4D-DECT对甲状旁腺腺瘤的诊断价值

目的:探讨甲状旁腺腺瘤(PA)的4D-DECT影像特征及物质成分信息,评价其定位及定性诊断价值.资料和方法:回顾性分析经手术及病理证实的53例PA患者的临床资料及4D-DECT影像资料,逐一观察并记录CT征象,分别对病变与邻近组织的CT衰减值(HU)、碘浓度、Rho、Z值及DEI进行测定及比较分析.结果:53例患者中,...     

“人工鲸落”型海洋牧场的理论基础与构建体系

海洋牧场作为新的生态型海洋渔业生产方式,同时也是我们获取优质蛋白的重要来源,近年来得到快速发展,目前已形成了增殖型、养护型和休闲型海洋牧场建设模式。随着海洋强国战略的加快实施,海洋牧场逐渐挺进深蓝,在其快速发展的同时也存在建设模式单一、同质化现象突出和生态承载力提升受限等问题,在一定程度上限制了海洋牧场的创新发展。而鲸落生态系统作为海洋生态系统的一部分,其生态作用对海洋牧场的发展将会起到显著的促进作用。文章在系统梳理海洋牧场发展历史和鲸落生态系统原理的基础上,把二者有机结合,将鲸落形成的生态原理充分运用到海洋牧场建设过程中,构建人工鲸落型海洋牧场技术体系和建设模式,通过人工方式充分发挥鲸落等大型动物外源性营养物质的规模化输入效应,提升海洋牧场区域生产力,进而提高资源养护与产出能力,以期为我国海洋牧场建设发展提供新的思路和方向参考。     

海草床鱼类群落结构的时空变化及其在热带海草床中的育幼

本文以印尼北苏拉威西东部的潟湖为对象,研究了热带海草床鱼类群落的种类组成和时空变化。研究发现当地鱼类的香农-威纳指数在1.57-3.69之间多样性相对较高。在科水平,天竺鲷科的丰度（8.27 ind./（100 m²））和生物量（28.49 g/（100 m²））最高。在物种水平,侧带天竺鲷（Apogon lateralis）的丰度最高,环纹圆天竺鲷（Sphaeramia orbicularis）的生物量最大。对于物种的空间变化,潟湖湖顶、湖中和湖口首先聚类在一起,这可能是由于基质类型引起的。干季和湿季的鱼类种类、丰度和生物量均比转换季高,这可能是由较强的季风造成的,强季风为鱼类提供了更适宜的环境和食物。93.1%的鱼类的最大体长小于它们的性成熟体长,暗示了海草床是很多鱼类的育幼场。因此,保护海草床对渔业和资源的可持续利用至关重要。     

基于MapGIS的气象预报分析系统的设计与实现

介绍了以MapGIS地理信息系统为技术平台所开发的气象预报分析系统(WeatherGIS)的组织结构,数据录入、来源数据编辑、数据处理、结果数据编辑、数据输出、系统设置等模块的主要功能,以及系统应用状况。     

印度尼西亚北苏拉威西蓝碧海峡浮游动物种类组成及分布

Based on oceanographic survey data in June 2012 in the Lembeh Strait, the zooplankton ecological characteristics such as species composition, individual abundance, dominant species and distribution were analyzed. The results showed that 183 species(including 4 sp.) had been recognized, most of them belonged to copepoda.Cnidaria followed with 43 species(including 1 sp.) were identified. The average abundance of zooplankton was(150.47±58.91) ind./m~3. As to the horizontal distribution, the abundance of the zooplankton was higher in the southern waters than in the northern waters. The dominant species in the study area were Lensia subtiloides,Sagitta enflata, Lucifer intermedius, Oikopleura rufescens, Diphyes chamissoni, Creseis acicula, Subeucalanus subcrassus, Temora discaudata, Aglaura hemistoma, Doliolum denticulatum, Canthocalanus pauper, Oikopleura longicauda and Nanomia bijuga. Zooplankton biodiversity indexes were higher in study area than previous study in the other regions. The findings from this study provide important baseline information for future research and monitoring programs.     

Direct constraint on cosmic neutrino mass using observational Hubble parameter data

In order to explore the properties of cosmic neutrinos, i.e. sum of the neutrino mass(∑m_ν) and the effective number of neutrino species(N_(eff)), which affects the Hubble expansion rate H(z)and the power of observational Hubble parameter data(OHD) in constraining cosmological parameters under the ΛCDM model, we utilize OHD to constrain the properties of cosmic neutrinos and apply an accurate H(z) function with mνand Neff. First, we simulate new OHD beyond the existing 43 OHD. According to the predictions of measurements of H_0(the current H(z) value), baryon acoustic oscillations(BAO) peaks, Sandage-Loeb(SL) test and cosmic microwave background(CMB), we assume observational accuracy up to 2% and redshift 0 z ≤5. With simulated H(z) data obtained from the fiducial model, we constrain the parameters including mνand Neff. When all parameters are set free, mν 0.196 eV(95%) and N_(eff)= 2.984 ± 0.826(68%) are obtained, and when fixing Neff as the standard baseline 3.046, we attain ∑m_ν 0.240 eV(95%). These constrained results are much tighter than the ones obtained by the current OHD, which makes the prospect of OHD in constraining cosmological parameters more promising as its accuracy and quantity grow.     

Research on the Application of Fast-steering Mirror in Stellar Interferometers

In stellar interferometers, the fast-steering mirror (FSM) is widely utilized to correct the wavefront tilt caused by the atmospheric turbulence and internal instrumental vibration, because of its high resolution and fast response frequency. In this study, the non-coplanar error between the FSM and the actuator deflection axis introduced by the manufacturing, assembly, and adjustment is analyzed systematically. Via a numerical method, the additional optical path difference (OPD) caused by the above factors is studied, and its effect on the fringe tracking accuracy of a stellar interferometer is also discussed. On the other hand, the starlight parallelism between the beams of two arms is one of the main factors for the loss of fringe visibility. By analyzing the influence of wavefront tilt caused by the atmospheric turbulence on fringe visibility, a simple and efficient real-time correction scheme of starlight parallelism is proposed based on a single array detector. The feasibility of this scheme is demonstrated by a laboratory experiment. The results show that after the correction of fast-steering mirror, the starlight parallelism meets preliminarily the requirement of a stellar interferometer on the wavefront tilt.     

Effect of slow-solvent-vapour treatment on performance of polymer photovoltaic devices

In this work, enhanced poly(3-hexylthiophene):[6,6]-phenyl-C61-butyric acid methyl ester (P3HT:PCBM) bulk-heterojunction photovoltaic devices are achieved via slow-solvent-vapour treatment. The correlations between the morphology of the active layer and the photovoltaic performance of polymer-based solar cell are investigated. The active layers are characterized by atomic force microscopy and optical absorption. The results show that slow-solvent-vapour treatment can induce P3HT self-organization into an ordered structure, leading to the enhanced absorption and efficient charge transport.     

Structural, curvature and electronic properties of Rh adsorption on armchair single-walled carbon nanotube

This paper systematically studies the rolling effects of the (n, n) single-wall carbon nanotubes (SWCNT) with different curvatures on Rh adsorption behaviours by using density functional theory. The outside charge densities of SWCNTs are found to be higher than those inside, and the differences decrease with the increase of the tube radius. This electronic property led to the discovery that the outside adsorption energies are higher than the inside ones, and that the differences are reduced with the increase of the tube radius. Partial density of states and charge density difference indicate that these strong interactions induce electron transfer between Rh atoms and SWCNTs.     

多溴联苯醚在海洋生物中的富集及毒性效应评述

多溴联苯醚(PBDEs)作为一种新型的持久性有机污染物,在海洋环境中广泛存在,对海洋生物的影响也日趋加大,因此评价PBDEs的海洋生态效应十分必要.本文在简介海水中PBDEs化学行为的基础上,依次阐述PBDEs在海洋浮游生物、底栖动物、游泳生物体内的富集,其沿海洋生态食物链(网)的传递规律与毒性效应,还展望了PBDEs海洋生态效应今后需加强的研究内容.