Spatial and temporal variability of crustal magnetization of a slowly spreading ridge: Mid-Atlantic Ridge (20°–24° N)

The results of the two- and three-dimensional magnetic inversions performed on data located between 20°–24° N on the Mid-Atlantic Ridge indicate the crustal magnetization has decayed exponentially for the last 10 Ma, and that this decay has been fairly symmetric about the ridge axis. After removal of the mean temporal decay, the residual field is characterized by more positive magnetizations at the second-order discontinuities, regardless of initial magnetization direction. A model that involves the preferential emplacement of serpentinized lithologies near the discontinuities is proposed to explain this correlation. The temporal detrending method also indicates that several ridge-parallel depressions located on the flanks of the ridge axis are regions of more positive magnetizations. These bathymetric depressions may mark the locations of detachment faulting that occurred during amagmatic periods of extension. The general symmetry of the crustal magnetization about the ridge axis does not support the occurrence of continuous detachment faulting proposed to correspond to the inner and outer corners of ridge axis discontinuities.     

A rifted inside corner massif on the Mid-Atlantic Ridge at 5°S

The structure of the Mid-Atlantic Ridge at 5°S was investigated during a recent cruise with the FS Meteor. A major dextral transform fault (hereafter the 5°S FZ) offsets the ridge left-laterally by 80 km. Just south of the transform and to the west of the median valley, the inside corner (IC – the region bounded by the ridge and the active transform) is marked by a major massif, characterized by a corrugated upper surface. Fossil IC massifs can also be identified further to the west. Unusually, a massif almost as high as the IC massif also characterizes the outside corner (OC) south of the inactive fracture zone and to the east of the median valley. This OC massif has axis-parallel dimensions identical to the IC massif and both are bounded on their sides closest to the spreading axis by abrupt, steep slopes. An axial volcanic ridge is well developed in the median valley both south of the IC/OC massifs and in an abandoned rift valley to the east of the OC massif, but is absent along the new ridge-axis segment between the IC and OC massifs. Wide-angle seismic data show that between the massifs, the crust of the median valley thins markedly towards the FZ. These observations are consistent with the formation of the OC massif by the rifting of an IC core complex and the development of a new spreading centre between the IC and OC massifs. The split IC massif presents an opportunity to study the internal structure of the footwall of a detachment fault, from the corrugated fault surface to deeper beneath the fault, without recourse to drilling. Preliminary dredging recovered gabbros from the scarp slope of the rifted IC massif, and serpentinites and gabbros from the intersection of this scarp with the corrugated surface. This is compatible with a concentration of serpentinites along the detachment surface, even where the massif internally is largely plutonic in nature.     

中国东部中新生代盆地成因及其地球动力学

中国东部大兴安岭－太行山－武陵山重力梯度带一线以东至太平洋西岩，大陆连缘中新生代盆地系的形成，中生代岩浆活动，盆地基本特征同Ｍｏｈｏ、岩石圈和软流圈及上地幔基本特征的内在联系等都表明，它们在时空和成因上有一定联系，可以纳入同一地球动力学过程之中，这种动力学机制可能与岩石圈界，地壳底界的拆离作用有关。     

Seismic reflection imaging of an oceanic detachment fault: Atlantis megamullion (Mid-Atlantic Ridge, 30°10′N)

We present multichannel seismic reflection data collected over the Atlantis megamullion, at the eastern ridge-transform intersection of Atlantis fracture zone on the northern Mid-Atlantic Ridge, and over its conjugate crust. These data image for the first time the internal structure of a young, well-developed megamullion dome formed by tectonic extension across a long-lived oceanic detachment fault. The exposed, corrugated detachment-fault surface exhibits a sharp, coherent reflection that contrasts with less organized reflectivity of surrounding basaltic seafloor. At the termination of the megamullion the fault is imaged ∼13 km along-strike beneath a volcanic hanging-wall block at a sub-seafloor depth of 0.2-0.5 s two-way travel time, reaching north as far as 30°19′N. The eastward dipping of the fault beneath the hanging-wall block is estimated to be ∼6-14°. The corrugated fault surface is underlain by a continuous, strong, and relatively smooth reflection (D) at 0.2-0.25 s sub-bottom below the central axis of the dome. This reflection deepens up to 0.6 s sub-bottom beneath the western slope and it appears to intersect the seafloor on the eastern slope. We suggest that Atlantis massif formed by sequential slip on two different detachment faults that merged at depth, with breakaways as little as ∼2 km apart. The initial detachment is represented by reflection D, and the second corresponds to the presently exposed fault surface. In this interpretation, much of the sliver between the faults is interpreted to be strongly serpentinized peridotite with reduced seismic velocity; it lies in contact with less altered, higher-velocity mantle below the first detachment, resulting in the strong, smooth character of reflection D. Mantle rocks exposed in the megamullion indicate that the feature formed during a period of extreme tectonic extension and probably limited magmatism. In conjugate crust corresponding to termination of the megamullion, observed sub-bottom reflections are interpreted as base of seismic layer 2A. This layer is as thick as or thicker (∼570-900 m) than layer 2A in normal Atlantic crust, and it suggests that relatively normal crustal accretion occurred by the time the megamullion stopped forming.     

Crater formation in soils by raindrop impact

The process of crater formation by the impact of water drops on soil, sand and various other target material was studied. Craters of various shapes and sizes were observed on different target materials or conditions, ranging from circumferential depression to completely hemispherical shape. Crater shape was dependent upon target material, its ?ow stress or shear strength and the presence and thickness of water on the surface. Between 5 and 22 per cent of impact energy was spent on cratering, but the relationship between crater volume and kinetic energy of a raindrop was curvilinear, indicating a lower ef?ciency of impact energy in removing target material as the energy increases. Impact impulse, on the other hand, showed a more linear relationship with crater volume, and the ratio of impulse over crater volume (I/V) remained constant for the entire range of drop sizes, impact velocities, and surface conditions used in this study. Surface shear strength, represented by the penetration depth of fall‐cone penetrometer, appeared to be a key factor involved in this process. An equation was developed which related crater volume to cone penetration depth and impact impulse. Crater volume, which appeared to be a better indicator of the total amount of material dislodged by a raindrop than splash amount, can thus be predicted using this equation. Copyright © 2004 John Wiley & Sons, Ltd.     

东北帕米尔中新世中下地壳物质的折返过程：公格尔西滑脱剪切带的构造变形与年代学证据

公格尔西滑脱剪切带位于东北帕米尔公格尔片麻岩穹窿西缘。通过我们详细的野外观测、显微构造观察、石英电子背散射衍射(EBSD)测试以及锆石U-Pb测年,对公格尔西滑脱剪切带的几何学、运动学特征及其形成演化时限进行了研究。公格尔西滑脱剪切带糜棱岩中大量的石榴子石、矽线石和蓝晶石等表明其为高级变质产物。S/C组构、旋转碎斑及不对称褶皱等变形现象说明剪切带上盘向W或SW低角度剪切的运动特征。高级变质糜棱岩和浅色岩脉记录约20 Ma的206 U-238Pb锆石年龄,说明公格尔西滑脱剪切带初始形成于早中新世。结合前人研究成果,我们认为公格尔西滑脱剪切带曾是狭长的帕米尔中下地壳滑脱带的最北段。由于新生代印度亚洲大陆碰撞以后印度板块仍持续向N俯冲推进,帕米尔地壳由S向N开始增厚,进变质作用最初发生于南帕米尔,约20 Ma时到达北帕米尔。东北帕米尔中下地壳物质开始折返于中新世中期。而直到6~4 Ma,东北帕米尔公格尔地区开始快速隆起,此时公格尔新生代高级变质岩才快速折返。     

西藏南羌塘增生杂岩中俯冲反向驱动高压变质岩折返:来自猫耳山大型拆离断层的启示

大洋岩石圈俯冲增生过程中可能伴随着复杂的深部板片运动过程。高压变质岩无疑是记录这些深部过程的良好载体。最近的研究提出,在特定情况下,双向俯冲中占主导的俯冲板块拖曳另一侧板块发生反向运动,从而短板片可能被另一侧长板片拖出。该研究提示我们关注俯冲增生过程中这种可能的“不正常”的板片运动方式,从而客观而全面地剖析碰撞造山带。现有高压变质岩折返模式中,除了俯冲隧道流模式,其余模式均强调单次快速折返。然而,俯冲反向运动导致的折返过程有所不同:对单个高压变质岩来说仍是快速折返,但是对整体高压变质岩带来说,整个俯冲反向期间必然都存在高压变质岩折返,从而形成较长的折返过程持续时间。对上地壳层次的折返相关构造变形的研究有助于揭示上述过程。     

两次强降水过程雨滴谱特征及差异

利用寿县观测站内的Parsivel激光雨滴谱仪结合观测站雨量数据及雷达基数据,分析了发生在2015年6月26—30日梅雨期间和2015年8月7—10日超强台风"苏迪罗"影响期间2次强降水过程的雨滴谱结构特征及其差异,拟合了雨强与雷达反射率因子之间的关系。结果表明:雨强的大小直接影响雨滴谱的特征参量,且随着雨强增大而增大;梅雨锋暴雨中1.0mm直径≤1.5mm的粒子所占比例最多,雨强贡献率最大;台风雨中0.75mm直径≤1.0mm的粒子所占比例最多,但1.0mm直径≤1.25mm的粒子对雨强的贡献最大,说明较大粒子对强降水的贡献较大。     

一次拖曳型飑线过程雨滴谱演变特征研究

利用Thies激光雨滴谱仪观测资料和CINRAD/SA多普勒雷达观测资料,分析了2017年7月18日一次典型中纬度拖曳型飑线过程不同发展阶段雨滴谱和积分参数的演变特征,主要结果为：1）成熟飑线回波包括对流带、过渡区和拖曳层状云区三部分,对流带前侧不断有对流带生成并合并到主对流带中,使得对流带的前沿具有强的反射率因子,并且有多个雨强大值中心。2）垂直穿过飑线对流带,雨强增加阶段有较少的小粒子（直径小于1 mm）和特大粒子（直径大于5 mm）,以及较低的雨滴浓度和反射率因子,而雨强减弱阶段有较多的小粒子和特大粒子,以及较高的雨滴浓度和反射率因子;飑线加强阶段,雨滴谱有较大的峰值直径（0.44 mm）、较多的大（直径大于3 mm）和特大粒子,而飑线减弱阶段,雨滴谱有较小的峰值直径（0.19 mm）、较少的大粒子。3）对流带、过渡区和层状云降水雨滴谱的Gamma谱三参数N0、μ、λ随雨强增大有明显的分层特征,相同雨强时,对流云和过渡区降水的三参数比层状云降水的数值大;而飑线不同发展阶段、不同降水类型的λ-μ关系具有一致性,二次多项式可以很好地拟合λ-μ关系。4）归一化雨滴谱参数NW和D0的分布可以用来区分对流云和层状云降水,并给出了新的分离线方程;另外,飑线在发展和减弱阶段的雨滴谱特征有明显差异,表明飑线演变过程降水形成的微物理机制发生变化,前期冷云过程有重要影响,而后期暖云过程起主导作用。     

降水现象仪观测应用评估

利用2017年9月至2018年8月北京20个站降水现象仪采集数据与人工平行观测数据,对降水现象仪进行了对比评估。结果表明:降水现象仪的缺测率为0.01%,空报率为0.6%,捕获率为93.5%,漏报率为27.9%,错报率为10.0%。从统计结果可知,降水现象仪的缺测率、空报率较低,捕获率较高,体现出设备性能良好的一面,漏报率和错报率偏高,表明设备漏识别和错误识别的情况较多,漏报主要发生在弱降水过程中,错报主要出现在毛毛雨的识别上。设备测量和人工观测降水开始时间一致性较好,终止时间一致性偏差;降水现象仪现存问题:在大雨强时易出现雨滴叠加误识别,在小雨强时识别率会降低,在无降水错误输出降水现象方面缺少质控。