长江三角洲城市带扩展对区域温度变化的影响   总被引：7，自引：0，他引：7  

杜银  谢志清  曾燕  施雅风  武金岗 《地理学报(英文版)》2007,17(4):387-398

Based on non-radiance-calibrated DMSP/OLS nighttime light imagery from 1992 to 2003, urban land area statistical data, meteorological data and land surface temperature data retrieved by MODIS and NOAA/AVHRR data, the influence of urbanization on regional cli- matic trend of temperature in the Yangtze River Delta (YRD) was analyzed. Conclusions are as follows: 1) There is a significant urbanization process from 1992 to 2003 in the YRD. Four city clusters of Nanjing–Zhenjiang–Yangzhou, Suzhou–Wuxi–Changzhou, Shanghai and Hangzhou Bay form a zigzag city belt. The increase rate of annual mean air temperature in city-belt is 0.28–0.44℃/10a from 1991 to 2005, which is far larger than that of non-city-belt. 2) The urban heat island (UHI) effect on regional mean air temperature in different seasons is summer>autumn>spring>winter. 3) The UHI intensity and the urban total population logarithm are creditably correlated. 4) The UHI effect made the regional annual mean air temperature increased 0.072℃ from 1961 to 2005, of which 0.047℃ from 1991 to 2005, and the annual maximum air temperature increased 0.162℃, of which 0.083℃ from 1991 to 2005. All these indicating that the urban expansion in the YRD from 1991 to 2005 may be regarded as a serious climate signal.  相似文献   

大地电场变化的频谱特征   总被引：22，自引：8，他引：14       下载免费PDF全文

叶青  杜学彬  周克昌  李宁  马占虎 《地震学报》2007,29(4):382-390

处理了中国大陆地区嘉峪关、昌黎、崇明、蒙城、兴济、宝坻和阳原等7个台的地电场观测数据,应用最大熵谱方法研究了大地电场日变化、地电暴等谱成分的特征. 结果表明,大地电场日变化主要是12 h的半日波成分最强, 24~25 h的全日波和8 h周期成分次之; 地电暴是在大尺度空间同步发生的,其谱值高于日变化谱值约2～3个数量级,主要以较长周期成分为主. 这一结果初步解释了大地电场变化的主要谱成分的生成机制.   相似文献   

EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts   总被引：1，自引：0，他引：1  

C. Y. Li  Y. Chen  B. Wang  G. P. Ruan  S. W. Feng  G. H. Du  X. L. Kong 《Solar physics》2017,292(6):82

Type-I bursts (i.e. noise storms) are the earliest-known type of solar radio emission at the meter wavelength. They are believed to be excited by non-thermal energetic electrons accelerated in the corona. The underlying dynamic process and exact emission mechanism still remain unresolved. Here, with a combined analysis of extreme ultraviolet (EUV), radio and photospheric magnetic field data of unprecedented quality recorded during a type-I storm on 30 July 2011, we identify a good correlation between the radio bursts and the co-spatial EUV and magnetic activities. The EUV activities manifest themselves as three major brightening stripes above a region adjacent to a compact sunspot, while the magnetic field there presents multiple moving magnetic features (MMFs) with persistent coalescence or cancelation and a morphologically similar three-part distribution. We find that the type-I intensities are correlated with those of the EUV emissions at various wavelengths with a correlation coefficient of 0.7?–?0.8. In addition, in the region between the brightening EUV stripes and the radio sources there appear consistent dynamic motions with a series of bi-directional flows, suggesting ongoing small-scale reconnection there. Mainly based on the induced connection between the magnetic motion at the photosphere and the EUV and radio activities in the corona, we suggest that the observed type-I noise storms and the EUV brightening activities are the consequence of small-scale magnetic reconnection driven by MMFs. This is in support of the original proposal made by Bentley et al. (Solar Phys. 193, 227, 2000).  相似文献   

雷诺数对圆形渐缩喷嘴湍流射流的影响   总被引：2，自引：0，他引：2  

杜诚  徐敏义  米建春 《海洋学报》2010,32(9):6331-6338

The present study systematically investigates by experiment the influence of Reynolds number (Re) on a turbulent jet issuing from a smoothly-contracting round nozzle. Measurements were performed for seven Reynolds numbers varying from Re = 4,050 to Re = 20,100 using single hot-wire anemometry and over an axial distance of 30 nozzle exit diameters. Although all the exit velocity profiles are of "top-hat" shape, these measurements reveal significant dependence on Re of the exit and downstream flows. The effect of Re on both the mean and turbulent fields is substantial for Re ＜ 10,000 and becomes weak beyond Re = 10,000. The length of the jet’s potential core and the far-field rates of decay and spread all depend significantly on Re.  相似文献   

Role of buffer layer in electronic structures of iron phthalocyanine molecules on Au(111)     

孙家涛  潘理达  胡昊  杜世萱  高鸿钧 《海洋学报(英文版)》2010,29(9)

We investigate the electronic structures of one and two monolayer iron phthalocyanine (FePc) molecules on Au(111) surfaces. The first monolayer FePc is lying flat on the Au(111) substrate, and the second monolayer FePc is tilted at ～15° relative to the substrate plane along the nearest neighbour [101^-] direction with a lobe downward to the central hole of the unit cell in the first layer. The structural information obtained by first-principles calculations is in agreement with the experiment results. Furthermore, it is demonstrated that the electronic structures of FePc molecules in one-monolayer FePc/Au(111) system are perturbed significantly, while the electronic structures of FePc molecules in the second monolayer in two-monolayer FePc/Au(111) system remain almost unchanged due to the screening of the buffer layer on Au(111).  相似文献   

The anomalous radiation force of light on a left-handed material     

易煦农  刘劲松  陈欢  杜秋姣 《海洋学报(英文版)》2010,29(11)

This paper derives the force of the electromagnetic radiation on left-handed materials (LHMs) by a direct application of the Lorentz law of classical electrodynamics. The expressions of radiation force are given for TE-polarised and TM-polarised fields. The numerical results demonstrate that electromagnetic waves exert an inverse lateral radiation force on each edge of the beams, that is, the lateral pressure is expansive for TE-polarised beams and compressive for TM-polarised beams. The investigation of the radiation force will provide insights into the fundamental properties of LHMs and will provide to better understanding of the interaction of light with LHMs.  相似文献   

Modelling the effect of wave overtopping on nearshore hydrodynamics and morphodynamics around shore-parallel breakwaters     

Yanliang Du  Shunqi Pan  Yongping Chen 《Coastal Engineering》2010

Wave overtopping nearshore coastal structures, such as shore-parallel breakwaters, can significantly alter the current circulation and sediment transport patterns around the structures, which in turn affects the formation of tombolos and salients in the nearshore area. This paper describes the implementation of a wave overtopping module into an existing depth-averaged coastal morphological mode: COAST2D and model applications to investigate the effect of wave overtopping on the hydrodynamics and morphodynamics around a group of shore-parallel breakwaters. The hydrodynamic aspects of the model were validated against a series of laboratory conditions. The model was then applied to a study site at Sea Palling, Norfolk, UK, where 9 shore-parallel segmented breakwaters including 4 surface-piercing and 5 low-crested breakwaters are present, for the storm conditions in Nov 2006. The model results were compared with laboratory data and field measurements, showing a good agreement on both hydrodynamics and morphological changes. Further analysis of wave overtopping effect on the nearshore hydrodynamics and morphodynamics reveals that wave overtopping has significant impacts on the nearshore circulation, sediment transport and the resulting morphological changes within such a complex breakwater scheme under the storm and macro-tide conditions. The results indicate the importance of including the wave overtopping in modelling nearshore morphodynamics with the presence of coastal structures.  相似文献   

许昌市供电量与气象要素相关分析     

杜彩月  张国平  刘玉巧  徐景花 《气象与环境科学》2007,30(4):85-87

利用20052006年许昌市逐日供电量和气温、降水、相对湿度等气象要素资料,分析了供电量和这些气象要素之间的相关关系,结果表明,温度为影响本地用电量的主要气象因子,特别是夏季用电量对气温变化的反应更加敏感.  相似文献   

皖浙赣断裂带的界定及其基本特征   总被引：12，自引：0，他引：12  

余心起  江来利  许卫  邱瑞龙  杜建国  戴圣潜 《地学前缘》2007,14(3):102-113

以往文献中及众多研究者所指的“皖浙赣断裂带”实际上包括了不同时代形成的、方向有变化的多组规模巨大的区域性断裂带;最早的断裂带形成于新元古代,最晚的形成于晚中生代。在地壳演化过程中,随着构造应力场的变化,不同时代的断裂带方向变化较大,新元古代晋宁期为北东向,早古生代加里东期为近东西向—北东东向,晚中生代为北北东向;每一期断裂带都有它们自己的大地构造背景和指示意义。文中认为,不同阶段形成的断裂带不能混为一谈。新元古代晋宁期的北东向断裂带南段基本上以赣东北蛇绿混杂岩带为代表,向北东延至皖南伏川断裂带,具有板块(或地体)边界断裂的性质;加里东期以近东西向祁门—歙县断裂带为代表,其西段被后期牵引成北东向,造成两侧的变质基底特征明显不同;二者均不属于皖浙赣断裂带的组成部分。而通常意义上所指的具有区域控岩控矿作用的皖浙赣断裂带,是晚中生代北北东向的赣东北—五城—歙县—绩溪—宁国断裂带,控制了侏罗—白垩纪红色盆地及燕山期岩浆岩的形成和分布,是一条具有控矿作用的重要的构造岩浆岩带。  相似文献   

盆地形成及成矿与地幔流体间的成因联系   总被引：11，自引：0，他引：11  

杜乐天  欧光习 《地学前缘》2007,14(2):215-224

文中共讨论以下5个问题:(1)盆地起源于幔壳溃变和膨隆,后者是地幔流体(超临界态(>375℃)HACONS流体,简称幔汁)上涌、渗入、交代、富化、致熔的产物。地幔流体造成油气盆地深部的高热流、异常超高压、伊利水云母化、硅化和地层有机碳的加氢成油作用。(2)盆地成矿可分两大阶段,先是沉积时的同生成矿;地层沉积后还有众多的后生成矿。两者组成“盆地矿套”(杜乐天,2002)。成矿无论同生还是后生,其分布均受断裂控制,都和地幔流体活动有关。(3)黑色页岩的实质是碳-硅-泥三元岩系,和热液成矿中的碳酸盐-硅质-泥质蚀变三元完全相当。此类岩系中总是有几十种亲壳亲幔亲气元素的特殊富集。奇异的是,石油、油页岩、沥青及砂岩型铀矿彼此有完全类似的继承性元素特殊富集。此等元素群不可能都是来自盆地之外蚀源区岩体的风化。研究证明,相当多的元素是地幔流体携带上来的。(4)盆地地层中广泛发育由地幔流体衍生的热液作用。(5)盆地实质上是气盆,全盆地排气。许多气田是地幔流体排气形成的。沙漠(原地型)和天然气田的共生很值得注意,两者皆源于地球强烈排气,导致地下和大气增温,过度蒸发,不易降雨,长期干旱而形成沙漠。  相似文献