河北保定岩溶地热结垢过程模拟及防垢对策

我国的地热发电以及部分供暖工程出现了比较严重的结垢现象,阻碍了地热能的大规模开发利用,目前地热市场急需成熟的防垢理论和工艺。地热工程的结垢现象尤以碳酸钙结垢最为普遍,为解决碳酸钙结垢问题,本文以华北保定岩溶地热井结垢为研究对象,通过理论和实验相结合的手段研究分析了垢质成分,成垢机理,结垢位置和过程以及防垢措施。研究结果表明:(1)系统降压造成的闪蒸是碳酸钙结垢的主因,液相二氧化碳逸出到气相是碳酸钙结垢的主要驱动力;(2)根据井口参数,结合质量、动量和能量守恒以及两相流压降理论,可以模拟结垢过程,确定结垢位置以及不同深度处的压力、温度、干度和二氧化碳分压等参数;(3)闪蒸造成的碳酸钙结垢,确定了闪蒸位置和闪蒸压力后,可以通过加压和加注阻垢剂的方式进行阻垢。通过模拟计算,确定了加压防垢系统所需的最低压力,通过控制系统压力可防止闪蒸,抑制二氧化碳逸出造成的结垢。设计了阻垢工艺,研制了阻垢剂加注设备,开展了井下化学阻垢实验并评价了阻垢效果,通过加注阻垢剂可有效阻止90%以上的垢生成,论证了通过加注化学阻垢剂可以有效解决碳酸钙结垢。通过上述研究,积累了从结垢原因分析,结垢位置确定,结垢过程模拟,防垢工艺和设备研发,防垢实践到阻垢效果现场评价一整套经验,可为其他地热井碳酸钙结垢问题的解决提供参考依据。     

Full scale decay test of a tanker: field data and theoretical analysis

This paper presents results from a full scale decay test made with a tanker in a relatively protected area in the Brazilian coast. In at least two tests the environmental loads (wind, waves and current) were very small and the time history of the surge motion was well behaved, making it possible to check some proposed models for the damping in the hull and mooring lines. Field data seem to confirm that the damping is indeed of the fluid viscosity type and the theoretical models are able to recover roughly 75% of the observed damping, the energy dissipation in the mooring lines being, by far, the major contribution. The remaining 25% are likely due to non modeled effects, such as the environment influence, which although small and not measured certainly exists, and to the friction between the mooring lines and the seabed.     

Molecular analysis of the commercial deep-sea crabs Chaceon ramosae and Chaceon notialis (Brachyura,Geryonidae) reveals possible cryptic species in the South Atlantic

Deep-sea red crabs Chaceon ramosae and Chaceon notialis are commercially and ecologically important crustaceans in South Atlantic waters. With some overlapping occurring at the edge of the crabs’ distribution, the fisheries are managed separately in Brazil and Uruguay, with some differences in the regulations, although the stock is supposedly shared between the two countries. To assess genetic information on these two species, we examined the nucleotide sequence of the mitochondrial 16S rDNA and CO1 mtDNA genes in samples from the southern region. We also compared these data to sequences from other congeners. The genetic analysis revealed a clear separation between C. notialis and C. ramosae. In addition, we detected the existence of at least two different groups within the species that is currently recognized as C. notialis. This might indicate the existence of cryptic species, leading us to speculate about the presence of two different taxonomic entities, although further research is needed to resolve this issue.     

港口及临港工业围填海规模综合评价研究

针对港口及临港工业围填海的特点,运用多目标决策理论与方法,构建了港口及临港工业围填海规模评价指标体系,包括现状评定和综合影响两类评价因子,包含自然条件、社会经济条件、资源环境影响、效益评估四类评价要素,共计15个评价指标。并根据成本型、效益型和固定型指标的特点提出了各自的标准化方法,采用主客观综合赋权法确定评价因子的权重,采用线性加权和法计算港口及临港工业围填海规模方案的综合得分,以此为依据确定围填海规模的适宜程度和适宜等级。以江苏辐射沙洲半岛式浅滩腰沙为例,运用港口及临港工业围填海规模综合评价方法,确定腰沙海域最佳的港口及临港工业围填海规模为理论基面+3.0 m。提出的研究方法能够为沿海省市港口及临港工业围填海规模评价提供参考和方法借鉴,对于围填海规模决策和围填海总量控制指标的制定具有重要意义。     

考虑空间相关尺度特征的细观力学模型及其应用

天然岩石材料内部存在各种缺陷,在微、细观尺度表现出高度的非均质特性。基于连续介质力学框架,采用非线性标量损伤本构关系描述岩石材料的变形与破坏行为,建立了岩石细观损伤本构模型,并在常规Weibull随机分布模型基础上,引入空间相关尺度因子以模拟实际岩石材料各项物理力学指标具有的空间相关特征。选取典型岩石单轴拉伸试验算例,分析随机场内空间相关尺度因子的变化对试样荷载-加口张开度关系曲线以及破坏行为的影响。结果表明,考虑岩石材料各项物理力学指标的空间相关尺度特征对评价其力学指标的离散性以及破坏形态特征有着较显著的影响。     

一个简单陆气耦合模式中的绿洲-荒漠化效应

发展了一个简单的地气相互作用模式 ,讨论了不同气候和植被条件对绿洲消长的影响。结果表明 ,能使绿洲扩大的主要条件是低纬度、小尺度 ,并具有低水汽、较高温度的环境以及较小气孔阻力的植被。这一简单的理论分析对发展复杂的数值模式和对观测的布局有参考意义 ,对治理荒漠也有一定的启示。     

基于逆散射理论的介质参数与其地震响应的尺度对应关系研究

在反演过程中进行频带控制是多尺度反演的重要策略,但数据频率成分与要反演的参数之间的尺度对应关系尚不清晰。本文利用Kormendi论文中的测井曲线模型,基于逆散射理论将地下介质参数的扰动分解为0-0-9-11 Hz、9-11-18-22 Hz、18-22-36-44 Hz和36-44-80-90 Hz共4个尺度,并利用反射率正演模拟方法生成4个尺度扰动成分的地震响应。通过对比地下介质参数不同尺度的扰动及其地震响应的频带成分,发现二者在4个扰动尺度上均具有一致性,由此得出介质参数与其地震响应具有定量尺度对应关系的结论。据此从介质扰动的尺度概念引申出反射系数的尺度概念,从逆散射理论角度探讨实验结果的理论依据,并对其在指导反演分频参数选取及薄互层解释等方面的应用展望进行讨论。     

Cepheid parallaxes and the Hubble constant

Revised Hipparcos parallaxes for classical Cepheids are analysed together with 10 Hubble Space Telescope ( HST )-based parallaxes. In a reddening-free V , I relation we find that the coefficient of log  P is the same within the uncertainties in our Galaxy as in the Large Magellanic Cloud (LMC), contrary to some previous suggestions. Cepheids in the inner region of NGC 4258 with near solar metallicities confirm this result. We obtain a zero-point for the reddening-free relation and apply it to the Cepheids in galaxies used by Sandage et al. to calibrate the absolute magnitudes of Type Ia supernova (SNIa) and to derive the Hubble constant. We revise their result for H ₀ from 62 to 70 ± 5 km s⁻¹ Mpc⁻¹. The Freedman et al. value is revised from 72 to 76 ± 8 km s⁻¹ Mpc⁻¹. These results are insensitive to Cepheid metallicity corrections. The Cepheids in the inner region of NGC 4258 yield a modulus of 29.22 ± 0.03 (int.) compared with a maser-based modulus of 29.29 ± 0.15. Distance moduli for the LMC, uncorrected for any metallicity effects, are 18.52 ± 0.03 from a reddening-free relation in V , I ; 18.47 ± 0.03 from a period–luminosity relation at K ; 18.45 ± 0.04 from a period–luminosity–colour relation in J , K . Adopting a metallicity correction in V , I from Macri et al. leads to a true LMC modulus of 18.39 ± 0.05.     

The Cepheid period–luminosity zero-point from radial velocities and Hipparcos proper motions

A value for the zero-point (ρ) of the Cepheid period–luminosity relation, <  M _V  >= 2.81 log P  + ρ, is deduced by comparing the value of the Oort constant, A , derived from radial velocities with that derived from Hipparcos proper motions. We find in this way that ρ =−1.47 ± 0.13, in excellent agreement with the value derived from Hipparcos trigonometrical parallaxes, ρ = −1.43 ± 0.10, by Feast &38; Catchpole in a recent paper.