海水中液-固界面的台阶型动力学曲线 Ⅱ.液膜扩散-递进扩散-界面分级交换反应联合控制的复合模型理论

为定量解释海水中液-固界面的台阶型动力学曲线及其台阶的消长变化规律,在我们已提出的“液膜扩散和递进液膜扩散控制的复合模型”和“海水中液-固界面分级离子/配位子交换理论”基础上,吸取Crank的若干数学处理方法,进而提出适合于非稳态体系的“液膜扩散-递进扩散-界面分级交换反应联合控制的复合模型”。     

日本沼虾染色体及其核型的研究

于１９９２年３月在上海青县采集日本沼虾，以改进的空气干燥法研究精巢细胞染色体及核型，特别较详细地研究了减数分裂前期Ｉ染色体的行为。结果表明，日本沼虾染色体数ｎ＝５３，２ｎ＝１０４，共分为Ａ，Ｂ，Ｃ，Ｄ４个染色体组；核型组成是Ｎ＝３７Ｍ＋４ＳＴ＋１１Ｔ；初级精母细胞减数分裂前期Ｉ可分为细线期／偶线期，粗线期、双线期和终变期５个时期，双线期的二价体存在弥散阶段，减数分裂的同步率高，大多处于双线期，且双     

基于COⅠ基因序列的长腹剑水蚤系统进化关系

长腹剑水蚤属（Oithona）是广泛分布于海洋近岸和外海海域的中小型桡足类中最为丰富的类群之一,由于个体小且形态差异微小,通过传统的形态学分类法对其进行准确鉴定难度较大。本文对南海分布的长腹剑水蚤属内的5个种,即瘦长腹剑水蚤（O.tenuis）、羽长腹剑水蚤（O.plumifera）、刺长腹剑水蚤（O.setigera）、伪长腹剑水蚤（O.fallax）和长刺长腹剑水蚤（O.longispina）线粒体COⅠ基因序列以及DNA数据库中长腹剑水蚤属其他地区种类COⅠ基因序列进行比较分析,使用ABGD （Automatic Barcode Gap Discovery）和GMYC （Generalized Mixed Yule Coalescent）模型进行物种界定,分析种间种内遗传距离,并构建系统进化关系。结果显示ABGD和GMYC模型均可以很好地对长腹剑水蚤进行种类划分;种内遗传距离为0.0%~1.6%,种间遗传距离为17.7%~44.5%（Kimura 2-parameter双参数模型）,表明种间出现较高的分化;贝叶斯系统树和最大似然树进化树结果均表明,简长腹剑水蚤（O.simplex）与其他种类相距较远,羽长腹剑水蚤和拟长腹剑水蚤（O.similis）中存在隐种的分化,分别是我国南海海域和地中海的羽长腹剑水蚤以及朝鲜海峡和北海的拟长腹剑水蚤,种间遗传距离分别为18.6%、22.9%。     

陕西黄土高原人工林土壤干层及形成原因

1 Introduction Abroad, a lot of research on soil water removal, seeping and evaporation has been done (Ole, 1998; Rapp, 2000). A seeping model of soil water was suggested (Yuin, 1998) and it was known that water removal is very slow in the unsaturated zon…     

长江三角洲城市带扩展对区域温度变化的影响

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.     

大地电场变化的频谱特征

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.      

EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts

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).     

雷诺数对圆形渐缩喷嘴湍流射流的影响

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.     

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

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).     

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

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.