翼龙重建：方法论的一个研究例子

Reconstructions of fossil animals are widespread and often very high profile, yet many of these reconstructions exhibit low standards of scientific accuracy.     

OBITUARY NOTE ON MR.S.W.WANG

The untimely death of Mr.S.W.Wang on Feb.10th 1936 iscertainly a serious loss to the Chinese geology.Although his name is notso well known as others in the geological circle,Mr.Wang has indeedmade remarkable contribution to the study of Chinese crystals and     

Diagnosis of trace metal contamination in sediments: the example of Ensenada and El Sauzal, two harbors in Baja California, Mexico

Total metal concentrations in sediments from within Ensenada and El Sauzal Harbors are generally higher than at the mouths. Grain-size analyses suggested that this enrichment could be due to the presence of fine-grained sediments in the inner part of the harbors rather than to anthropogenic perturbations. The (Me/Al)(sample) ratios for Pb, Co, Ni and Fe were significantly higher for Ensenada Harbor relative to El Sauzal Harbor, whereas the ratios for Cd, Mn, Zn and Cu were statistically equivalent for both harbors. Calculated enrichment factors [EF(Me)=(Me/Al)(sample)/(Me/Al)(shale)] indicated that the metals showing slight enrichment were those associated with anthropogenic contamination (Pb, Zn), or probably related to primary productivity in the water column (Cd, Co). The levels of most of the metals were not greatly enriched, a consideration that is of the utmost importance when contamination issues are at stake.     

云南哈播斑岩型铜（ 钼 金）矿床地质与成矿背景研究

哈播斑岩铜(-钼-金)矿床位于哀牢山-红河新生代成矿带南端西侧,是近年来新发现的一个斑岩型矿床.矿区内出露的哈播侵入体具有多期侵入的特征,花岗岩依次侵入的序列为坪山花岗岩、三道班花岗岩、阿树花岗岩、哈播南山花岗岩(37.3 Ma),随后有4期斑岩侵入到哈播南山花岗岩中,依次为黑云母钾长石斑岩、石英钾长石斑岩、石英二长斑岩和晚期黑云母钾长石斑岩岩脉.采用LA-ICP-MS锆石U-Pb年龄法测定黑云母钾长石斑岩和石英二长斑岩的加权平均年龄分别为36.20±0.20 Ma和36.19±0.22 Ma,哈播南山花岗岩和4期斑岩具有相似的岩石地球化学特征,都有富钾、高氧化态和类似岛弧花岗岩的岩石地球化学特征,可能具有相同的来源.辉钼矿Re-Os年龄显示,哈播矿床的成矿年龄为35.47±0.16 Ma.相似的成岩-成矿年龄暗示哈播矿床成岩和成矿作用是一个连续的岩浆-热液过程,与玉龙斑岩铜矿相似.基于哈播矿床的岩石学、地球化学特点,结合前人关于青藏高原东部斑岩铜矿的研究成果,我们认为哈播斑岩矿床可能为藏东富碱斑岩带向东南的延伸,与玉龙斑岩铜矿带具有相似的成因,为哀牢山-红河新生代成矿带的重要组成部分,是晚碰撞构造转换背景下的重要产物.     

OBSERVATIONS ON THE QUATERNARY GEOLOGY OF THE LADAKH RANGE, NORTHWEST INDIAN HIMALAYA

OBSERVATIONS ON THE QUATERNARY GEOLOGY OF THE LADAKH RANGE, NORTHWEST INDIAN HIMALAYA     

黑龙江嘉荫地区白垩纪-第三纪界线初步观察

本文报道了黑龙江嘉荫白山头地区一条新的地层剖面及其K／T界线的初步研究。新命名的“白山头段”代表乌云组下部的早古新世地层,含以Tiliaephyllum tsagajanicum等为代表的达宁早期植物化石。在白山头剖面上,作者发现可能为白垩纪末期的凝灰岩。结合与俄罗斯布列亚盆地含K／T界线的查加扬群标准剖面的对比,推测嘉荫地区的K／T界线可能位于白山头段底部与上述凝灰岩之上的一层炭质泥岩之间。     

Actually achieving marine sustainability demands a radical re-think in approach, not 'more of the same'

The UK is committed to meeting a series of ‘high-level marine objectives’ which are required to satisfy national obligations and to meet international commitments for the marine environment. There are more than 16 such international high-level policy driven obligations and commitments, together with more than 18 European and more than 12 of national origin. In the UK, there is an assumption that the current and planned monitoring will provide evidence to demonstrate achievement against these high-level objectives.     

8.4 ka以来纳木错湖芯介形类组合的环境变化意义

对青藏高原中南部纳木错长332cm的NMLC1孔湖芯研究发现,沉积物的介形类动物群计有6属15种。介形类属种生态特征和组合变化分析表明这些介形类对环境条件具有敏感性,其组合能够很好地反映过去环境变化的特征。结果表明,8．4ka以来具有三个不同的环境变化时期：早期在8400～6800aBP,湖泊由浅向深发展,环境具有相对冷湿的特征：中期在6800～2500aBP,湖泊深度逐渐加大,环境经历了暖湿-冷湿-冷干的变化．其中由冷湿向冷干的转化奠定了纳木错现今环境条件的基础：晚期在2500--9aBP,湖泊深度继续增加,这个时期的较早阶段,继续保持了前一时期的冷干特点,但湖水盐度可能开始增加．较晚阶段的冷干化加剧,陆面流水的活跃性大大降低。研究发现,纳木错NMLC1钻孔介形类黑色壳体的高峰值与介形类的最大生产量相一致,并且与沉积水动力条件增强相适应．指示了这些黑壳的产生与介形类的大量繁殖处于同一阶段．并且主要为异地搬运为主。钻孔中出现大量Candona幼虫壳体．其原因可能与沉积环境的水动力条件迅速改变有关。     

On the Radii of Close-in Giant Planets

The recent discovery that the close-in extrasolar giant planet HD 209458b transits its star has provided a first-of-its-kind measurement of the planet's radius and mass. In addition, there is a provocative detection of the light reflected off of the giant planet tau Bootis b. Including the effects of stellar irradiation, we estimate the general behavior of radius/age trajectories for such planets and interpret the large measured radii of HD 209458b and tau Boo b in that context. We find that HD 209458b must be a hydrogen-rich gas giant. Furthermore, the large radius of a close-in gas giant is not due to the thermal expansion of its atmosphere but to the high residual entropy that remains throughout its bulk by dint of its early proximity to a luminous primary. The large stellar flux does not inflate the planet but retards its otherwise inexorable contraction from a more extended configuration at birth. This implies either that such a planet was formed near its current orbital distance or that it migrated in from larger distances (>/=0.5 AU), no later than a few times 107 yr of birth.     

百万分之一中国地質图的編图方法問題和要求

我們知识的每个領域在其一定的发展阶段上都要經历一个实际资料极为丰富的时朋,把这些資料按照严整的科学体系加以总结就是更新、更大的跃进基础。中国人民从三大敌人的压迫下解放出来以后在国民經济、科学各个方面,尤其是地质方面实現了一个