基于行动者网络理论的乡村绅士化演化过程与机制解析——以广西巴马盘阳河流域为例

乡村绅士化是城乡要素双向流动背景下乡村转型与振兴的新型路径。基于对广西巴马盘阳河流域乡村绅士化现象的历时性田野调查,采用行动者网络理论解析乡村绅士化演化的过程、类型与机制。研究表明：在巴马盘阳河流域乡村人类行动者与非人类行动者、“草根”行动者与机构行动者共同缔结的行动者网络的转换过程中,伴随关键行动者从“候鸟人”先锋、屯社精英向地方政府、投资开发商的更替,乡村绅士化路径从“草根”绅士化向机构绅士化演替,乡村产业从接待“候鸟人”、发展旅游转向大健康产业融合发展,乡村绅士化类型从单一的舒适移民绅士化向舒适移民、旅游和地产共构的“一地多类”绅士化演化。关键行动者更替及其功能角色转换、绅士化路径变迁和主导产业更替与融合发展、宏观乡村发展制度与地域自然人文环境共同作用于乡村绅士化的阶段演替与类型共生。行动者网络理论与方法利于呈现乡村绅士化的阶段演替脉络与共生演化特征,并揭示乡村绅士演化的一般机制与地域机制。     

基于生态恢复的阿克苏河流域生态输水调度优化研究

生态输水调度是生态保护和恢复最有效的措施之一,实施生态输水对恢复干旱半干旱地区天然生态系统、维护绿洲生态系统健康具有重要意义。结合阿克苏河流域生态输水现状,在识别自然植被重点区和估算生态需水的基础上,建立了基于生态恢复目标的流域生态输水调度优化框架。首先采用高分系列影像识别自然植被信息,建立阿克苏河流域2015—2020年自然植被数据集,逐像元统计自然植被出现频次确定了艾希曼湖湿地区、第一师边缘胡杨林区、五团边缘胡杨林区3个自然植被重点区,面积达1257.69 km2;借助面积定额法和水量平衡法估算3个自然植被重点区的生态输水量分别为1.53×10⁸m³、2.73×10⁸m³、1.14×108m³;确定了流域生态输水的最佳时间为5—9月,单次或2次进行生态输水,建议单次生态输水量大于0.2×10⁸m³且输水天数大于10 d;渠系网络分析显示3个自然植被重点区设置的8个输水口可以作为今后生态输水路径的参考。研究结果对阿克苏河流域生态输水...     

黄河宁夏段凌汛期气温变化特征

利用宁夏1991~2010年20 a凌汛期水文和气温序列资料,研究了宁夏凌汛期特征、凌汛灾害发生主要时段,黄河封河、开河集中期与日平均气温之间的关系。结果表明:宁夏凌汛特征为封开河时序相反,小流量、高水位行洪,受强冷空气影响较大;凌汛灾害主要发生在封河和开河期间;日平均气温正负转化日期与封、开河期有对应关系,宁夏封河集中期在12月20日至1月19日;开河集中日期在2月13~20日。在凌汛关键期结合MODIS遥感数据对凌汛灾害监测防范有一定指导意义。     

灰色时序组合模型在基坑监测中的运用

科学、实时、准确地分析和预报建筑物、构筑物的变形在现代测量工程实践中有着重要的意义。文中将时间序列分析与灰色系统理论相结合用于变形监测沉降数据预测。结合国家超级计算长沙中心项目天河广场深基坑沉降监测的数据实例,说明预测方法具有容易实现与预测准确的优点,是一种非常有效的预测方法。     

基于QSSP的震源破裂过程反演方法

在Qt平台上,基于QSSP软件,利用C⁺⁺进行地震破裂过程反演方法研究。采用按阶段反演的方法,第1阶段反演采用热浴算法进行全局搜索,先按断层区域的构造背景等初始条件对参数范围进行划取,在该范围内随机给定一组初始值开始迭代,使波形初步拟合避开局部最优解;第2阶段反演使用拟牛顿法进行快速收敛,提高波形拟合程度,迭代至目标函数小于误差条件时停止,输出满足误差条件的待解模型参数。为避免模型参数出现病态问题,使用拉普拉斯方程建立平滑矩阵并引入平滑因子对断层模型进行平滑约束。使用棋盘模型验证该方法的稳定性和可靠性。最后,将全国13个台站的重力数据积分后对2013-04-20芦山7.0级地震的破裂过程进行反演,并与其他研究结论进行对比分析。     

Using modified state surface approach to select parameter values in the Barcelona basic model

The Barcelona basic model (BBM) successfully explained many key features of unsaturated soils and received extensive acceptance. It is also one of the few elastoplastic constitutive models for unsaturated soils that have been implemented within finite element codes and applied to the analysis of real boundary value problems. The BBM was proposed in incremental forms according to theories of soil plasticity in which individual aspects of the isotropic virgin behavior are controlled by multiple parameters, whereas at the same time, a single parameter controls more than one aspect of soil behavior. Although a variety of methods have been recently developed for calibrating model parameters for elastoplastic soil models, at present, there are no well‐established, simple, and objective methods for selecting parameter values in the BBM from laboratory tests. This has been one of the major obstacles to the dissemination of this constitutive model beyond the research context. This article presents an optimization approach especially developed for simple and objective identification of material parameters in the BBM. This is achieved by combining a modified state surface approach, recently proposed to model the elastoplastic behavior of unsaturated soils under isotropic stress conditions, with the Newton or quasi‐Newton method to simultaneously determine the five parameters governing isotropic virgin behavior in the BBM. The comparison between results using the proposed method and an existing method for the same laboratory tests was discussed from which the simplicity and objectivity of the proposed method were evaluated. Copyright © 2012 John Wiley & Sons, Ltd.     

A unified linear theory of wavelike perturbations under general ocean conditions

A linearized instability analysis model with five unknowns was proposed to describe disturbance motions under general oceanic background conditions, including large-scale current shear, density stratification, frontal zone, and arbitrary topography. A unified linear theory of wavelike perturbations for surface gravity waves, internal gravity waves and inertial gravity waves was derived for the adiabatic case, and the solution was then found using Fourier integrals. In this theory, we discarded the assumptions widely accepted in the literature concerning derivations of wave motions such as the irrotationality assumption for surface gravity waves, the rigid-lid approximation for internal gravity waves, and the long-wave approximation for inertial gravity waves. Analytical solutions based on this theory indicate that the complex dispersion relationships between frequency and wave-number describing the propagation and development of the three types of wavelike perturbation motions include three components: complex dispersion relationships at the sea surface; vertical invariance of the complex frequency; and expressions of the vertical wave-number (phase). Classical results of both surface waves and internal waves were reproduced from the unified theory under idealized conditions. The unified wave theory can be applied in the dynamical explanation of the generation and propagation properties of internal waves that are visible in the satellite SAR images in the southern part of the China Seas. It can also serve as the theoretical basis for both a numerical internal-wave model and analytical estimation of the ocean fluxes transported by wavelike perturbations.     

鄂尔多斯盆地高自然伽马异常特征

为了加深对盆地深部和浅部高自然伽马异常特征综合分析研究,揭示高自然伽马异常地质成因,从而促进盆地多种能源矿产协同开发研究,针对收集大量的地球物理测井资料、地质资料及其他相关成果,绘制并分析了相关成果图。研究中遵循从单孔测井曲线特征分析到典型剖面研究,并按层对高自然伽马的平面分布特征进行分析研究。化验测试结果和自然伽马能谱测井成果研究表明,在本区,自然伽马异常增大主要是由于铀的活化和聚集,导致铀元素增加而引起。相关研究表明,盆地深部和浅部的铀异常具有一定的关系,盆地历经的沉积环境变迁是铀元素富集的主导因素。     

速度分布和银盘厚度效应对正常脉冲星Z向分布的影响

基于彭秋和等1978年得到的无扰动有限厚盘引力势,根据两个引力势参数(h_(z1)= 0．001kpc,h_(z2)=0．325 kpc)和两个速度分布参数(σ_(v1)=115km/s,σ_(v2)=200 km/s)组合的4种情况,对4×10~5颗脉冲星做了三维蒙特卡洛模拟．4×10~5颗脉冲星按着10~8年间隔被分成20组,计算了每组“逃逸”脉冲星所占比例．对每组中“未逃逸”脉冲星,分别在0＜r＜25kpc和5＜r＜11kpc两个区域中对|z|分布做了统计,研究了“未逃逸”脉冲星在这两个区域中的分段标高和累积标高的演化特征．“未逃逸”脉冲星的分段标高在一定空间范围内的变化不规则,但累积标高的变化却比较平滑．在相对长的时间里(＞10~8年),银盘厚度对脉冲星累积标高演化有显著的复杂影响；在相对短的时间中(＜2×10~7年),这种效应很小,而且累积标高对时间的依赖关系是线性的．在长时间里,初始速度分布对累积标高也有显著影响．在引力势h_(z2)=0．325 kpc的条件下,在径向范围5＜r＜11kpc和时间t=9．22×10~6年以及σ_(v2)=200km/s的情况下,模拟的累积标高是0．596±0．005 kpc．     

密近双星自转的测量和研究（Ⅰ）观测和处理结果

用相同的仪器条件在美国ＫｉｔｔＰｅａｋ国立天文台观测了一批密近双星，并用两种方法得出其自转速度，最后给出了７５个双星系统的９９个子星的自转速度，其中５４个子星是首次进行自转测量。这批高精度的自转值为研究双星的同步性和检验各种同步机制提供了可靠的观测资料。