白令海北部陆坡晚第四纪的古海洋与古气候学记录

白令海北部陆坡B2 9柱状样中放射虫Cycladophoradavisiana含量曲线和深海SPECMAP氧同位素记录的对比 ,为该柱状样建立了晚第四纪约 1 0万年以来的地层年代框架。该柱状样中微体化石、碳屑颗粒、筏冰碎屑 (石英和岩屑颗粒 )的定量分析结果表明 ,作为表层生产力指标的粗组份自氧同位素 5 .3期以来呈阶梯状增加 ,反映表层生产力阶段式的增长 ;碳屑颗粒丰度自氧同位素 5 .3期至末次冰消期的增加说明白令海末次冰消期以前气候较全新世干冷 ,天然火灾发生的概率较全新世大大增加 ;冰期和早、中全新世较高的筏冰碎屑反映了冰期和早、中全新世白令海陆架海冰的扩大以及气候转暖所导致的海冰消融的过程 ,揭示了白令海对过去全球气候变化的响应。     

火山岩熔融,结晶,淬火实验及其岩石学意义

本文对我国福建，江西，河南等地某些典型玄武岩和部分安山岩以及意大利威苏维火山的白响岩质碱玄岩进行了实验研究，其中包括熔融，结晶，淬火实验。根据实验结果，分析了熔浆成分对首晶矿物的影响，阐明了晶体形态与结晶温度，生长速度及成核密度的关系，研究了斜长石，白榴石的晶出及其矿物学，岩石学意义，论述了橄榄石，辉石的成分特生上春晶出后熔浆成分的演化趋势，讨论了单斜辉石的淬火效应与压力效应。     

Analysis of buried pipelines subjected to reverse fault motion

Presently available simplified analytical methods and semi-empirical methods for the analysis of buried pipelines subjected to fault motion are suitable only for the strike-slip and the normal-slip type fault motions, and cannot be used for the reverse fault crossing case. A simple finite element model, which uses beam elements for the pipeline and discrete nonlinear springs for the soil, has been proposed to analyse buried pipeline subjected to reverse fault motion. The material nonlinearities associated with pipe-material and soil, and geometric nonlinearity associated with large deformations were incorporated in the analysis. Complex reverse fault motion was simulated using suitable constraints between pipe-nodes and ground ends of the soil spring. Results of the parametric study suggest that the pipeline's capacity to accommodate reverse fault offset can be increased significantly by choosing a near-parallel orientation in plan with respect to the fault line. Further improvement in the response of the pipeline is possible by adopting loose backfill, smooth and hard surface coating, and shallow burial depth in the fault crossing region. For normal or near normal orientations, pipeline is expected to fail due to beam buckling at very small fault offsets.     

Composition and Useful Properties of Tailings of Marine Manganese Nodules and Crusts

Marine manganese nodules and crusts, when processed, yield tailings which may be utilized for environmental and economic benefit. The key to the reasonable and effective utilization of these tailings lies in making a systematic appraisal of their composition and properties. This article gives an introduction to the investigation of manganese tailings properties. The tailings have a high iron and/or manganese content, high surface area, high porosity, and fine grain size. Some tailings have a high rare earth element content which is valuable. They may also have high SO₃, arsenic, and uranium contents which are harmful. Depending on the process used to produce the tailings, there will likely be some differences in chemical composition, mineral assemblages, surface area and adsorption capability, pore diameter and volume, density and pH. In assigning potentially beneficial applications for these tailings, these differences should be taken into account to optimize utilization.     

Acoustic Mode Frequencies of the Sun During the Minimum Phase Between Solar Cycles 23 and 24

We investigate the spatial and temporal variations of the high-degree mode frequencies calculated over localized regions of the Sun during the extended minimum phase between solar cycles 23 and 24. The frequency shifts measured relative to the spatial average over the solar disk indicate that the correlation between the frequency shift and magnetic field strength during the low-activity phase is weak. The disk-averaged frequency shifts computed relative to a minimal activity period also reveal a moderate correlation with different activity indices, with a maximum linear correlation of about 72?%. From the investigation of the frequency shifts at different latitudinal bands, we do not find a consensus period for the onset of solar cycle 24. The frequency shifts corresponding to most of the latitudes in the northern hemisphere and 30° south of the equator indicate the minimum epoch to be February 2008, which is earlier than inferred from solar activity indices.     

初值及物理过程对\

利用国防科技大学全球中期数值天气预报模式（YinHe Global Spetral model,YHGS）产品驱动WRF对2018年7月4日华中地区暴雨过程进行模拟,并与ERA-interim资料作初始场模拟结果对比,评估YHGS模式产品在此次暴雨过程预报中的应用能力。结果表明：（1）WRF-YHGS对2018年7月4日华中地区暴雨过程有一定的预报能力,其模拟的大尺度环流形势、水汽收支量变化趋势与WRF-ERA有着很好的一致性,YHGS模式产品驱动中尺度数值预报是可行的。（2）WRF-YHGS模拟效果较WRF-ERA差,但大雨量级WRF-ERA湿偏差较大,两组试验各物理量模拟结果存在一定差距,且随着积分时间的增加差异逐渐增大。（3）WRF-YHGS、WRF-ERA模拟结果的差异主要来自YHGS与ERA初始场中差异较大的次天气尺度运动和YHGS全球模式预报场误差两个方面。

     

乌东德水电站开建以来坝区暴雨的统计研究

对乌东德水电站开建以来坝区暴雨及伴随的短时强降水时空分布进行统计研究,并划分出暴雨天气概念模型。结果表明:乌东德水电站开建以来坝区共出现18个暴雨日,平均3.0个/a,暴雨自6月上旬开始出现,到10月上旬结束,出现暴雨最多的季节是夏季,多为范围小的局地性暴雨出现。暴雨日数、年平均降水量、20~30mm h^-1及≥20mm h^-1的短时强降水的空间分布均呈现“西北多东南少”的特征。20~30mm h^-1的短时强降水发生频次最多(占63.6%),其次为30~40mmh^-1(占27.3%),40~50mm h^-1最少(仅占9.1%)。短时强降水及不同等级短时强降水均表现为夜间高发、白天低发的日变化特征。总结归纳出切变冷锋型8次(占44.4%)、两高辐合型4次(占22.2%)、西南涡型2次(占11.1%)、孟加拉湾风暴型2次(占11.1%)、切变线型1次(占5.6%)和高空槽型1次(占5.6%)六类暴雨天气概念模型。     

2011—2012年广州高建筑物雷电磁场特征统计

为研究不同高度的建筑物对雷电磁场的影响,对2011年7月—2012年8月广州高建筑物雷电观测试验中获取的雷电磁场波形数据进行统计分析,共选取击中14个高建筑物的40次雷电 (均为负极性雷电) 的磁场数据,结果表明：高建筑物对回击磁场峰值有增强作用,且建筑物越高对回击磁场峰值的增强作用越大,高度在200 m以上的建筑物上雷电首次回击磁场峰值的几何平均值是高度在200 m以下的建筑物上的2.4倍;高建筑物雷电回击的磁场波形呈多峰特征;观测到的20次击中200 m以下高建筑物的雷电中,有13次 (65%) 雷电首次回击的磁场波形出现后续峰值比初始峰值大的现象,击中200 m以上高建筑物的14次雷电中有8次 (57%) 出现该现象;40次高建筑物雷电中有22次 (55%) 为多回击雷电,135个回击间隔时间的几何平均值为69.1 ms, 多回击高建筑物雷电中有10次 (45%) 出现继后回击的磁场峰值大于首次回击磁场峰值的现象。