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961.
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   
962.
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   
963.
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   
964.
利用最新古生物、磁性地层年代学资料对鸡西群、龙爪沟群进行了年代地层划分.确定了两群形成时间为早白垩世凡兰吟期-阿尔布中期。同时采用层序地层、盆地形成动力学、事件地层学、盆地湖(海)平面升降曲线与全球海平面升降曲线对比等方法.对两群进行了综合对比.证实两群为同一构造-沉降旋回背景下的等时异相关系。笔者认为龙爪沟群自下而上划分为4个组,即裴德组、七虎林河组、下云山组、朝阳组,其在横向上分别对应鸡西群滴道组、城子河组、穆棱组、东山组。这一研究结果将对进一步讨论黑龙江东部中生代海陆变迁机制、地层、构造格架建立及煤矿预测等具有重要的指示意义。  相似文献   
965.
本文论述了公婆泉盆地下白垩统新民堡群的层序地层特点———层序分布和时代、界面特征和内部构成、沉积相,以及层间氧化带和铀矿化特点。认为该盆地在公婆泉地段具有一定的找铀矿远景,但北骆驼泉地段铀成矿条件不佳,那林疏怀地段不具备铀成矿远景。  相似文献   
966.
伊犁盆地侏罗系水西沟群层序地层学研究   总被引:2,自引:0,他引:2  
伊犁盆地侏罗系水西沟群是一套在基本一致的构造应力和沉积环境下形成的含煤碎屑岩建造,但在这套地层的中部(三工河组)出现了岩性、颜色的突变,并且对应的测井曲线也出现明显的突坎现象。笔者运用层序地层学的观点,从年代地层、岩性、体系域、沉积韵律以及测井曲线解释等5方面对这一现象进行了分析,认为该群中部存在一不整合面(或层序界面),并尝试对水西沟群层序地层进行重新划分。  相似文献   
967.
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   
968.
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   
969.
利用区域地物化资料,采用多元统计方法及GIS空间分析技术,通过对东天山成矿带中黄山铜镍矿床、小热泉子铜锌矿床的地质、地球物理、地球化学特征的分析,对东天山西段进行了有色金属矿床找矿靶区预测。预测结果认为:色尔特能、铜花山—硫磺山、米什沟、马鞍桥、彩华沟是今后找寻大型有色金属矿床的重要靶区。  相似文献   
970.
张国英 《西北地质》2006,39(1):83-88
在1∶25万红宝石幅(K47C002001)图幅中,雀儿山群分布于哈萨克斯坦板块南缘,红石山蛇绿混杂岩带以北地带的双沟山—雀儿山一带,为一套宏观色调为灰绿色中基性、中酸性火山岩及其火山碎屑岩夹碎屑岩和灰岩的岩石组合。碎屑岩及灰岩中含腕足、珊瑚、三叶虫、海百合茎等生物化石。其中:Latonotoechiacf.latana(Barrande)原产于波希来亚地区布拉格期。AcrospirifercobedanusvariusKaplun见于哈萨克斯坦地区下泥盆统中上部和新疆的和布克赛尔组。EoschuchertellaguangxiensisWangetRong原于广西郁江组上部六景段。该群形成于与岛弧有关的滨浅海环境,在区域上可与新疆大南湖组、头苏泉组及和布克赛尔组对比。该群形成时代为早—中泥盆世,年代地层为下—中泥盆统。  相似文献   
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