西沙群岛大气中海盐粒子的分布特征   总被引：9，自引：1，他引：9  

吴兑  游积平  关越坚 《热带气象学报》1996,12(2):122-129

分析了在西沙永兴岛观测的Ｃｌ＾－海盐核资料，主要结果有：（１）东北季风期干直径大于２μｍ的Ｃｌ＾－核平均浓度８７８个／Ｌ，平均含盐量１０５．４μｇ／ｍ＾３，其中干直径大于４μｍ的特大核平均为１９０个／Ｌ，最大间观测到干直径５７μｍ的Ｃｌ＾－粒子，均较该地在１９８７年５月西南季风盛行期的观测值高。谱型呈准单调下降的幂函数递减谱。（２）随距海面高度增加海盐粒子浓度与含盐量均有所减小。（３）Ｃｌ＾－粒子  相似文献   

Adakite-like signature of Late Miocene intrusions at the Los Pelambres giant porphyry copper deposit in the Andes of central Chile: metallogenic implications   总被引：7，自引：0，他引：7  

Martin?Reich  Miguel?A.?ParadaEmail author  Carlos?Palacios  Andreas?Dietrich  Frank?Schultz  Bernd?Lehmann 《Mineralium Deposita》2003,38(7):876-885

Adakite-like features are recognized in the Late Miocene (~10 Ma) porphyritic intrusions of the Los Pelambres giant porphyry copper deposit, central Chile (32°S). Located within the southern portion of the flat-slab segment (28–33°S) of the Chilean Andes, the Al- and Na-rich porphyries of Los Pelambres display distinctly higher Sr/Y (~100–300) and La_N/Yb_N (~25–60) ratios than contemporaneous and barren magmatic units (e.g., La Gloria pluton, Cerro Aconcagua volcanic rocks) of the same Andean magmatic belt. Strong fractionation of heavy rare earth elements (HREE), absence of Eu anomalies, high Sr/Y and Zr/Sm and low Nb/Ta ratios suggest melt extraction from a garnet-amphibolite source. The Late-Miocene adakite-like porphyritic intrusions at Los Pelambres formed closely related in time and space to the subduction of the Juan Fernández Ridge (JFR) hotspot chain along the Chilean margin. Current tectonic reconstructions reveal that, at the time of formation of the Los Pelambres rocks, a W-E segment of the JFR started to subduct beneath them, producing a slow-down of a previously rapid southward migration of a NE-ridge—trench collision. These particular tectonic conditions are favorable for the origin of the Los Pelambres porphyry suite by melting of subducting young hotspot rocks under flat-slab conditions. The incorporation of crustal components into the oceanic lithopheric magma source by subduction erosion is evidenced by the Sr-Nd isotope composition of the Los Pelambres rocks different from the MORB signatures of true adakites. A close relationship apparently exists between the origin of this adakite-like magmatism and the source of the mineralization in the Los Pelambres porphyry copper deposit.Editorial handling: R.J. Goldfarb  相似文献   

华南巨型锑矿带的特征及其制约因素   总被引：5，自引：0，他引：5       下载免费PDF全文

刘建明  顾雪祥  刘家军  郑明华 《地球物理学报》1998,41(Z1):207-215

华南巨型锑矿带位于中国南方扬子陆块与华夏陆块的接合过渡地段,锑矿床都产在沉积地层中,具有显著的层控性,常有整合的层状矿体出现,赋矿地层都显示异常高的锑丰度,充分显示了与沉积盆地演化密不可分的内在联系矿石的硫同位素受赋矿地层层位和沉积相的控制,碳同位素特征反映了深部因素与浅部过程的耦合,铅同位素则暗示研究区地层及其中锑矿化的亲缘关系和统一演化历史．锑是一个趋于在地壳浅部富集的中低温热液成矿元素,因此成熟度越高的地壳块段锑的丰度越高,锑矿产出概率也越大．华南巨型锑矿带的形成乃是扬子陆块南缘沉积盆地长期演化的结果,可能与这一岩石圈块段长期以来强烈的物质分异和再循环有关．  相似文献   

The development of the pinnacles (Lena pillars) along Middle Lena (Sakha Republic,Siberia, Russia)     

Márton Veress  Zoltán Zentai  Kálmán Péntek  Ljubov Döbröntei  Ljubov Danilovna Kiprijanova 《Proceedings of the Geologists' Association. Geologists' Association》2014

The study deals with the Lena Pillars (Sakha Republic, Russia, Siberia). The Lena Pillars are pinnacle features which are characteristic on karsts. The importance of these features is that they are extremely large and occur on very large areas. Their occurrence is interesting because they do not appear on tundra karst. We investigated the veneers of cliffs, the fracture density of the building rock, the distribution and dispersion of the fracture directions, direction distribution and dispersion of the giant grikes between the pillars, the layer thickness of the building rock, the size and dispersion of debris. We distinguished pillar types, and then we classified the features on the area of the pillars from a morphogenetical point of view. According to investigations and morphological analyses, the pillars developed from palaeokarsts. During the former karstification grikes and caverns developed close to the surface. These features coalesced into each other. The giant grikes of great size became filled and the pillars were covered. After the cut of the Lena River these features were revealed and became exhumed. Now the pillars are destroyed and continue developing by frost weathering.  相似文献   

Seasonal change in the deep atmosphere of Uranus     

Mark D Hofstadter  Bryan J Butler 《Icarus》2003,165(1):168-180

We present high-resolution radio maps of Uranus, made from data collected in 1994 at wavelengths of 2 and 6 cm, which show large-scale changes occurring deep and rapidly in the troposphere. Brightness features in these maps are significantly different from those observed throughout the 1980's. These differences are not due to the changing viewing geometry, but result from atmospheric changes in the 5 to 50 bar region. All the observations show strong latitudinal variations in absorber abundance and/or temperature, causing the South Pole to appear brighter than lower latitudes. The transition between bright pole and darker latitudes is always near −45°, but between 1989 and 1994 the contrast between the regions increased significantly. This suggests that the large-scale circulation in the upper 50 bars of the uranian Southern Hemisphere changed. Older, disk-averaged microwave observations have suggested that seasonal variability occurs, but these new maps are the first to provide detailed timing and location information which can be used to test dynamical models.  相似文献   

Interpretation of the carbon abundance in Saturn measured by Cassini     

Franck Hersant  Daniel Gautier 《Planetary and Space Science》2008,56(8):1103-1111

Spectral observations of Saturn from the far infrared spectrometer aboard the Cassini spacecraft [Flasar, F.M., et al., 2005. Temperatures, winds, and composition in the Saturnian system. Science 307, 1247-1251] have revealed that the C/H ratio in the planet is in fact about twice higher than previously derived from ground based observations and in agreement with the C/H value derived from Voyager IRIS by Courtin et al. [1984. The composition of Saturn's atmosphere at northern temperate latitudes from Voyager IRIS spectra - NH₃, PH₃, C₂H₂, C₂H₆, CH₃D, CH₄, and the Saturnian D/H isotopic ratio. Astrophys. J. 287, 899-916]. The implications of this measurement are reanalyzed in the present report on the basis that volatiles observed in cometary atmospheres, namely CO₂, CH₄, NH₃ and H₂S may have been trapped as solids in the feeding zone of the planet. CH₄ and H₂S may have been in the form of clathrate hydrates while CO₂ presumably condensed in the cooling solar nebula. Carbon may also have been incorporated in organics. Conditions of temperature and pressure ease the hydratation of NH₃. Such icy grains were included in planetesimals which subsequently collapsed into the hydrogen envelope of the planet, then resulting in C, N and S enrichments with respect to the solar abundance. Our calculations are consistent, within error bars, with observed elemental abundances on Saturn provided that the carbon trapped in planetesimals was mainly in the form of CH₄ clathrate and CO₂ ice (and maybe as organics) while nitrogen was in the form of NH₃ hydrate. Our approach has implications on the possible pattern of noble gases in Saturn, since we predict that contrary to what is observed in Jupiter, Ar and Kr should be in solar abundance while Xe might be strongly oversolar. The only way to verify this scenario is to send a probe making in situ mass spectrometer measurements. Our scenario also predicts that the ¹⁴N/¹⁵N ratio should be somewhat smaller in Saturn than measured in Jupiter by Galileo.  相似文献   

哈大巨型城市带要素集聚程度与生态环境水平关系演变   总被引：1，自引：1，他引：0  

刘艳军  田俊峰  付占辉  刘德刚 《地理科学》2017,37(2):172-180

基于耦合模型和象限图法,从整体和内部分异2个角度对2000~2012年哈大巨型城市带要素集聚程度与生态环境水平演变及其关系进行分析,结果表明：哈大巨型城市带要素集聚程度呈波动上升的演变特征,生态环境则“先波动上升,后缓慢下降”,城市带整体要素集聚程度与生态环境水平间关系趋于协调,产业结构演变、资源消耗水平、经济密度是导致城市带要素集聚程度与生态环境水平协调度提高的主要驱动因子,其中产业结构演变的影响作用更加明显。城市带内部要素集聚的“四城市”格局已经形成,呈现出“核心-边缘”结构,要素集聚程度与生态环境水平可分为高级协调、要素集聚滞后、低级协调、生态环境滞后4种类型。4个区域中心城市要素集聚程度与生态环境水平关系趋向不协调,中心城市周边地区主要向要素集聚滞后型转变,资源型城市和重工业城市要素集聚程度与生态环境水平多表现为低级协调。  相似文献   

哈大巨型城市带空间开发-经济发展-环境演变的耦合分异机制   总被引：4，自引：1，他引：3  

刘艳军  刘德刚  付占辉  于会胜  祝丽媛 《地理科学》2018,38(5):662-671

通过构建空间开发、经济发展、资源环境水平的评价指标体系,引入耦合度概念,并应用变异系数、趋势面分析、回归分析等定量模型研究2000~2014年哈大巨型城市带空间开发-经济发展-环境演变的耦合分异特征及其影响机制,主要得到以下结论：① 2000年以来哈大巨型城市带各城市空间开发-经济发展-环境演变的耦合度均处在不同程度失调状态,且整体表现为“西高东低-南高北低”的空间格局,但耦合度水平总体趋于上升。哈长次区域和辽中南次区域以及哈大巨型城市带整体的耦合度波动性均先升高后下降,总体趋势不断向好;② 政府投入强度是2000年影响哈大巨型城市带各城市耦合度差异的重要作用因素,资本投入强度与科技投入规模是2007年、2014年2个阶段的主导影响因素,且城市发展能级差异与2007年各城市间的耦合度差异表现出一致性;③ 在政府投入强度、科技投入规模、资本投入强度等因素的共同作用下,哈长次区域空间开发-经济发展-环境演变的耦合程度出现空间分异。辽中南次区域耦合度分异的影响因素由人力资本效率和行政等级逐渐演变为以资本投入强度主导。  相似文献   

Cosmic-ray positrons: are there primary sources?     

Stphane Coutu  Steven W. Barwick  James J. Beatty  Amit Bhattacharyya  Chuck R. Bower  Christopher J. Chaput  Georgia A. de Nolfo  Michael A. DuVernois  Allan Labrador  Shawn P. McKee  Dietrich Müller  James A. Musser  Scott L. Nutter  Eric Schneider  Simon P. Swordy  Gregory Tarl  Andrew D. Tomasch  Eric Torbet 《Astroparticle Physics》1999,11(4):208-435

Galactic cosmic rays consist of primary and secondary particles. Primary cosmic rays are thought to be energized by first order Fermi acceleration processes at supernova shock fronts within our Galaxy. The cosmic rays that eventually reach the Earth from this source are mainly protons and atomic nuclei, but also include electrons. Secondary cosmic rays are created in collisions of primary particles with the diffuse interstellar gas. They are relatively rare but carry important information on the Galactic propagation of the primary particles. The secondary component includes a small fraction of antimatter particles, positrons and antiprotons. In addition, positrons and antiprotons may also come from unusual sources and possibly provide insight into new physics. For instance, the annihilation of heavy supersymmetric dark matter particles within the Galactic halo could lead to positrons or antiprotons with distinctive energy signatures. With the High-Energy Antimatter Telescope (HEAT) balloon-borne instrument, we have measured the abundances of positrons and electrons at energies between 1 and 50 GeV. The data suggest that indeed a small additional antimatter component may be present that cannot be explained by a purely secondary production mechanism. Here we describe the signature of the effect and discuss its possible origin.  相似文献   

Volatile element chemistry during accretion of the earth     

《Chemie der Erde / Geochemistry》2020,80(1):125594

We review some issues relevant to volatile element chemistry during accretion of the Earth with an emphasis on historical development of ideas during the past century and on issues we think are important. These ideas and issues include the following: (1) whether or not the Earth accreted hot and the geochemical evidence for high temperatures during its formation, (2) some chemical consequences of the Earth’s formation before dissipation of solar nebular gas, (3) the building blocks of the Earth, (4) the composition of the Earth and its lithophile volatility trend, (5) chemistry of silicate vapor and steam atmospheres during Earth’s formation, (6) vapor - melt partitioning and possible loss of volatile elements, (7) insights from hot rocky extrasolar planets. We include tabulated chemical kinetic data for high-temperature elementary reactions in silicate vapor and steam atmospheres. We finish with a summary of the known and unknown issues along with suggestions for future work.  相似文献