of CoRoT-7b at 0.017 AU and Kepler-10b at 0.01684 AU and assuming that these planets orbit a K- or G-type host star. Our findings indicate that hydrogen-rich gas giants within the mass domain of Saturn or Jupiter cannot thermally lose such an amount of mass that CoRoT-7b and Kepler-10b would result in a rocky residue. Moreover, our calculations show that the present time mass of both rocky exoplanets can be neither a result of evaporation of a hydrogen envelope of a “Hot Neptune” nor a “Hot Uranus”-class object. Depending on the initial density and mass, these planets most likely were always rocky planets which could lose a thin hydrogen envelope, but not cores of thermally evaporated initially much more massive and larger objects.     

河北省崇礼幅1∶50 000矿产地质图数据库

根据《固体矿产地质调查技术要求(1∶50 000)》(DD 2019-02)和行业其他规范要求,完成河北省崇礼幅1∶50 000专项地质填图379.93 km²、矿点检查11处,采集水系沉积物样品1622件、重力测量物理点1623个,测试锆石U-Pb年龄样3组、流体包裹体样80余件,系统编制了河北省崇礼幅1∶50 000矿产地质图,并建立了数据库。突出了对燕山期岩浆岩和相关脉岩、碱性杂岩体和谷嘴子岩组、矿化蚀变等相关成矿信息的表达,厘定了崇礼幅中太古代、新太古代的变质深成侵入体,划分了海西期、印支期、燕山期的岩浆岩建造类型,划分了张家口组火山岩的7个建造类型、谷嘴子岩组变质岩的3个建造类型,系统总结了该区金矿的成矿地质体、成矿构造及成矿结构面、成矿作用特征标志。该数据库为该区金矿的找矿工作提供了基础数据支撑,对金矿目标层地质信息和构造建造信息的提取提供了便利条件,对今后矿产勘查部署具有一定的参考价值。     

铜镍硫化物矿床的成冈——以诺里尔斯克（俄罗斯）和金川（中国）为例

与超基性岩浆作用有关的铜镍硫化物矿床主要有两种成矿建造,一种为含铬建造,另一种为含铂建造。尖晶石类矿物成分的变化清楚地反映了这两类建造的成矿属性,含铬建造的尖晶石属于铬铁矿－尖晶石系列,含铂建造中则为尖晶石－磁铁矿系列。从含铬建造向含铂建造转变的原因,可以解释为超基性岩艇中硫的作用增加,从而引起反应：４ＦｅＯ＋Ｓ＝ＦｅＳ＋Ｆｅ３Ｏ４（磁铁矿）,同时分散性铂族元素的专属性特征也发生相应变化（Ｒｕ＋Ｏｓ＋Ｉｒ）→（Ｐｔ＋Ｐｄ）。因此,含铬建造中主要富含Ｒｕ、Ｏｓ和Ｉｒ,而含铂建造中则富含Ｐｔ和Ｐｄ。超基性岩浆作用中硫的化学活动性增加与基碱度增加直接有关。因此,含铂的超基性岩大多数情况下与富碱的玄武岩形成共生组合,当富铁熔浆发生硫化作用时,将会导致硫化物与硅酸岩熔浆的不混融,从而形成矿浆,据此,金川含铂铜镍矿石不是矿     

Timing of Proterozoic magmatism in the Sunsas belt,Bolivian Precambrian Shield,SW Amazonian Craton

We present new U-Pb zircon and monazite ages from the Sunsas belt granitic magmatism in Bolivia,SW Amazonian Craton.The geochronological results revealed four major magmatic events recorded along the Sunsas belt domains.The older igneous event formed a granitic basement coeval to the Rio Apa Terrane(1.95-1.85 Ga)in the southern domain.The second magmatic episode is represented by 1.68 Ga granites associated to the Paraguá Terrane(1.69-1.66 Ga)in the northern domain.The 1.37-1.34 Ga granites related to San Ignacio orogeny represent the third and more pervasive magmatic event,recorded throughout the Sunsas belt.Moreover,magmatic ages of～1.42 Ga revealed that the granitogenesis asso-ciated to the Santa Helena orogeny also affected the Sunsas belt,indicating that it was not restricted to the Jauru Terrane.Lastly,the 1.10-1.04 Ga youngest magmatism was developed during the Sunsas oro-geny and represents the final magmatic evolution related to Rodinia assembly.Likewise,the 1.95-1.85 and 1.68 Ga inherited zircon cores obtained in the～1.3 Ga and 1.0 Ga granite samples suggest strong par-tial melting of the Paleoproterozoic sources.The 1079±14 Ma and 1018±6 Ma monazite crystallization ages can be correlated to the collisional tectono-thermal event of the Sunsas orogeny,associated to reac-tions of medium-to high-grade metamorphism.Thus,the Sunsas belt was built by heterogeneous 1.95-1.85 Ga and 1.68 Ga crustal fragments that were reworked at 1.37-1.34 Ga and 1.10-1.04 Ga related to orogenic collages.Furthermore,the 1.01 Ga monazite age suggests that granites previously dated by zir-con can bear evidence of a younger thermal history.Therefore,the geochronological evolution of the Sunsas belt may have been more complex than previously thought.