Comparison of P‐wave attenuation models of wave‐induced flow

Wave‐induced oscillatory fluid flow in the vicinity of inclusions embedded in porous rocks is one of the main causes for P‐wave dispersion and attenuation at seismic frequencies. Hence, the P‐wave velocity depends on wave frequency, porosity, saturation, and other rock parameters. Several analytical models quantify this wave‐induced flow attenuation and result in characteristic velocity–saturation relations. Here, we compare some of these models by analyzing their low‐ and high‐frequency asymptotic behaviours and by applying them to measured velocity–saturation relations. Specifically, the Biot–Rayleigh model considering spherical inclusions embedded in an isotropic rock matrix is compared with White's and Johnson's models of patchy saturation. The modeling of laboratory data for tight sandstone and limestone indicates that, by selecting appropriate inclusion size, the Biot‐Rayleigh predictions are close to the measured values, particularly for intermediate and high water saturations.     

热带气旋暴雨增幅造成北方特大暴雨的预报

利用人工神经元网络的非线性决策特性，采用前向多层的误差反向传输网络，研制了一个登陆北上热带气旋暴雨增幅造成北方特大暴雨的预报方法－－能自动判虽有无暴雨增幅及其出现地区的人工神经元分类预报网络。该方法简便客观，试用效果较好，即可投入业务使用。     

建德铜矿床的海底喷流沉积成因

建德铜矿床是浙江西部多金属成矿带中一个引人瞩目的重要矿床。它产于中石炭统底部伴有火山岩、硅质岩和碧玉岩的白云岩中。整合块状矿体之下有一筒状矿化蚀变带。其成分以Ｃｕ＞Ｚｎ＞Ｐｂ为特征。根据矿床地质、地球化学特征以及近年来研究所获得资料，认为该矿床属海底喷流沉积成因     

内蒙古狼山地区的层控铀矿及其控制因素的卫片影象模式

狼山地区广泛分布着花岗岩型铀矿化和砂岩型铀矿化。本文通过对该区的遥感地质综合解译,重点研究了几个含铀盆地的砂岩型铀矿化成矿特点及其通感图象的影象特征,发现广布于早白垩世断陷盆地的砂岩型铀矿化是一典型的层控型铀矿。并通过区域构造型式的研究,强调了弧形构造的断块活动特征及其对含铀盆地和含矿层分布的控制作用;揭示了弧形构造的后期活动和环形构造、北北东向线性构造与铀矿化的再造关系。从而得出砂岩铀矿化是受地层岩相和弧、环、线构造“四位一体”条件控制的新认识。该矿化在MSS图象上呈现一定的影象特征,据此,本文概括出本区层控铀矿的影象模式。     

Influence of environmental, root, and stand parameters on soil surface CO2 efflux in a Populus euphratica of desert forest in extreme arid region

Spatial variation in soil surface CO2 efflux was measured in a stand of Populus euphratica in the Ejina Oasis of desert riparian forest in the extreme arid region in northwestern China from April 2007 through October 2007.Measurements were taken with a gas-exchange analyzer linked to a soil-respiration chamber.The mean soil CO2 efflux in the stand was 2.71 μmol/(m2·s) during the growing season and 1.38 μmol/(m2·s) in the nongrowing season.The seasonal maximum (end of May through early June) andminimum (October) CO2 efflux were 3.38 and 0.69 μmol/(m2·s),respectively.The diurnal fluctuation of CO2 efflux was relatively small (< 20 percent),with theminimum appearing around 05:00 and the maximum around 15:00.Linear regression analysis showed soil-surface CO2 efflux to be most highly correlated with soil temperature (R2=0.435) and soil moisture (R2=0.213).When all variables were considered simultaneously,only soil temperature (R2=0.378),soil moisture (R2=0.147),and root volume density (R2=0.021) explained a significant amount of variance in soil surface CO2 efflux.Stand volumes were not correlated with soil CO2 efflux on our sites.     

Study on the Period Changes of xy Leonis

XY Leo (BD+18° 2307, p = 0d .28) was observed each season from 1992 through 1995 at Yunnan Observatory with the 1 m telescope and 37 new heliocentric times of minimum light were determined. The newly expanded database of the minimum times,including these new epochs, definitely confirm the sine-like variation of its O–C values. Observations and analyses strongly supported the viewpoint that the variation of the O–C values of the minimum times is mainly caused by the light- time effect. Based on this newly expanded database, new light elements for the eclipsing system XY Leo and new light-time orbit for this complex system have been obtained with much better accuracy than before by means of the least squares fitting to the light-time equation. It's also noted that the additional period variation for XY Leo probably may not be ruled out besides the light-time effect. The method of analysis and the discussion of the results are presented in this paper. This revised version was published online in July 2006 with corrections to the Cover Date.     

Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in the Spitzer First Look Survey Field

We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506.     

基于模糊层次分析法对“一带一路”重要区域地质灾害危险性评价——以关中经济区为例

在“一带一路”沿线区域开展地质灾害危险性评价与区划具有重大意义。本文以关中经济区为例,综合考虑地质灾害特点、分布规律与孕灾环境等要素,基于坡度和地形起伏度的组合,提出了地质灾害安全区域与非安全区域的初步识别方法。在此基础上,采用模糊层次分析法和GIS空间分析方法对地质灾害各孕灾因子进行了危险性等级评价,并分别进行了单因子和多因子综合制图与结果验证。研究结果表明：1）地质灾害安全区域与非安全区域的初步判识,对灾害风险管理和降低防灾减灾成本有重要参考价值,也大大提高了地质灾害评价区域的针对性和准确性。2）研究区地质灾害安全区域面积占比22.9%（17054.5km²）,非安全区域占比77.1%（57462.6km²）,轻度危险区、低危险区、中危险区和高危险区面积分别占非安全区域面积的17.2%、32.2%、32.0%、18.6%,以中、低危险性为主（64.2%）。高危险性区域集中分布在关中经济区的西北、西南、东南部,而轻度危险性区域集中分布在关中平原以南地区,呈现出东西走向的“条带状”。3）共计3230个灾害点中,仅有3.3%（106个）的灾害点分布在安全区域中,其余96.7%（3124个）的灾害点均分布在非安全区域之中。分布在轻度危险、低危险、中危险和高危险区域中的分别有328个（10.2%）、765个（23.7%）、1007个（31.2%）、1024个（31.7%）,这与危险性等级区划结果具有很好的一致性。表明本文提出的地质灾害安全区域识别方法和地质灾害危险性区划方法具有一定的科学性和准确性。

     

低地球轨道（LEO）的大型航天器充电

本文根据ＬＥＯ中等离子体温度低，密度高，德拜长度小的特点，采用薄鞘层近似，计算了离子收集电流；根据电流平衡方程，考虑表面二次电子发射，计算了大型航天器表面在沉降电子流辐照下的充电特性。     

地面观测资料地形高度订正对我国东部暴雨数值模拟的影响

采用中尺度气象模式 WRFv3.8.1(Weather Research and Forecasting Model)和 GSI 同化系统(Gridpoint Statistical Interpolation System),建立了一套循环同化系统,开展了一个月的地面观测资料、探空资料、雷达资料和卫星资料的同化试验....