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901.
Swept-frequency (1/10 MHz) ionosonde measurements were made at Helston, Cornwall (50°06N, 5°18W) during the total solar eclipse on August 11, 1999. Soundings were made every three minutes. We present a method for estimating the percentage of the ionising solar radiation which remains unobscured at any time during the eclipse by comparing the variation of the ionospheric E-layer with the behaviour of the layer during a control day. Application to the ionosonde date for 11 August, 1999, shows that the flux of solar ionising radiation fell to a minimum of 25±2% of the value before and after the eclipse. For comparison, the same technique was also applied to measurements made during the total solar eclipse of 9 July, 1945, at Sörmjöle (63°68N, 20°20E) and yielded a corresponding minimum of 16 ± 2%. Therefore the method can detect variations in the fraction of solar emissions that originate from the unobscured corona and chromosphere. We discuss the differences between these two eclipses in terms of the nature of the eclipse, short-term fluctuations, the sunspot cycle and the recently-discovered long-term change in the coronal magnetic field.  相似文献   
902.
We report on the development and current capabilities of the ALOMAR Rayleigh/Mie/Raman lidar. This instrument is one of the core instruments of the international ALOMAR facility, located near Andenes in Norway at 69°N and 16°E. The major task of the instrument is to perform advanced studies of the Arctic middle atmosphere over altitudes between about 15 to 90 km on a climatological basis. These studies address questions about the thermal structure of the Arctic middle atmosphere, the dynamical processes acting therein, and of aerosols in the form of stratospheric background aerosol, polar stratospheric clouds, noctilucent clouds, and injected aerosols of volcanic or anthropogenic origin. Furthermore, the lidar is meant to work together with other remote sensing instruments, both ground- and satellite-based, and with balloon- and rocket-borne instruments performing in situ observations. The instrument is basically a twin lidar, using two independent power lasers and two tiltable receiving telescopes. The power lasers are Nd:YAG lasers emitting at wavelengths 1064, 532, and 355 nm and producing 30 pulses per second each. The power lasers are highly stabilized in both their wavelengths and the directions of their laser beams. The laser beams are emitted into the atmosphere fully coaxial with the line-of-sight of the receiving telescopes. The latter use primary mirrors of 1.8 m diameter and are tiltable within 30° off zenith. Their fields-of-view have 180 rad angular diameter. Spectral separation, filtering, and detection of the received photons are made on an optical bench which carries, among a multitude of other optical components, three double Fabry-Perot interferometers (two for 532 and one for 355 nm) and one single Fabry-Perot interferometer (for 1064 nm). A number of separate detector channels also allow registration of photons which are produced by rotational-vibrational and rotational Raman scatter on N2 and N2+O2 molecules, respectively. Currently, up to 36 detector channels simultaneously record the photons collected by the telescopes. The internal and external instrument operations are automated so that this very complex instrument can be operated by a single engineer. Currently the lidar is heavily used for measurements of temperature profiles, of cloud particle properties such as their altitude, particle densities and size distributions, and of stratospheric winds. Due to its very effective spectral and spatial filtering, the lidar has unique capabilities to work in full sunlight. Under these conditions it can measure temperatures up to 65 km altitude and determine particle size distributions of overhead noctilucent clouds. Due to its very high mechanical and optical stability, it can also employed efficiently under marginal weather conditions when data on the middle atmosphere can be collected only through small breaks in the tropospheric cloud layers.  相似文献   
903.
The configuration of Alpine accumulation areas during the last glacial maximum (LGM) has been reconstructed using glacial–geological mapping. The results indicate that the LGM ice surface consisted of at least three major ice domes, all located south of the principal weather divide of the Alps. This implies that the buildup of the main Alpine ice cover during oxygen isotope stage (OIS) 2 was related to precipitation by dominant southerly atmospheric circulation, in contrast to today's prevalent westerly airflow. Such a reorganization of the atmospheric circulation is consistent with a southward displacement of the Oceanic Polar Front in the North Atlantic and of the associated storm track to the south of the Alps. These results, combined with additional paleoclimate records from western and southern Europe, allow an interpretation of the asynchronous evolution of the different European ice caps during the last glaciation. δ18O stages (OIS) 4 and 3 were characterized by location of the Polar Front north of 46°N (Gulf of Biscay). This affected prevailing westerly circulation and, thus, ice buildup in western Scandinavia, the Pyrénées, Vosges, and northern Alps. At the LGM, however, the Polar Front lay at 44°N, causing dominating southerly circulation and reduced precipitation in central and northern Europe.  相似文献   
904.
The spatially distributed soil erosion and sediment delivery model WATEM/SEDEM was used to simulate the impact of riparian vegetated filter strips (RVFSs) on river sediment delivery at different spatial scales. For a field plot with a straight slope, sediment reduction by the RVFSs is comparable to results obtained through experimental set‐ups elsewhere (i.e. >70%). However, at the scale of an entire catchment, sediment reduction is much less (i.e. ±20%) due to (1) overland flow convergence, which reduces the sediment trapping efficiency of an RVFS, and (2) because part of the sediment bypasses the RVFSs through ditches, sewers and road surfaces. These results suggest that, at the catchment scale, RVFSs should be accompanied with other conservation techniques that are more appropriate for reducing river sediment loads, and that also reduce on‐site soil erosion. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   
905.
刘宇  管玉平  林一骅 《地球科学进展》2006,21(11):1185-1192
现代大洋热盐环流的特点之一是北大西洋有深水形成而北太平洋没有,这种不对称性对周边气候产生了重要影响。尽管理论上认为大洋热盐环流可能存在对应不同气候的多平衡态,但北太平洋是否曾有过深水形成已成为目前学术争论的一个热点。简要介绍了最新的热盐环流研究成果,重点分析现代北太平洋无深水形成的原因,其中亚洲季风的水汽输送和低蒸发是两个重要的影响因子。  相似文献   
906.
胶东金矿集区矿石中普遍含金属硫化物和碳酸盐矿物,某些矿床中还见有富含炭质的断裂破碎带.成矿溶液中含有大量的SO4^2-、HCO3^-、CO2和有机质等的含硫和含碳组分.矿石硫同位素组成明显富集重硫,结合胶东金矿主要成矿时期(早白垩世)特殊的地质背景、同期海水硫酸盐δ^34S平均值(约+16‰)及现代海水沿NE-NNE向断裂倒灌情况,笔者认为,硫的主要来源与海水硫的大量补给有关.而根据碳、氧同位素组成特征分析,形成金矿床中方解石的物源有很大一部分来自前寒武系碳酸盐岩.浅表环境下成矿金属元素及硫、碳等物质在热液对流系统中的大规模循环是成矿的关键,SO4^2-与S2^-之间的临界转化是制约成矿金属元素活化-迁移-聚集的重要因素,而含碳组分(CO3^2-、HCO3^-、CO2和有机质)则有利于Au、Cu、Pb、Zn等元素的活化和迁移,含硫和含碳组分的循环及有关的物理化学反应之间有明显的关联性.  相似文献   
907.
油气包裹体己成为油气成藏研究的有力工具,在划分油气运移充注期次、确定油气藏的形成时间、反映油气的成熟度及来源等方面均有重要的应用价值。近年来,利用油气包裹体及其共生的盐水溶液包裹体估算油气藏形成时的pVT条件是油气包裹体研究中的一个新热点,它为更准确地计算油气藏形成的温度一压力条件提供了一种独立的、更准确的技术手段。研究表明,包裹体岩相学和流体体系的热力学研究仍将是今后的发展重点。油气包裹体的pVT模拟技术尚处于初始阶段,两种软件(VTFlinc和FIT)的准确性和精确性虽有待进一步提高,但已经成为今后一个重要的发展方向。  相似文献   
908.
杨昌华  刘星  罗荣生 《云南地质》2006,25(3):286-290
在不到10km^2的范围内,集中发现了滇黔桂金三角地区常见的多种矿化类型:微细粒浸染型金矿、不整合面上金矿(大厂层)、基性火山岩金矿、火山碎屑沉积型金矿、石英脉型金矿、现代河流沉积中的砂金,且存在不同的找矿标志。  相似文献   
909.
天山地区新元古代-早寒武世火山岩地球化学和岩石成因   总被引:1,自引:0,他引:1  
天山地区新元古代-早寒武世玄武质熔岩包括拉斑玄武质和碱性玄武质两个主要岩浆系列,前者是早期(早南华世贝义西组、早震旦世扎摩克提组)喷发的火山岩系的主要组成,后者是晚期(早震旦世苏盖特布拉克组、晚震旦世水泉组、早寒武世西山布拉克组)喷发的火山岩系的主要组成。稀土、微量元素和Sr、Nd同位素特征揭示,这些火山岩均形成于大陆裂谷环境,其源区可能是源于一种似洋岛玄武岩源的软流圈地幔源,并且在岩浆上侵喷发过程中发生了岩石圈的混染。  相似文献   
910.
新疆-甘肃北山金矿南带的成矿流体演化和成矿机制   总被引:1,自引:0,他引:1  
刘伟  潘小菲 《岩石学报》2006,22(1):171-188
北山金矿南带是西北5省区规模最大的金矿带。选择北山南带的新金厂、老金厂和小西弓金矿床,在矿床地质和岩相学研究的基础上,对脉石英的流体包裹体进行了显微温度计和激光拉曼探针气体成分测定;对石英和矿石黄铁矿的包裹体H2O,CO2和CH4进行了H和C同位素组成测定,对石英和黄铁矿分别做了O和S同位素组成测定。3个金矿床的脉石英含有富CO2+CH4、H2O溶液以及H2O-CO2+CH4包裹体。小西弓金矿床流体包裹体的均一化温度主要介于270℃-450℃,一部分H2O溶液包裹体圈闭了高盐度流体(16.43—18.63wt.%NaCl equiv.),大部分H2O溶液包裹体和全部富CO2+CH。包裹体代表了中-低盐度(2.8%-13.6%)流体。新金厂金矿床流体包裹体的均一化温度主要介于210℃-346℃;一部分流体包裹体圈闭了高盐度(10.98%~14%NaCl equiv.)流体,一部分H2O溶液包裹体和绝大多数富CO2+CH4包裹体圈闭了中-低盐度(2.9%-8.81%NaCl equiv.)流体。老金厂金矿床H2O溶液包裹体的均一化温度主要分布于141℃-400℃,含盐度介于1.4%-8.28%,属于中-低盐度流体。进行了大气降水-围岩^18O/^16O、D/H交换反应模拟。小西弓矿床早期硫化物-石英脉金矿成矿流体对应较高的水/岩比(=0.01—0.05),其^18O/^16O和D/H组成更受钾长花岗岩者控制,硫化物的δ^34S值也接近钾长花岗岩的黄铁矿者,指示热液流体围绕着钾长花岗岩的对流淋滤。成矿晚期,围绕着花岗岩侵入体的热液对流崩溃,矿区围岩内发育更大尺度的彼此分离的弥漫性流体渗透淋滤;相应地,小西弓矿床晚期蚀变岩金矿成矿流体的8D值对应低水/岩比(0.005-≈0.01),其δ^18O值变化范围较宽,受当地中元古界变质岩控制,蚀变岩型金矿黄铁矿的δ^34S值也接近中元古界长英质片岩的黄铁矿者。新金厂金矿和老金厂金矿成矿流体的δD值和δ^18O值对应的水/岩值分别介于0.004—0.01和0.007~0.02,与岩浆流体或者下二叠统哲斯群辉绿岩和英安岩围岩具有更密切的关系。新金厂金矿和老金厂金矿黄铁矿样品的δ^34S值介于-2.58‰和-6.32‰,指示S来源于下二叠统哲斯群辉绿岩、英安岩和碳质板岩围岩。3个金矿的石英包裹体CO2(δ^13C=-2.20‰--9.14‰),以及石英和黄铁矿包裹体CH4(δ^13C=013.10‰--27.40‰)不平衡;前者来源于幔源岩浆去气,后者来源于哲斯群碳质板岩或者中元古界长英质片岩中的还原碳。3个金矿黄铁矿包裹体的CO(δ^13C=-10.79‰--23.62‰)主要来源于哲斯群碳质板岩或中元古界长英质片岩中的还原碳,但是,也混合了较少的岩浆CO2。包裹体CO2和CH4δ^13C值的系统变化,也反映了从岩浆侵位和去气、流体对流,到围岩中流体大面积弥漫性渗透淋滤的演化过程。CH4介入成矿流体,导致流体不混溶和金的沉淀。北山金矿南带的形成既不同于典型的造山带型金矿床,也不同于与侵入岩有关的金矿床。我们提出北山金矿南带的成矿模式为:岩浆去气和流体对流、岩石挤压破碎、流体弥漫性渗透淋滤。  相似文献   
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