基于随机森林的中小跨径公路梁桥双柱墩地震易损性模型

为准确建立线路中小跨径梁桥桥墩的地震易损性模型,采用统计工具得到某山区高速公路桥梁双柱墩的结构、几何和材料特性的概率分布,由拉丁超立方体抽样生成桥墩属性数据集,建立了参数化的有限元模型.通过Pushover分析和基于非弹性需求谱的能力谱方法获取双柱墩的地震需求和抗震性能数据点,提出由随机森林(RF)模型建立桥墩地震易损...     

基于飞机观测资料的石家庄秋季对流层CH4垂直分布特征

为研究石家庄秋季对流层内CH₄垂直分布特征,2018年9月使用“空中国王350”飞机搭载Picarro温室气体在线观测仪和气象要素观测设备,对石家庄上空（600—5500 m）CH₄浓度进行探测。探测期间共飞行7架次,取得7条CH₄浓度廓线数据。结果表明: 石家庄上空近地面层（1000 m以下）CH₄平均浓度与同时间段区域背景站上甸子站CH₄浓度呈显著正相关（r=0.81,P < 0.03）。探测到的CH₄浓度最小值为1898×10^-9摩尔分数,最大值为2219×10^-9摩尔分数,平均浓度为1981×10^-9摩尔分数。观测得到的7条廓线均有较好的一致性,2000 m以上,浓度均随高度呈先增大后减小的趋势。利用后向轨迹模式（HYSPLIT）对探测时段内石家庄上空不同高度层主要气流传输路径进行统计分析表明,600 m高度输送路径较短,CH₄浓度受本地排放影响较大; 3000 m受输送作用影响较大,偏西和西南路径可能将较高CH₄浓度气团输送至石家庄上空; 5000 m气团传输对CH₄浓度影响较小,浓度相对较稳定,对传输路径的变化不敏感。     

The heating of the solar transition region

The temperature curve in the solar chromosphere has puzzled astronomers for a long time.Referring to the structure of supergranular cells,we propose an in ductive heating model.It mainly includes the following three steps.(1) A small-scale dynamo exists in the supergranulation and produces alternating small-scale magnetic fluxes;(2) The supergranular flow distributes these small-scale fluxes according to a regular pattern;(3) A skin effect occurs in the alternating and regularly-distributed magnetic fields.The induced current is concentrated near the transition region and heats it by resistive dissipation.     

The “Same Side – Opposite Side Effect” of the Heliospheric Current Sheet in Ionospheric Negative Storms

Using 141 CME-interplanetary shock (CME-IPS) events and foF2 from eight ionosonde stations from January 2000 to September 2005, from the statistical results we find that there is a “same side?–?opposite side effect” in ionospheric negative storms, i.e., a large portion of ionospheric negative disturbances are induced by the same-side events (referring to the CMEs whose source located on the same side of the heliospheric current sheet (HCS) as the Earth), while only a small portion is associated with the opposite-side events (the CMEs source located on the opposite side of the HCS as the Earth); the ratio is 128 vs. 46, and it reaches 41 vs. 14 for the intense ionospheric negative storms. In addition, the ionospheric negative storms associated with the same-side events are often more intense. A comparison of the same-side event (4 April 2000) and the opposite-side event (2 April 2001) shows that the intensity of the ionospheric negative storm caused by the same-side event is higher than that by the opposite-side event, although their initial conditions are quite similar. Our preliminary results show that the HCS has an “impeding” effect to CME-IPS, which results in a shortage of energy injection in the auroral zone and restraining the development of ionospheric negative perturbations.     

AMR Simulations of Magnetohydrodynamic Problems by the CESE Method in Curvilinear Coordinates

The objective of this paper is to present new extensions of the space – time conservation element and solution element (CESE) method for simulations of magnetohydrodynamic (MHD) problems in general curvilinear coordinates by using an adaptive mesh refinement (AMR) grid system. By transforming the governing MHD equations from the physical space (x,y,z) to the computational space (ξ,η,ζ) while retaining the form of conservation, the CESE method is established for MHD in the curvilinear coordinates. Utilizing the parallel AMR package PARAMESH, we present the first implementation of applying the AMR CESE method for MHD (AMR-CESE-MHD) in both Cartesian and curvilinear coordinates. To show the validity and capabilities of the AMR-CESE-MHD code, a suite of numerical tests in two and three dimensions including ideal MHD and resistive MHD are carried out, with two of them in both Cartesian and curvilinear coordinates. Numerical tests show that our results are highly consistent with those obtained previously by other authors, and the results under both coordinate systems confirm each other very well.     

The Contribution from Radio Quiet Quasars to γ-ray Background

The EGRET observations have confirmed and proposed the new isotropically distributed γ-ray background, but the known objects radiating γ-rays can not supply so much radiation. Meanwhile, EGRET also reveals a population of γ-ray sources with no radio counterparts which are isotropically distributed in the sky, indicating their possible cosmological origins. Wang et al.^[13] proposed a new γ-ray radiation process driven by the radiation feedback of AGNs. The energy of the radiation peaks around 1 GeV—0.1 TeV with the typical luminosity of 10⁴²—10⁴³ ergs · s^?1. This kind of radiation process in the radio quiet quasars make them the potential γ-ray radiation sources as well as the contributors to the γ-ray background. We consider two cases in which the seed photons in the inverse-Compton processes are from the accretion disks of quasars and cosmic microwave background (CMB), respectively. We find that the former contributes 78%—92% of the background radiation around 1 GeV, while the contribution from the latter is negligible. The radio quiet quasars are highly likely to become the objects which contribute the most energy to the γ-ray background around 1 GeV.     

海水鱼类寄生虫刺激隐核虫(Cryptocaryon irritans)趋化性研究

应用本实验室建立的趋化模型对海水鱼类寄生虫刺激隐核虫(Cryptocaryon irritans)的趋化特性进行研究。结果显示, 刺激隐核虫幼虫在30min时趋化达到饱和, 在温度28℃时趋化率达到最高; 多种硬骨鱼的血清与粘液对刺激隐核虫的幼虫都有着强烈的吸引作用, 刺激隐核虫幼虫对碳水化合物、氨基酸等小分子物质没有趋化作用; 在组织匀浆液中, 刺激隐核虫幼虫对肌肉匀浆液有一定的趋化作用, 对肝、肠、胃的匀浆液都没有趋化作用; 感染后鱼类血清对刺激隐核虫的幼虫有着更加强烈的吸引作用(P<0.01); 18种中草药中的五倍子、大黄、槟榔、苦楝、虎杖、贯众等6种中药草对刺激隐核虫的幼虫有一定的驱虫作用。本文的研究结果有助于深化对刺激隐核虫致病性的认识并对“白点病”的防治有一定的参考价值。     

银鲳(Pampus argenteus)幼鱼饥饿前后侧囊及肝脏超微结构的变化

分别采用扫描和透射电镜, 观察了正常和饥饿5d银鲳(Pampus argenteus)幼鱼的食道侧囊及肝脏超微结构的变化。结果表明, 正常银鲳幼鱼侧囊内壁具有许多平均高度为800?m的乳突, 上有次级突起。乳突黏膜由复层扁平上皮构成, 上皮细胞表面有指纹状的微嵴, 有缓解上皮细胞的机械损伤作用; 银鲳肝脏具肝血窦、胆小管、狄氏窦等结构, 肝细胞排列较紧密, 内含丰富的细胞器和脂滴, 核仁大而明显, 线粒体数目多, 多分布在细胞核、内质网和狄氏窦周围。饥饿后, 侧囊乳突变低矮, 平均高度700?m, 乳突上黏膜变薄, 逐渐退缩, 次级突起顶端露出了尖刺状的角质刺; 肝细胞体积缩小, 核变小, 细胞器数目减少, 线粒体水肿, 粗面内质网数量显著降低, 脂滴数量降低, 这是银鲳幼鱼对饥饿的生理性防御。     

垃圾填埋场渗沥液pH值变化对粘土防渗层压缩性的影响

粘土防渗层是垃圾填埋设施中直接接触渗沥液的防渗层,防渗层有效地阻隔了垃圾渗沥液下渗,减少了渗沥液对环境的污染.以成都粘土为研究对象,采用高压固结试验研究粘土防渗层在不同浸润时间、不同pH渗沥液浸润下对粘土层固结参数的影响.结果表明:浸润时间和渗沥液pH对粘土固结参数的影响较大.随着浸润时间的增加,渗沥液pH值对土的压缩...     

Heavy metal contamination in western Xiamen Bay sediments and its vicinity, China

Concentrations of selected heavy metals (Cu, Pb, Zn, Cd, Cr, Ni and Fe) in surface sediments from nine sites in western Xiamen Bay and its vicinity were studied in order to understand current metal contamination due to urbanization and economic development in Xiamen, China. The sediment samples were collected in December 2004 and July 2005 respectively in order to examine temporal variations. In this study, we found that heavy metal concentrations in surface sediments sampled in the western Xiamen Bay and adjacent Maluan Bay and Yuandang Lagoon varied from 19 to 97mg kg(-1) for Cu, 45 to 60mg kg(-1) for Pb, 65 to 223mg kg(-1) for Zn, 0.11 to 1.01mg kg(-1) for Cd, 37 to 134mg kg(-1) for Cr, 25 to 65mg kg(-1) for Ni and 3.08 to 4.81% for Fe. Although all metal concentrations in sediments meets Chinese National Standard Criteria for Marine Sediment Quality, both metal enrichment factors (EF) and geoaccumulation index (I(geo)) show that Pb contamination exists in the entire study area and contamination of other metals are also present in some locations depending on the sources, of which sewage outlets and commercial ports are the main sources of contaminants to the area. This study shows that using the sediment quality standard criteria only to assess sediments cannot properly reflect sediment contamination. A multiple approaches should be applied for the sediment quality assessment.