Zn-Al-rich chlorite in interleaved phyllosilicate grains from the low-temperature metamorphic Ordovician terrane of Iglesiente,south-west Sardinia,Italy     

Gabriele Cruciani  Marcello Franceschelli  Stefano Battaglia  Sandro Pasci  Mariano Puxeddu 《Mineralogy and Petrology》2015,109(6):713-718

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The transition between ‘orogenic’ and ‘anorogenic’ magmatism in the western Mediterranean area: the Middle Miocene volcanic rocks of Isola del Toro (SW Sardinia,Italy)     

Michele Lustrino  Vincenzo Morra  Lorenzo Fedele  Marcello Serracino 《地学学报》2007,19(2):148-159

The Isola del Toro is a small island (∼1 km²) about 5 nautical miles SW of Sardinia entirely made up of mildly alkaline sodic evolved rocks (benmoreites and trachytes) related to each other by fractionation processes. ⁴⁰Ar/³⁹Ar dating of an anorthoclase mineral separate from a trachyte gave an age of 11.83 ± 0.10 Ma. This age estimate falls within an interval previously considered a‐magmatic in Sardinia. The results of this study shift the beginning of the Middle Miocene–Quaternary anorogenic volcanism of Sardinia back to the Late Serravalian. The transition between orogenic and anorogenic activity in Sardinia is markedly different from that recorded in the rest of the circum‐Mediterranean area, where this transition is much more gradual, both in time and in terms of magma composition. On the other hand, the transition between orogenic and anorogenic magmatism in Sardinia is rather sharp and lacks hybrid compositions. The Isola del Toro volcanic rocks represent the first anorogenic products produced during the opening of the western Mediterranean Sea.  相似文献   

塔里木河流域2004年"四源一干"河川径流情势及输水运行分析   总被引：14，自引：9，他引：5  

阿迪力·艾则孜  王建文  张建岗  毛炜峄  张丽萍  沈永平  王顺德  王刚 《冰川冻土》2006,28(6):931-940

2004年塔里木河流域平原的年平均气温特高,山区偏高.平原与山区年降水量均正常略偏多,流域内春夏季0℃层高度偏低.2004年塔里木河四条源流出山口天然径流量224.0×108m3,属平水年.天山南坡的河流水量偏丰,阿克苏河偏多15.9%,为丰水年;开都河-孔雀河偏多4.2%,为平略偏丰水年.而喀喇昆仑山及昆仑山北坡的河流水量均少于多年均值,如叶尔羌河偏少10.8%,为偏枯水年;和田河偏少17.9%,为枯水年.四条源流阿克苏河、和田河、叶尔羌河、开都河-孔雀河入塔里木河总水量为27.02×108m3,占四条源流出山口天然径流总量的12.1%,叶尔羌河全年无水输入塔里木河.2004年塔里木河干流上游段阿拉尔-英巴扎耗水量为19.19×108m3,是干流最大的耗水区段;中游段英巴扎-恰拉耗水量为7.530×108m3,为治理前的30.3%,是输水堤工程竣工和加强管理的效益.2004年4月22日至6月25日,实施了第6次从博斯腾湖向塔里木河下游应急输水,历时65 d从博斯腾湖调出水量1.600×108m3,大西海子水库泄洪闸向下游输水量1.020×108m3,水头再次到达台特玛湖,多年来的调水已使下游河段两岸生态环境有了明显改善.  相似文献   

昆仑山北麓克里雅绿洲生态服务价值对土地利用变化的响应   总被引：2，自引：0，他引：2  

麦麦提吐尔逊·艾则孜  海米提·依米提  迪拉娜·尼加提  魏彬 《地理科学》2012,(9):1148-1154

基于1991、2002与2008年卫星遥感资料,采用中国陆地生态系统的服务价值测算方法,分析克里雅绿洲土地利用变化对生态系统服务价值与结构的影响。研究表明:①研究区生态服务价值从1991年的144 224.8万元降到2008年的128 716.3万元,生态服务价值损失10.8%,每年净损失生态服务价值达24.2元/hm2。生态服务总价值的减少主要是由湿地、水域总面积的减少而导致的;②研究区各生态服务功能对区域总生态服务价值贡献率由高到低依次为:废物处理、土壤形成、生物多样性保护、水源涵养、气候调价、气体调价、食物生产、娱乐休闲和原材料;③研究区生态服务价值对生态服务功能指数缺乏弹性。  相似文献   

Satellite kinematics – II. The halo mass–luminosity relation of central galaxies in SDSS     

Surhud More †  Frank C. van den Bosch  Marcello Cacciato  H. J. Mo  Xiaohu Yang  Ran Li 《Monthly notices of the Royal Astronomical Society》2009,392(2):801-816

The kinematics of satellite galaxies reflect the masses of the extended dark matter haloes in which they orbit, and thus shed light on the mass–luminosity relation (MLR) of their corresponding central galaxies. In this paper, we select a large sample of centrals and satellites from the Sloan Digital Sky Survey and measure the kinematics (velocity dispersions) of the satellite galaxies as a function of the r -band luminosity of the central galaxies. Using the analytical framework presented in More, van den Bosch & Cacciato, we use these data to infer both the mean and the scatter of the MLR of central galaxies, carefully taking account of selection effects and biases introduced by the stacking procedure. As expected, brighter centrals on average reside in more massive haloes. In addition, we find that the scatter in halo masses for centrals of a given luminosity,  σ_{log  M}   , also increases with increasing luminosity. As we demonstrate, this is consistent with  σ_{log  L}   , which reflects the scatter in the conditional probability function   P ( L _c| M )  , being independent of halo mass. Our analysis of the satellite kinematics yields  σ_{log  L} = 0.16  ±  0.04  , in excellent agreement with constraints from clustering and group catalogues, and with predictions from a semi-analytical model of galaxy formation. We thus conclude that the amount of stochasticity in galaxy formation, which is characterized by  σ_{log  L}   , is well constrained, independent of halo mass and in a good agreement with current models of galaxy formation.  相似文献   

Physical properties of (2) Pallas     

Benoît Carry  Christophe Dumas  Jérôme Berthier  Stéphane Erard  Jack D. Drummond  Marcello Fulchignoni 《Icarus》2010,205(2):460-472

Ground-based high angular-resolution images of asteroid (2) Pallas at near-infrared wavelengths have been used to determine its physical properties (shape, dimensions, spatial orientation and albedo distribution).We acquired and analyzed adaptive optics (AO) J/H/K-band observations from Keck II and the Very Large Telescope taken during four Pallas oppositions between 2003 and 2007, with spatial resolution spanning 32-88 km (image scales 13-20 km/pixel). We improve our determination of the size, shape, and pole by a novel method that combines our AO data with 51 visual light-curves spanning 34 years of observations as well as archived occultation data.The shape model of Pallas derived here reproduces well both the projected shape of Pallas on the sky (average deviation of edge profile of 0.4 pixel) and light-curve behavior (average deviation of 0.019 mag) at all the epochs considered. We resolved the pole ambiguity and found the spin-vector coordinates to be within 5° of [longitude, latitude] = [30°, −16°] in the Ecliptic J2000.0 reference frame, indicating a high obliquity of about 84°, leading to high seasonal contrast. The best triaxial-ellipsoid fit returns ellipsoidal radii of , and . From the mass of Pallas determined by gravitational perturbation on other minor bodies , [Michalak, G., 2000. Astron. Astrophys. 360, 363-374], we derive a density of significantly different from the density of C-type (1) Ceres of [Carry, B., Dumas, C., Fulchignoni, M., Merline, W.J., Berthier, J., Hestroffer, D., Fusco, T., Tamblyn, P., 2008. Astron. Astrophys. 478 (4), 235-244]. Considering the spectral similarities of Pallas and Ceres at visible and near-infrared wavelengths, this may point to fundamental differences in the interior composition or structure of these two bodies.We define a planetocentric longitude system for Pallas, following IAU guidelines. We also present the first albedo maps of Pallas covering ∼80% of the surface in K-band. These maps reveal features with diameters in the 70-180 km range and an albedo contrast of about 6% with respect to the mean surface albedo.  相似文献   

An integrated evaluation of thirteen modelling solutions for the generation of hourly values of air relative humidity     

Simone Bregaglio  Marcello Donatelli  Roberto Confalonieri  Marco Acutis  Simone Orlandini 《Theoretical and Applied Climatology》2010,102(3-4):429-438

The availability of hourly air relative humidity (HARH) data is a key requirement for the estimation of epidemic dynamics of plant fungal pathogens, in particular for the simulation of both the germination of the spores and the infection process. Most of the existing epidemic forecasting models require these data as input directly or indirectly, in the latter case for the estimation of leaf wetness duration. In many cases, HARH must be generated because it is not available in historical series and when there is the need to simulate epidemics either on a wide scale or with different climate scenarios. Thirteen modelling solutions (MS) for the generation of this variable were evaluated, with different input requirements and alternative approaches, on a large dataset including several sites and years. A composite indicator was developed using fuzzy logic to compare and to evaluate the performances of the models. The indicator consists of four modules: Accuracy, Correlation, Pattern and Robustness. Results showed that when available, daily maximum and minimum air relative humidity data substantially improved the estimation of HARH. When such data are not available, the choice of the MS is crucial, given the difference in predicting skills obtained during the analysis, which allowed a clear detection of the best performing MS. This study represents the first step of the creation of a robust modelling chain coupling the MS for the generation of HARH and disease forecasting models, including the systematic validation of each step of the simulation.  相似文献   

Increasing the detail of European land use/cover data by combining heterogeneous data sets     

Konštantín Rosina  Filipe Batista e Silva  Pilar Vizcaino  Mario Marín Herrera  Sérgio Freire  Marcello Schiavina 《International Journal of Digital Earth》2020,13(5):602-626

ABSTRACT

Data on land use and land cover (LULC) are a vital input for policy-relevant research, such as modelling of the human population, socioeconomic activities, transportation, environment, and their interactions. In Europe, CORINE Land Cover has been the only data set covering the entire continent consistently, but with rather limited spatial detail. Other data sets have provided much better detail, but either have covered only a fraction of Europe (e.g. Urban Atlas) or have been thematically restricted (e.g. Copernicus High Resolution Layers). In this study, we processed and combined diverse LULC data to create a harmonised, ready-to-use map covering 41 countries. By doing so, we increased the spatial detail (from 25 to one hectare) and the thematic detail (by seven additional LULC classes) compared to the CORINE Land Cover. Importantly, we decomposed the class ‘Industrial and commercial units’ into ‘Production facilities’, ‘Commercial/service facilities’ and ‘Public facilities’ using machine learning to exploit a large database of points of interest. The overall accuracy of this thematic breakdown was 74%, despite the confusion between the production and commercial land uses, often attributable to noisy training data or mixed land uses. Lessons learnt from this exercise are discussed, and further research direction is proposed.  相似文献   

Diesel oil and PCB-degrading psychrotrophic bacteria isolated from Antarctic seawaters (Terra Nova Bay, Ross Sea)   总被引：2，自引：0，他引：2  

Maria De  Domenico  Angelina Lo Giudice  Luigi Michaud  Marcello Saitta  Vivia Bruni 《Polar research》2004,23(2):141-146

Fifty-seven Antarctic marine bacteria were examined for their ability to degrade commercial diesel oil as the sole organic substrate at both 4 °C and 20 °C. Based on the preliminary screening, two isolates (B11 and B15) with high capacity to degrade diesel oil were selected and their biodegradation efficiency was quantified by gas chromatographic analysis. As expected for psychrotrophs, diesel oil biodegradation was slower at 4 °C than at 20 °C. The two strains also mineralized the C₂₈ n-paraffin octacosane at 20 °C and polychlorinated biphenyls (PCBs) at 4 °C and 20 °C.  相似文献   

IGCP440"罗迪尼亚超大陆汇聚与裂解"项目2003年度工作进展   总被引：2，自引：0，他引：2  

S.彼萨列夫斯基 《世界地质》2004,23(2):118-122

借助于最新的地质、同位素年代学、地球化学和航空地球物理资料,对全球各地原属于罗迪尼亚大陆组成单元的构造环境、地质事件特征及其演化历史进行了探讨,并提出一些新见解和成因模式.认为东欧克拉通在1.7～0.9Ga有复杂的演化历史一个新的劳仑古陆和西伯利亚的重建发生在1 050～1 000Ma;中、新元古代南美洲造山拼贴的岩石构造历程构成南美陆台的西部边界非洲克拉通是古元古代/太古宙陆块汇聚收敛的结果;东南极的一部分在中元古时期附属于非洲南部;印度西北的新元古代长英质岩浆事件构成了罗迪尼亚大陆的西部边缘;前格林威尔时期的劳仑古陆已被确定为古元古代末期的一个主要大陆;在罗迪尼亚大陆中,华南可能位于劳仑古陆南部和澳大利亚东部之间;塔里木克拉通和扬子克拉通相连接或邻近.据此检验了关于Pisarevsky提出的罗迪尼亚超大陆汇聚和裂解的新模式.新模式提出初始裂解是沿着劳仑古陆的西部边缘,与大西洋北部相类似.同时认为一些大陆(印度、刚果/圣·弗朗西斯科)可能不是罗迪尼亚超大陆的组成部分.  相似文献