近十年来渤海湾围填海工程对渤海湾水交换的影响   总被引：2，自引：0，他引：2  

王勇智  吴頔  石洪华  赵晓龙  闫文文 《海洋与湖沼》2015,46(3):471-480

近十年来我国海岸带地区快速城市化,对土地的需求持续高涨,导致沿海地区围海造地现象愈演愈烈,海湾纳潮海域面积持续萎缩,对海湾的水交换带来了较大压力。为此,选取我国海岸带快速城市化的典型区域——渤海湾为例,研究近十年来渤海湾海岸带城市化对渤海湾水交换的影响。基于国际流行的MIKE3水动力模型耦合粒子追踪模块,应用2000年和2010年两个典型年份的渤海湾岸线资料,分别计算了2000年和2010年渤海湾环流系统及其驱动下的水质点运移规律和变化特征。研究将渤海湾划分为8个区块,定量化研究和对比了近十年来由于渤海湾持续围填海导致的海湾水存留时间和不同区块水交换能力的变化。结果表明,随着近十年来渤海湾沿岸快速城市化产生的岸线变化,导致湾内环流涡旋增多,决定湾内水交换的流场结构发生了显著变化,导致各区块的水交换能力和平均水存留时间不仅存在较大差异,而且发生了显著的变化。与2000年相比,2010年天津港、黄骅港和曹妃甸港区海域的平均水存留时间明显增加,水交换率下降,对区域水质的改善十分不利。  相似文献   

冰激直立腿海洋平台疲劳寿命分析   总被引：1，自引：1，他引：0  

张大勇  刘笛  许宁  岳前进  郭龙玮 《海洋工程》2015,33(4):35-44

由于渤海特殊环境条件与油藏分布决定了该海域导管架油气平台属于典型的柔性抗冰结构。多年现场观测发现,该类结构存在显著的冰激振动现象。冰振不仅能激起较大的甲板加速度响应,还会引起明显的导管架管节点交变应力。在结构设计与安全保障中进行疲劳分析及寿命估计是必要的。对于直立腿抗冰结构,精确的冰激疲劳寿命计算方法还不成熟。基于多年的现场监测,首先分析了冰与直立腿抗冰结构相互作用过程;其次,提出了冰激直立腿平台的疲劳寿命分析流程;最后,选取渤海某典型直立腿平台,利用ANSYS数值模拟,对比了稳态冰力和随机冰力下结构的疲劳损伤,进而计算出疲劳寿命。本研究为寒区柔性结构抗冰设计与安全保障提供了理论基础。  相似文献   

基于简译的高分辨率卫星影像信息提取研究     

杨昊  杨壮  孙迪 《测绘与空间地理信息》2021,44(z1):168-170,176

利用简译遥感信息提取软件,以资源三号高分辨率卫星影像为数据源,选取老挝首都万象市为研究区,采用分层信息提取思想,在道路、建筑等地表覆盖要素人工提取结果的基础上,对未分类地物(水田、旱地、林地、工矿用地),利用最小距离算法和深度学习算法进行信息提取研究.研究结果表明,基于最小距离算法的总体分类精度为85.7％,Kappa系数为0.8165;基于深度学习算法的总体分类精度为89.29％,Kappa系数为0.8634,都可以达到很好的智能化提取效果.  相似文献   

全球变暖减缓背景下欧亚秋冬温度变化特征和原因   总被引：3，自引：2，他引：1  

王迪  何金海  祁莉  栾健  蔡波 《气象科学》2015,35(5):534-542

采用气候序列变化趋势诊断和一元线性回归等分析法,研究和讨论了2000-2012年和1976-1999年两种年代际背景下全球陆地不同区域的年平均地表温度的变化特征。发现欧亚大陆中高纬度地区是对全球变暖减缓贡献最大的区域。且该地区在2000年以来秋季年代际增温,而冬季年代际降温。从同期大气环流的配置来看,在对流层低层,秋季西伯利亚高气压年代际减弱,而冬季西伯利亚高气压年代际增强。在对流层中高层,秋季从西欧至东北亚为"高-低-高"的高度场异常分布,纬向环流加强,经向环流减弱,而冬季极地与贝加尔湖地区的高度场呈偶极型分布,东亚大槽加深,经向环流加强。进一步研究发现,超前一个季节的喀拉海附近的海冰与欧亚中高纬度秋冬两季温度的年代际变率有着密切的联系。一方面,夏季(秋季)海冰减少影响秋季(冬季)中高纬度大气环流;另一方面,夏季(秋季)海冰减少,使得秋季(冬季)从北极至中高纬度大陆的对流层低层水汽含量增加(减少),大气逆辐射增强(减弱)导致秋季(冬季)增温(降温)。  相似文献   

Optimal two-impulse rendezvous using constrained multiple-revolution Lambert solutions     

Gang Zhang  Di Zhou  Daniele Mortari 《Celestial Mechanics and Dynamical Astronomy》2011,110(4):305-317

A solution to the fixed-time minimum-fuel two-impulse rendezvous problem for the general non-coplanar elliptical orbits is provided. The optimal transfer orbit is obtained using the constrained multiple-revolution Lambert solution. Constraints consist of lower bound for perigee altitude and upper bound for apogee altitude. The optimal time-free two-impulse transfer problem between two fixed endpoints implies finding the roots of an eighth order polynomial, which is done using a numerical iterative technique. The set of feasible solutions is determined by using the constraints conditions to solve for the short-path and long-path orbits semimajor axis ranges. Then, by comparing the optimal time-free solution with the feasible solutions, the optimal semimajor axis for the two fixed-endpoints transfer is identified. Based on the proposed solution procedure for the optimal two fixed-endpoints transfer, a contour of the minimum cost for different initial and final coasting parameters is obtained. Finally, a numerical optimization algorithm (e.g., evolutionary algorithm) can be used to solve this global minimization problem. A numerical example is provided to show how to apply the proposed technique.  相似文献   

POLARIX: a pathfinder mission of X-ray polarimetry     

Enrico Costa  Ronaldo Bellazzini  Gianpiero Tagliaferri  Giorgio Matt  Andrea Argan  Primo Attinà  Luca Baldini  Stefano Basso  Alessandro Brez  Oberto Citterio  Sergio Di Cosimo  Vincenzo Cotroneo  Sergio Fabiani  Marco Feroci  Antonella Ferri  Luca Latronico  Francesco Lazzarotto  Massimo Minuti  Ennio Morelli  Fabio Muleri  Lucio Nicolini  Giovanni Pareschi  Giuseppe Di Persio  Michele Pinchera  Massimiliano Razzano  Luigia Reboa  Alda Rubini  Antonio Maria Salonico  Carmelo Sgro’  Paolo Soffitta  Gloria Spandre  Daniele Spiga  Alessio Trois 《Experimental Astronomy》2010,28(2-3):137-183

Since the birth of X-ray astronomy, spectral, spatial and timing observation improved dramatically, procuring a wealth of information on the majority of the classes of the celestial sources. Polarimetry, instead, remained basically unprobed. X-ray polarimetry promises to provide additional information procuring two new observable quantities, the degree and the angle of polarization. Polarization from celestial X-ray sources may derive from emission mechanisms themselves such as cyclotron, synchrotron and non-thermal bremsstrahlung, from scattering in aspheric accreting plasmas, such as disks, blobs and columns and from the presence of extreme magnetic field by means of vacuum polarization and birefringence. Matter in strong gravity fields and Quantum Gravity effects can be studied by X-ray polarimetry, too. POLARIX is a mission dedicated to X-ray polarimetry. It exploits the polarimetric response of a Gas Pixel Detector, combined with position sensitivity, that, at the focus of a telescope, results in a huge increase of sensitivity. The heart of the detector is an Application-Specific Integrated Circuit (ASIC) chip with 105,600 pixels each one containing a full complete electronic chain to image the track produced by the photoelectron. Three Gas Pixel Detectors are coupled with three X-ray optics which are the heritage of JET-X mission. A filter wheel hosting calibration sources unpolarized and polarized is dedicated to each detector for periodic on-ground and in-flight calibration. POLARIX will measure time resolved X-ray polarization with an angular resolution of about 20 arcsec in a field of view of 15 × 15 arcmin and with an energy resolution of 20% at 6 keV. The Minimum Detectable Polarization is 12% for a source having a flux of 1 mCrab and 10⁵ s of observing time. The satellite will be placed in an equatorial orbit of 505 km of altitude by a Vega launcher. The telemetry down-link station will be Malindi. The pointing of POLARIX satellite will be gyroless and it will perform a double pointing during the earth occultation of one source, so maximizing the scientific return. POLARIX data are for 75% open to the community while 25% + SVP (Science Verification Phase, 1 month of operation) is dedicated to a core program activity open to the contribution of associated scientists. The planned duration of the mission is one year plus three months of commissioning and SVP, suitable to perform most of the basic science within the reach of this instrument. A nice to have idea is to use the same existing mandrels to build two additional telescopes of iridium with carbon coating plus two more detectors. The effective area in this case would be almost doubled.  相似文献   

The role of the equation of state in models of very low-mass stars     

Marcella Di Criscienzo  Paolo Ventura  Francesca D’Antona 《Astrophysics and Space Science》2010,328(1-2):167-169

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湘赣边界鹿井铀矿床流体包裹体及成矿机制          下载免费PDF全文

张笑天  潘家永  夏菲  刘颖  黄迪  赵奇峰  张勇  刘国奇  钟福军 《地球科学》2022,47(1):192-205

位于南岭成矿带南西部的鹿井矿床是华南热液型铀矿的典型代表.为查明其成矿流体来源、性质与演化以及成矿机制,开展了不同成矿阶段石英、萤石及方解石中流体包裹体的显微测温和不同阶段石英的氢?氧同位素分析.矿床地质特征表明成矿过程可划分为(I)粗晶石英+黄铁矿±绿泥石±绢云母、(II)沥青铀矿+硫化物+绿泥石+绢云母+暗灰色微晶...  相似文献   

Spectroscopic analysis (FTIR, Raman) of water in mafic and intermediate glasses and glass inclusions   总被引：1，自引：0，他引：1  

Maxime Mercier  Andrea Di Muro  Nicole Métrich  Olfa Belhadj 《Geochimica et cosmochimica acta》2010,74(19):5641-5656

Micro-Raman spectroscopy, even though a very promising technique, is not still routinely applied to analyse H₂O in silicate glasses. The accuracy of Raman water determinations critically depends on the capability to predict and take into account both the matrix effects (bulk glass composition) and the analytical conditions on band intensities. On the other hand, micro-Fourier transform infrared spectroscopy is commonly used to measure the hydrous absorbing species (e.g., hydroxyl OH⁻ and molecular H₂O) in natural glasses, but requires critical assumptions for the study of crystal-hosted glasses. Here, we quantify for the first time the matrix effect of Raman external calibration procedures for the quantification of the total H₂O content (H₂O_T = OH⁻ + H₂O_m) in natural silicate glasses. The procedures are based on the calibration of either the absolute (external calibration) or scaled (parameterisation) intensity of the 3550 cm⁻¹ band. A total of 67 mafic (basanite, basalt) and intermediate (andesite) glasses hosted in olivines, having between 0.2 and 4.8 wt% of H₂O, was analysed. Our new dataset demonstrates, for given water content, the height (intensity) of Raman H₂O_T band depends on glass density, reflectance and water environment. Hence this matrix effect must be considered in the quantification of H₂O by Raman spectroscopy irrespective of the procedure, whereas the parameterisation mainly helps to predict and verify the self-consistency of the Raman results. In addition, to validate the capability of the micro-Raman to accurately determine the H₂O content of multicomponent aluminosilicate glasses, a subset of 23 glasses was analysed by both micro-Raman and micro-FTIR spectroscopy using the band at 3550 cm⁻¹. We provide new FTIR absorptivity coefficients (ε₃₅₅₀) for basalt (62.80 ± 0.8 L mol⁻¹ cm⁻¹) and basanite (43.96 ± 0.6 L mol⁻¹ cm⁻¹). These values, together with an exhaustive review of literature data, confirm the non-linear decline of the FTIR absorptivity coefficient (ε₃₅₅₀) as the glass depolymerisation increases. We demonstrate the good agreement between micro-FTIR and micro-Raman determination of H₂O in silicate glasses when the matrix effects are properly considered.  相似文献   

硫氰酸钾分光光度法有效提高铀矿石中钼的测定精度   总被引：1，自引：0，他引：1  

王頔  张建梅  汪君  赵建新 《岩矿测试》2010,29(1):83-85

在国标GB/T 14353.9—1993基础上,以氯化亚锡为还原剂,硫氰酸钾为络合剂,用国家一级合成硅酸盐光谱分析标准物质验证,对比不同熔矿方法和不同酸性介质对钼最低检出范围的影响,优化了用硫氰酸钾比色法有效检测铀矿石中含量≥10.0μg/g钼的实验方法。数据结果稳定可靠,步骤简单,测得钼的最低检出限可降低至10.0μg/g。方法的测定值与等离子体发射光谱的分析结果相符,可满足实验室内铀矿石批量检测的要求。  相似文献