SD-WACCM模式对平流层化学组分的模拟研究

利用美国大气研究中心开发的全球气候模式,对2008年平流层的化学组分(HNO₃、HCl和O₃)进行了模拟研究,并结合了MLS卫星资料进行了对比分析。结果表明,模式可以较好地再现平流层的各化学组分的时空分布状况。并选取了8个区域,将模拟的2008—2009年O₃柱浓度与臭氧监测仪资料对比,结果表明,模式可以较好地再现全球O₃总量的季节变化情况。     

Effects of Enclosure on Plant and Soil Restoration in the Junggar Desert

Enclosure is commonly used in the restoration of degraded grasslands. However, the effects of enclosure on grassland plant and soil restoration remain controversial, particularly in deserts. To assess the effects of enclosure on desert plants and soil properties, using high throughput sequencing, the differences between plants and soil were systematically analyzed before and after enclosure construction. The soil organic carbon, total nitrogen and total phosphorus contents of the three desert flora increased and decreased, but the difference was not significant; enclosure increased plant height, coverage, aboveground biomass, and species richness by 58.99%, 59.35%, 33.29%, and 51.21%, respectively, in a Seriphidium transiliense formation; by 15.49%, 33.52%, 20.85%, and 5.13%, respectively, in a Haloxylon persicum formation; and by 83.80%, 31.51%, 76.66% and 33.33%, respectively, in an Anabasis salsa formation. For soil bacteria, enclosure significantly increased the average number of operational taxonomic units and Shannon-Wiener index by 12.74% and 2.92%, respectively, under S. transiliense formation and by 17.08% and 3.17%, respectively, under H. persicum formation. However, enclosure had no significant effect on the average number of operational taxonomic units or Shannon-Wiener index under A. salsa formation. Enclosure significantly increased desert plants, soil bacterial diversity, and desert plant community productivity; however, the increase in soil nutrient content was not significant. These results demonstrate that enclosure is effective for restoring desert ecosystems but may have little effect on the soil nutrient content.     

华北地区上部地壳结构的三维有限差分层析成像

采用正方形网格对华北地区速度模型进行参数化、网格维数为649×90×16,网格间距为1km. 通过对华北地区30条深地震测深剖面的Pg波三维有限差分速度层析成像反演,获得了该地区上部地壳的三维速度结构. 反演结果显示,低速的"棱形"华北盆地被高速的隆起所包围;而华北盆地又由两个大的断陷带中间夹一个隆起所组成.两个大的断陷带又被分割为多个小的断陷盆地.研究区内的断层多为铲式正断层,结晶基底深度变化较大. 所有这些表明华北地区具有复杂的地质构造和发生强震的深部背景.     

基于GIS的高等师范院校地理科学专业教学模式研究

GIS空间技术是当今地球科学研究的重要支撑手段,已成为地球科学各学科专业的必修课程之一.在论述开设GIS课程重要性的同时,针对GIS在地理专业教学中的特点,探讨了基于GIS的地理专业教学模式,认为基于GIS操作平台、GIS输出数据、3DGIS和VRGIS、WebGIS以及Google Erath的地理教学模式是地理科学教学方法改革的重要方向.     

区域沙漠化程度评价研究进展、问题及分析

通过回顾景观尺度及区域尺度的沙漠化程度评价发展过程,概括了国内外典型的区域沙漠化程度评价方法,通过假设各种情景分析、总结了目前各类区域沙漠化程度评价方法中存在的典型共性问题：(1)当被比较评价的几个区域中各类沙化土地面积相等时,目前所有的评价模型失去比较能力;(2)忽略了不同类型沙化土地空间分布的生态学意义及其对区域沙化整体程度的影响;(3)目前考虑了不同类型沙化土地空间分布的模型由于指标因子选择不恰当其评价结果在有些情况下与实际情况有距离。提出了在现有评价方法的基础上根据景观生态学原理引进景观生态学方法,特别是景观格局分析的方法,可以弥补现有区域沙漠化程度评价方法中存在的缺陷和不足,并且可以使区域沙漠化程度评价具有生态学意义。     

一种锁相环调频方法在铷原子频标中的应用

为了进一步实现铷原子频标小型化,分析了几种典型的锁相环调频电路及其特点,设计了一种锁相环二进制移频键控2FSK(binary frequency shift keying)调频方案,给出了调频信号的频谱测试结果。该调频方案已成功地应用在小型化数字式铷原子频标中,能够满足小型化铷原子频标的要求。     

Ex situ echo sounder target strengths of ice krill Euphausia crystallorophias

Ice krill is the keystone species in the neritic ecosystem in the Southern Ocean,where it replaces the more oceanic Antarctic krill. It is essential to understand the variation of target strength(TS in d B re 1 m 2) with the different body size to accurately estimate ice krill stocks. However,there is comparatively little knowledge of the acoustic backscatter of ice krill. The TS of individual,formalin-preserved,tethered ice krill was measured in a freshwater test tank at 38,120,and 200 k Hz with a calibrated split-beam echo sounder system. Mean TS was obtained from 21 individual ice krill with a broad range of body lengths(L :13–36 mm). The length( L,mm) to wet weight( W; mg) relationship for ice krill was W =0.001 218×103 × L 3.53( R 2= 0.96). The mean TS-to-length relationship were TS3 8 k Hz =-177.4+57log 10( L),( R 2 = 0.86); TS 120 k Hz =-129.9+31.56 log 10( L),( R 2 =0.87); and TS 200 k Hz =-117.6+24.66log1 0( L),( R 2 =0.84). Empirical estimates of the relationship between the TS and body length of ice krill were established at 38,120,and 200 k Hz and compared with predictions obtained from both the linear regression model of Greene et al.(1991) and the Stochastic Distorted Wave Born Approximation(SDWBA) model. This result might be applied to improve acoustic detection and density estimation of ice krill in the Southern Ocean. Further comparative studies are needed with in situ target strength including various body lengths of ice krill.     

Impact of sea spray on upper ocean temperature during typhoon passage: simulation with a 1-D turbulent model

At the interface between the lower atmosphere and sea surface, sea spray might significantly influence air-sea heat fluxes and subsequently, modulate upper ocean temperature during a typhoon passage. The effects of sea spray were introduced into the parameterization of sea surface roughness in a 1-D turbulent model, to investigate the effects of sea spray on upper ocean temperature in the Kuroshio Extension area, for the cases of two real typhoons from 2006, Yagi and Soulik. Model output was compared with data from the Kuroshio Extension Observatory (KEO), and Reynolds and AMSRE satellite remote sensing sea surface temperatures. The results indicate drag coefficients that include the spray effect are closer to observations than those without, and that sea spray can enhance the heat fluxes (especially latent heat flux) considerably during a typhoon passage. Consequently, the model results with heat fluxes enhanced by sea spray simulate better the cooling process of the SST and upper-layer temperature profiles. Additionally, results from the simulation of the passage of typhoon Soulik (that passed KEO quickly), which included the sea spray effect, were better than for the simulated passage of typhoon Yagi (that crossed KEO slowly). These promising 1-D results could provide insight into the application of sea spray in general circulation models for typhoon studies.     

银河系卫星星系研究进展

对银河系内卫星星系进行全面的"人口普查"具有重要的意义。目前已经发现了二十几个卫星星系,其光度范围分布很广,最暗的矮星系比球状星体还暗。叙述了卫星星系的光度分布、空间分布和动力学性质。总结了观测和理论研究进展,并讨论了星流和伽玛射线在研究银河系结构和暗物质性质方面的贡献。表明了卫星星系的统计分布能用来很好地限制冷暗物质理论和星系形成的相关物理过程,同时指出当前研究的局限性和可能的发展方向。     

沂水县北躲庄铁矿地质特征

山东省沂水县北躲庄矿区处于汞丹山凸起之上,其西侧为马站苏村凹陷,东侧为莒县凹陷。区域地层分布较齐全,构造复杂,岩浆岩发育。该矿区地层简单,只出露新太古代泰山岩群柳杭组地层包体和新生代第四纪松散堆积物;构造有韧性剪切带和脆性断裂构造2种;岩浆岩发育,主要分布有古元古代条花峪单元、松山单元、三官寨单元。铁矿体赋存于泰山岩群柳杭组的顶部,共圈定了7个矿体,矿体呈层状产出,倾向110＆#176;～120＆#176;,倾角47＆#176;～82＆#176;。TFe 品位29％～37％。其矿体成因为沉积变质型铁矿。