青藏及华北阵列式区域大地电磁场标准观测网建设方法与实验

大地电磁参数标准网的建设需要大量第一手的观测资料,观测资料的质量直接决定了标准网的可靠性。本文分析了大地电磁测深仪器设备、资料采集与处理技术,确定了青藏及华北阵列式区域大地电磁场标准观测网的建设方法;在此基础上,在山东菏泽地区对11535和11635号标准点进行了野外观测试验,对采集的宽频及长周期数据进行了深入处理,形成的对辅助测站和中心测站布置、数据采集时间、资料处理手段和远参考测站布设等要求,将指导青藏及华北阵列式区域大地电磁场标准网的建设,并对中国大陆其他区域大地电磁场标准网建设具有一定参考意义。     

青藏高原东北缘寺口子盆地新生代沉积演化及其构造意义

宁夏固原寺口子盆地发育巨厚的新生代地层,这些地层记录了青藏高原东北部的沉积演化特征和构造演变历史。根据剖面沉积物粒度特征、沉积结构和构造、沉积层序,识别出20种岩相、5种沉积相类型。结合前人对寺口子剖面的古地磁测年,分析研究盆地的沉积演化特征以及对构造的响应表明:20.1 Ma盆地以缓慢的坳陷沉降开始演化,直至1.2 Ma遭受破坏。在此期间青藏高原东北部经历了6.4 Ma、4.6 Ma和1.2 Ma这3次明显的构造挤压隆升运动,其中约6.4 Ma的构造运动是青藏高原向东北部扩展首次影响到海原—六盘山断裂以东地区。从盆地的形成和沉积演化过程来看,马东山山前断裂的逆冲推覆,导致了寺口子盆地的强烈变形和构造降升,并且最终成为青藏高原的最新组成部分。     

High‐ to ultrahigh‐temperature metamorphism in the lower crust: An example resulting from Hikurangi Plateau collision and slab rollback in New Zealand

Lower crustal xenoliths erupted from an intraplate diatreme reveal that a portion of the New Zealand Gondwana margin experienced high‐temperature (HT) to ultrahigh‐temperature (UHT) granulite facies metamorphism just after flat slab subduction ceased at c. 110–105 Ma. P–T calculations for garnet–orthopyroxene‐bearing felsic granulite xenoliths indicate equilibration at ~815 to 910°C and 0.7 to 0.8 GPa, with garnet‐bearing mafic granulite xenoliths yielding at least 900°C. Supporting evidence for the attainment of HT and UHT conditions in felsic granulite comes from re‐integration of exsolution in feldspar (~900–950°C at 0.8 GPa), Ti‐in‐zircon thermometry on Y‐depleted overgrowths on detrital zircon grains (932°C ± 24°C at aTiO₂ = 0.8 ± 0.2), and correlation of observed assemblages and mineral compositions with thermodynamic modelling results (≥850°C at 0.7 to 0.8 GPa). The thin zircon overgrowths, which were mainly targeted by drilling through the cores of grains, yield a U–Pb pooled age of 91.7 ± 2.0 Ma. The cause of Late Cretaceous HT‐UHT metamorphism on the Zealandia Gondwana margin is attributed to collision and partial subduction of the buoyant oceanic Hikurangi Plateau in the Early Cretaceous. The halt of subduction caused the fore‐running shallowly dipping slab to rollback towards the trench position and permitted the upper mantle to rapidly increase the geothermal gradient through the base of the extending (former) accretionary prism. This sequence of events provides a mechanism for achieving regional HT–UHT conditions in the lower crust with little or no sign of this event at the surface.     

干旱灾害和我国西北干旱气候的研究进展及问题

首先阐述了自然灾害中干旱灾害的严重性和复杂性；接着从西北干旱气候的时空分布特征、形成原因、干旱气候的比较以及监测和预测等方面回顾了近20年来我国西北干旱气候研究的进展；最后提出了西北干旱气候待研究的问题。     

黄土湿陷性的微结构不平衡吸力成因论

分析了黄土粒间吸力的基本特性及其湿陷的微观过程,探讨了黄土在应力状态作用下由于浸水增湿而产生的微结构单元体滑移动力和阻力随饱和度、上覆土压力的变化规律,提出了微结构与广义吸力综合效应的湿陷性控制机理---微结构不平衡吸力成因论及其定量模型,从理论上分析了湿陷性与增湿水量、压力及深度的关系,揭示了土湿陷效应的内在规律。文中认为,湿陷过程就是水的楔入导致小孔隙广义吸力的逐渐丧失和大孔隙湿吸力的逐渐增大引起的微结构重建动力与重建阻力间的动态对抗过程。最后,讨论了湿陷的基本条件及影响因素。     

20世纪西北地区降水量变化特征

利用英国东安哥拉大学气候研究中心(CRU)的Hulme最新的1900-1998年的全球降水量资料,分析了20世纪西北地区降水量的变化特征.结果表明,20世纪西北地区降水量处于下降通道中,后期略有回升;西北地区东部和西部降水量的年代际变化有相反的趋势;20世纪后期西北地区中西部降水量有明显的增多趋势,东部降水量持续偏少,干旱连年发生.     

利用磷灰石裂变径迹对断层摩擦生热探测或测量的初步探讨

以青藏高原东北缘断裂带为研究对像,对利用磷灰石裂变径迹热年代学对地震断层滑动摩擦生热的探测或测量进行了初步探讨。其基本思路是利用磷灰石裂变径迹热年代计的热敏感,通过对横跨断层垂直方向断层岩和围岩的磷灰石裂变径迹年龄及围限径迹长度分布的对比分析,对断层滑动摩擦生热进行探测。本次研究对来自3个断层剖面的13个样品进行了磷灰石裂变径迹分析,样品包括断层主滑动面上的断层泥、碎裂岩和断层围岩,分析结果并没有获得断层摩擦生热的证据,表明这些断层在地震滑动过程中的摩擦增温非常有限,没有达到磷灰石裂变径迹热年代计体系可加载热信息的温度－时间要求。结合前人已有的相关研究,对利用磷灰石裂变径迹热年代学对地震断层滑动摩擦生热进行探测或测量存在的主要问题及可行性进行了初步总结和探讨,认为只适应于对震级大、断层滑动距离和速率大,摩擦强度强,位于一定深度有大量摩擦热生成,并使断层附近增温达到或超过磷灰石裂变径迹部分或完全退火温度的断层进行滑动摩擦生热的探测或测量,将是一种潜在的能对地震断层滑动摩擦生热或增温进行测量的“热量计或温度计”。     

北麓河多年冻土区降水及河水稳定同位素特征分析

为了进一步全面理解和探索青藏高原水文水循环过程,采用同位素方法并结合气象资料对青藏高原北麓河区域2011年6~12月降水和河水稳定同位素时空特征进行分析。探讨了北麓河降水同位素与日平均气温、降水量之间的相互关系,同时也对比分析了北麓河降水和河水的同位素变化特征。结果表明:北麓河降水同位素在整个观测期内总体受温度控制,但存在季节变化,其中6~9月降水同位素受到温度和降水量效应的共同控制,9月以后则主要受温度的影响。河水同位素与降水同位素相似的变化特征,体现了降水补给特征,另外降水量也能够影响河水同位素变化:降水量小则降水对其影响较小,反之则大。与北麓河降水线相比,河水δ18O~δD关系的斜率和截距偏大,揭示该区域河水除了受大气降水的补给外,还受到区域水体内循环和蒸发分馏作用的影响。     

Heating duration of igneous rim formation on a chondrule in the Northwest Africa 3118 CV3oxA carbonaceous chondrite inferred from micro-scale migration of the oxygen isotopes

Due to their common occurrence in various types of chondrites, igneous rims formed on pre-existing chondrules throughout chondrule-forming regions of the solar nebula. Although the peak temperatures are thought to reach similar values to those achieved during chondrule formation events, the heating duration in chondrule rim formation has not been well defined. We determined the two-dimensional chemical and oxygen isotopic distributions in an igneous rim of a chondrule within the Northwest Africa 3118 CV3_oxA chondrite with sub-micrometer resolution using secondary ion mass spectrometry and scanning electron microscopy. The igneous rim experienced aqueous alteration on the CV parent body. The aqueous alteration resulted in precipitation of the secondary FeO-rich olivine (Fa_40–49) and slightly disturbed the Fe-Mg distribution in the MgO-rich olivine phenocrysts (Fa_11–22) at about a 1 μm scale. However, no oxygen isotopic disturbances were observed at a scale greater than 100 nm. The MgO-rich olivine, a primary phase of igneous rim formation, has δ¹⁷O = −6 ± 3‰ and δ¹⁸O = −1 ± 4‰, and some grains contain extreme ¹⁶O-rich areas (δ¹⁷O, δ¹⁸O = ∼−30‰) nearly 10 μm across. We detected oxygen isotopic migration of approximately 1 μm at the boundaries of the extreme ¹⁶O-rich areas. Using oxygen self-diffusivity in olivine, the heating time of the igneous rim formation could have continued from several hours to several days at near liquidus temperatures (∼2000 K) in the solar nebula suggesting that the rim formed by a similar flash heating event that formed the chondrules.