西太平洋暖池研究综述

西太平洋暖池（Western Pacific Warm Pool）是全球海温最高的海域,汇聚了巨大的热能,在地球气候系统中具有非常重要的作用。本文综述了近30年来有关西太平洋暖池的研究进展,包括西太平洋暖池的维持机制、在不同时间尺度西太平洋暖池的变异特征和物理机制,以及西太平洋暖池的观测和数值模拟等领域的研究进展。西太平洋暖池的维持是现有地形下大气过程和海洋过程相互作用导致的,在季节内到世纪尺度均存在很强的变化。其中：季节内变化的驱动机制主要包括与大气季节内振荡(Madden Julian Oscillation)相关的对流和海表面热通量变化,以及海洋波动等海洋动力过程;季节变化主要是太阳辐射的季节变化导致;在年际尺度上,西太平洋暖池作为El Ni?o-Southern Oscillation的一部分而振荡具有显著年际变化;太平洋代际振荡（Pacific Decadal Oscillation）和大西洋代际振荡（Atlantic Multi-decadal Oscillation）驱动着西太平洋暖池的年代际变化;世纪尺度的变化显示全球变暖背景下西太平洋暖池存在扩张趋势。人类对西太平洋暖池的系统观测始于海洋观测卫星的使用,随后历经WCRP/TOGA、TAO/TRITON、TOGA-COARE、WOCE、Argo、SPICE、NPOCE等多个观测计划,极大促进了西太平洋暖池的研究。但截止到第五次耦合模式比对计划（Coupled Model Intercomparison Project 5）,多数气候模式仍未能克服热带模拟偏差,对西太平洋暖池的模拟效果较差,表明在西太平洋暖池动力学的理解和模拟方面仍有较大进步空间。     

岬湾海滩剖面中长期变化特征及其控制因素——以青岛石老人海滩为例

了解海滩剖面变化可以更好地理解海滩动态过程。利用2007年5月~2014年12月近8 a青岛石老人海滩剖面的实测资料,计算剖面各段单宽体积变化量及后滨宽度,结合交叉小波和小波相干分析方法,探讨海滩剖面中长期淤蚀变化特征及其控制因素。结果表明,近8 a来海滩剖面表现为侵蚀状态,不同岸段侵蚀程度不同。剖面1岸段侵蚀明显,剖面2和剖面3岸段轻微侵蚀。剖面的变化过程可划分为平稳期、剧变期和微调期3个时期。各时期剖面的季节性变化较复杂,平稳期具冬蚀夏淤的交替变化特征,整体淤蚀量较小;剧变期剖面呈阶段性蚀退,变化幅度相对较大,微调期剖面可能仍处于剧变期的恢复阶段,季节性变化不明显。剧变期和微调期的小波交叉谱和相干谱分析显示,波浪和前滨单宽体积相干性较好,尤其当大于2 m的波高达到10%以上,海滩地形可以和波高变化产生同周期的变化。因此波高变化基本控制了剖面的季节变化。而海滩长周期变化主要受控于风暴潮作用及其漫长的恢复期,沿岸输沙和海平面变化则一定程度上导致了剖面长期侵蚀格局的形成。     

西太平洋雅浦海沟区海底热流原位测量

为了解西太平洋雅浦海沟区俯冲带及岛弧两侧的海底热流分布情况,2015年1-3月期间的西太平洋海山航次中,"科学"号利用最新一代Lister型热流探针对该区域开展了海底热流原位测量工作。沿着横跨俯冲带的站位测线,本次进行了10个热流站位测量,共获得8个站位的有效数据。测量结果表明,该地区地温梯度的变化范围为0.011~0.137 Km-1,平均0.089 Km-1,热导率的变化范围为0.58~1.32 Wm-1K-1,热流值则在14.4~118.85 mWm-2之间,平均为68.02 mWm-2。热流值分布显示,雅浦岛弧附近具有较高的热流值,自雅浦岛弧向两侧热流值逐渐降低,低热流区主要分布在帕里西维拉海盆。由于该地区热流测量数据依然稀缺,深入的讨论有待进一步研究。     

Tectono-sedimentary control on modern sand deposition on the forebulge of the Western Taiwan Foreland Basin

Whether the formation of the isolated sand body deposition in the forebulge area of a foreland basin system is structure- or deposition-controlled has puzzled geologists for decades, although sand body deposition is generally believed to be indicative of the position of the flexural forebulge in a foreland basin. The formation of a modern sand body in the forebulge area is thus examined by multi-scale geophysical observations based on combined reflection seismic profiles and compressed high-intensity radar pulse (CHIRP) profiles across the sand deposition along the forebulge of the Western Taiwan Foreland Basin (WTFB), which is a Late Miocene-present foreland basin in the overfilled stage. These profiles suggest that the accumulation of the sand deposits along the forebulge of the WTFB is not directly associated with forebulge faultings. The relief map of the forebulge deposit substratum shows a northwestward tilting slope, and the isopach of the forebulge sand body indicates that a large part of the sand body accumulated along the axis of the Taiwan Strait and the subdued forebulge of the WTFB. The difference between the prevailing directions of tidal currents between the Taiwan Strait and the East China Sea reflects the probable sedimentary influence of the cratonward migrating fold-thrust belt within a foreland shelf. We suggest that the formation and distribution of the sand deposits along the forebulge of the WTFB are generally controlled not only by the transverse downslope sedimentation but also longitudinal hydrodynamic processes at distal parts of the foreland basin. Our explanation provides a plausible tectono-sedimentary cause of the sand body deposition in the forebulge area in an overfilled foreland basin. The sedimentary dynamics of the sand body in the Taiwan Strait may be applicable for understanding the formation of isolated sand bodies in the distal part of the Cretaceous Western Interior Foreland Basin.     

南水北调西线雅砻江调水工程温波引水枢纽坝址径流计算的研究

南水北调西线雅砻江调水工程（简称西线调水）是从长江的一级支流雅砻江上游区引水至黄河源头地区的跨流域调水工程，是补充黄河水资源不足与解决我国西北和华北部分地区干旱缺水的重大战略措施，由于引水枢纽坝址缺乏实测水文资料，我们依据附近孜水文站实测资料，采用一些非确定性的数理统计模型来计算温波引水坝址的设计年径流量，并对计算成果进行了合理性分析，结果表明，上述计算成果基本反映了温波引水坝址径流变化的客观情况，从而为南水北调西线雅砻江调水工程缺乏实测水文资料地区的水文计算提供了科学依据。     

中国东部第四纪自然环境演化及庐山“冰碛层”堆积时期的自然环境研究

根据第四纪地层内孢粉组合和动物群等新资料恢复了我国东部各大区域第四纪各个时期的自然环境特征,其温暖期与干冷期的交替与深海沉积O~(18)温度变化趋势大致对应。庐山三次“冰期冰碛层”内孢粉组合表明均为温暖湿润针阔叶混交林景观,而不是寒冷的冰川环境。     

ON THE CHARACTERISTICS OF NON-LINEAR SOIL RESPONSE AND DYNAMIC SOIL PROPERTIES USING VERTICAL ARRAY DATA IN JAPAN

Non-linear response of the soil is investigated by comparing the spectral ratios (uphole/downhole) using weak and strong motions. Data from seven vertical arrays in Japan are analysed in this study. The frequency-dependent transfer function of soil is calculated as a ratio of the spectrum at uphole to the spectrum at downhole, considering the horizontal component of shear wave. In spectral ratio analysis auto- and cross-spectra are employed. The reduction in the predominant frequency of the transfer function with increases in excitation level reflects the non-linear response of the soil. Results of analysis demonstrate a significant non-linear ground response at six sites with surface PGA exceeding 90 gal. However, the results of one site show the linear response up to 130 gal surface PGA. Furthermore, the in situ strain-dependent soil behaviour is examined through the shear modulus – shear strain relationship. When compared, the actual and laboratory results of the shear strain – shear modulus relationship are in agreement. Additionally, a good consistency between the tendency of reduction in shear modulus ratio with shear strain increases, and reduction of predominant frequency with ground motion increases, confirms the significance of non-linearity in site effects study.     

近50年火山喷发和太阳活动对我国气候影响的研究

利用特征向量分析与时序叠加分析和谱分析相结合的方法，分析了近50a来我国地面气温和降水场中火山喷发和太阳活动的气候信号，强烈的火山喷发导致全国大部分地区降温，喷发1a多以后降温最明显，并能持续约半年。除这个主信号以外，青藏高原、东南沿海和东北地区都可能出现较为复杂的温度变化，温度变化与太阳活动之间的联系更多地反映在二者的振荡关系上。在降水场中的火山信号较弱，表现为火山喷发后的秋冬季节南方地区降水偏多。在青藏高原积雪和深层地温的变化中，没有发现火山和太阳活动信号。     

云南省潜在震源区综合统计判定之一

本文将云南省地震局多年来积累的关于中强震发生的地质构造、地貌、地球物理场、地形变等特征基础资料,用于Cora-3算法的模式识别,得出云南省潜在震源区的背景指标,结果是比较理想的。“投票”结果表明,80%的学习集D类对象仍被识别为D类,85%的学习集N类对象仍被识别为N类,控制试验的结果也表明识别结果是比较稳定和可靠的。     

Invariant Tori in the Secular Motions of the Three-body Planetary Systems

We consider the problem of the applicability of KAM theorem to a realistic problem of three bodies. In the framework of the averaged dynamics over the fast angles for the Sun–Jupiter–Saturn system we can prove the perpetual stability of the orbit. The proof is based on semi-numerical algorithms requiring both explicit algebraic manipulations of series and analytical estimates. The proof is made rigorous by using interval arithmetics in order to control the numerical errors.