Concurrent Determination of U‐Pb Age and REE Mass Fractions of Zircon by High Mass Resolution SIMS

A combined geochronological and geochemical investigation for the same domain of zircon provides valuable information on timing and genesis, particularly in the case of multi‐growth metamorphic zircon. A high spatial resolution concurrent analytical method for zircon U‐Pb age and rare earth element content was successfully achieved in this study, using a multi‐collector secondary ion mass spectrometer (SIMS) at a ~ 8 μm diameter scale. Special instrument parameters were employed, including a high mass resolution of approximately 15000 applied to replace the previous energy filter method, and a dynamic multi‐collector mode used to reduce the measurement time to 18 min per analysis. Six zircon reference materials yielded precise and accurate ²⁰⁶Pb/²³⁸U ages, which are comparable to those obtained by the ordinary mono‐collector method, but with 2–3 times higher spatial resolution. All zircon grains measured in this study showed enriched heavy‐REE (HREE) contents consistent with previously reported values determined by LA and solution ICP‐MS methods. The light‐REE (LREE) mass fractions measured using both SIMS and LA‐ICP‐MS methods in this study, although with quite different volume, show consistent results within uncertainties.     

安宁河断裂带北段的最新地面活断层与地震潜在能力研究

从最新地面活断层的不连续性,断层滑动速率以及古地震研究的角度讨论安宁河断裂带北段的地震潜在能力,认为不连续的活断层可能成为各自独立的地震破裂单元,从而决定了地震的潜在能力,其中,野鸡洞破裂段的潜在地震能力最强,可达7级。上次地震至今的平静时间已接近古地震的平均重现间隔,因而具有高度的地震危险性     

基于新测年资料的蓟县运动和燕山早期运动表现探讨:以深圳西部地区及东部大鹏半岛国家地质公园地区为例

近3年来在深圳西部及东部大鹏半岛国家地质公园等地,笔者等参加了地质路线调查研究和取样工作,先后采集了20组岩石同位素定年样品,采用新方法锆石U-Pb定年激光测试法测试,其中获得7个数据集中在1 007～897 Ma,首次发现中-新元古代蓟县纪-青白口纪,并基本可以证实蓟县运动(1 400～1 000 Ma)的存在;对中...     

On the dynamic activity in sheared corridors of large delta spots

In the extraordinarily flare-prolific region of March 1989, NOAA region No. 5395, unusual dynamic activity in the photosphere was observed for the first time inside the large delta spot (Wanget al., 1991). Analyses of two additional large delta spots with sheared penumbral fibrils revealed that what occurred in the March 1989 delta spot is not an isolated case; similar complex dynamic activity was observed in the August and October 1989 delta spots. Both are flare-prolific regions as well, each producing 5 X-class flares. As in the March 1989 case, registered and highly time-compressed white-light movies were made from digital data obtained at Big Bear Solar Observatory. The new evidence confirmed the unusual activity: (1) penumbral motions in the directions of sheared penumbral fibrils near the inversion line as well as elsewhere in the delta complex, and (2) new spots emerging in the midst of penumbral motions. The manner and place of emergence are different from those in ordinary emerging flux regions, and often the spots are without observable opposite polarity flux. It is easy to see how the emergence of new spots in the midst of strong fields as well as the shear motions near the inversion line further enhance the flare productivity of the large delta spot regions. But we have yet to understand the origin of the dynamic activity observed.     

Umbral oscillations and penumbral waves in Hα

We present examples of umbral oscillations observed on Big Bear H filtergram movies and investigate the relation between umbral oscillations and running penumbral waves occurring in the same sunspot. Umbral oscillations near the center of the umbra are probably physically independent of the penumbral waves because the period of these umbral oscillations (150 s) is shorter than the penumbral wave period (270 s) but not a harmonic. We also report dark puffs which emerge from the edge of the umbra and move outward across the penumbra, and which have the same period as the running penumbral waves. We interpret these dark puffs to be the extension of chromospheric umbral oscillations at the edge of the umbra. It is suggested that the dark puffs and the running penumbral waves have a common source: photospheric oscillations just inside the umbra.     

SEPARATION OF JETS FROM COMET HALE-BOPP'S COMA BY WAVELET METHOD

A new multiscale technique, the wavelet transform, is applied to the study of jets of comet. It has the advantage to show the features of jets.     

Intraguild predation by polyps of three scyphozoan jellyfish: Nemopilema nomurai,Aurelia coerulea,and Rhopilema esculentum

Journal of Oceanology and Limnology - Jellyfish blooms occur worldwide and have resulted in serious problems in tourism, fisheries, coastal industries, and the marine ecosystem. The life cycle of...     

新疆北部镁铁-超镁铁质岩的PGE成矿问题

铂族元素(PGE)矿化主要与镁铁-超镁铁杂岩有关,成矿类型主要为岩浆型矿床,这类PGE矿床的形成主要依赖两个条件:一是岩浆中富含PGE;二是具备PGE从岩浆中分离和富集的机制,主要是在岩浆演化过程中硫达到饱和。新疆北部镁铁-超镁铁质杂岩发育,并产有喀拉通克、黄山、黄山东、图拉尔根4个大型铜镍矿床和香山、土墩、葫芦、白石泉等中、小型铜镍矿,以及香山西、尾亚等中型钒钛磁铁矿矿床,但迄今尚未发现成型的PGE矿床。文中通过对PGE矿床的形成机制与镁铁-超镁铁杂岩源区特征研究,探讨了北疆地区PGE矿床的成矿问题。综合分析认为,新疆北部后碰撞镁铁-超镁铁质岩的岩石类型为经过了分离结晶形成的铁质岩石系列,是PGE矿床的有利容矿岩石;矿床的Sr、Nd、Pb、O、Os和S同位素和含矿岩石地球化学特征表明,铜镍硫化物矿床含矿岩浆在岩浆演化和成矿过程中有地壳物质加入并可导致硫化物熔离作用,说明在成矿机制上也存在形成岩浆型PGE矿化的条件。新疆北部PGE矿化微弱的原因可能在于该区广泛发育的亏损型地幔源(具正的εNd值特征),这一亏损型地幔可能部分源于洋壳熔融,与产于后碰撞造山带环境、发育于洋壳或不成熟陆壳基底之上有关,由此决定了原始岩浆为贫PGE的源区,因此不利于PGE的富集成矿。     

泰安市矿产开发监督管理工作的思考

根据泰安市区域矿产开发特点,及时掌握矿山企业开采情况,通过加强采矿登记现场预审查、开展矿山开采督察和采矿权人矿产资源开发利用年查等措施,强化了矿产资源开发过程中的监督管理,维护了正常开采秩序及采矿权人的合法权益。     

江苏夏季气温异常的时空变化特征

利用中国160气象观测站1951-2005 年和江苏省59气象观测站1961-2004年的月平均气温资料, 在分析江苏气温变化的季节-年际变化特征的基础上, 重点分析了江苏夏季气温的年际、年代际变化的时间和空间特征.发现:江苏夏季气温1970s到1990s前期基本上处在一个偏凉期,1960s及1990s中后期以后基本上处在一个偏热期;江苏夏季气温异常存在显著的准6 a、准9 a的年际周期和以16 a为中心的年代际周期;江苏夏季气温趋势自西北向东南呈现正负正的位相分布特点,即江苏西北部和东南部地区夏季气温呈现升高的趋势,其它地区呈现降低的趋势.