白龙江下游涉核地区的放射性环境水平现状调查

通过对白龙江下游涉核地区及周边地区的汽车能谱测量和地面伽玛能谱测量以及空气中的氡浓度的监测,得出区内各地层中的U、Th、K含量均符合当地各地层的特性,与当地本底基本一致,空气氡浓度范围为183.9~305.8 Bq/m3,均属正常,符合当地的天然放射性环境情况,对环境无任何影响。     

青海德尔尼铜钴矿外围综合物探方法应用研究

在分析德尔尼矿区试验剖面的基础上,论述了综合物探方法在调查外围隐伏矿体中的应用。激电扫面可快捷有效圈定异常范围,瞬变电磁法、可控源音频大地电磁法可快速判定异常体的位置、深度、倾向。多种方法相互佐证,结合地质资料排除干扰,可有效降低多解性,为下一步地质重点工程提供资料依据。实践表明,研究成果与钻孔资料、已知矿体基本吻合,在此基础上对德尔尼东、西两区提出了后期工作的重点目标靶区,表明在本区利用这些物探方法来寻找以低阻异常为特征的铜钴矿体是行之有效的。     

茶尖岭矿区M28异常分布区银多金属矿源条件浅析

茶尖岭矿区M28异常分布区银多金属矿的形成与燕山期中酸性浅成岩浆岩有空间、成因联系,属于浅成热液矿床中的矽卡岩型成因。银多金属的成矿是热液活动、构造作用的产物,根据地层中元素的初始含量及矿源岩来阐明该异常分布区银多金属矿源条件。初步分析认为,板岩类及闪长玢岩为M28异常分布区的矿源岩,该异常分布区地层中银多金属元素的初始含量较高,该异常分布区银多金属成矿的矿源条件比较好。     

高崖跨断层短水准异常变化机理分析

2017-01～2018-04高崖水准的观测结果出现异常,为研究该异常的机理,本文基于对二维不规则载荷模型的定量模拟和库容、降水量、地下水位等影响因子的定性、定量分析,得到如下认识：1）高崖水库库容载荷变化对高崖水准的影响微弱,基本可忽略不计;2）高崖水准异常变化的主要原因是地下水位变化通过水-岩作用造成水准两端岩体的不一致变形。通过跟踪观测资料的后续变化,验证了水准异常变化机理的合理性。     

鄂尔多斯盆地高自然伽马异常特征

为了加深对盆地深部和浅部高自然伽马异常特征综合分析研究,揭示高自然伽马异常地质成因,从而促进盆地多种能源矿产协同开发研究,针对收集大量的地球物理测井资料、地质资料及其他相关成果,绘制并分析了相关成果图。研究中遵循从单孔测井曲线特征分析到典型剖面研究,并按层对高自然伽马的平面分布特征进行分析研究。化验测试结果和自然伽马能谱测井成果研究表明,在本区,自然伽马异常增大主要是由于铀的活化和聚集,导致铀元素增加而引起。相关研究表明,盆地深部和浅部的铀异常具有一定的关系,盆地历经的沉积环境变迁是铀元素富集的主导因素。     

磺酸自硬砂引起球铁件表层异常组织的研究

通过实验研究,用甲苯磺酸作催化剂的呋喃树脂自硬砂与稀土镁作催化剂生产的球铁件,通常在其铸件表层出现异常组织。提出导致异常组织产生的原因,同时又降低了试件的冲击值,并且采用反应型或屏蔽型涂料将可防止球铁件表层异常组织缺陷,为生产性能良好的球铁件提供技术依据。     

基于双位置的磁悬浮陀螺异常数据检测

针对磁悬浮陀螺全站仪在极端工作环境下受异常数据干扰的问题,该文提出了一种利用磁悬浮陀螺双位置采样数据特征进行异常数据检测、剔除的数据处理方法。采用回归分析的方法对理想工作状态下的磁悬浮陀螺双位置采样数据与陀螺寻北方位间的函数关系进行拟合分析;通过区间预测的方法明确了陀螺寻北信息中异常数据的检验标准,并依据该标准实现了对寻北观测值中粗差等异常数据信息的有效识别。工程实测数据的验证结果表明:该检验法可以有效地对磁悬浮陀螺寻北数据中的异常值信息进行分离,提高陀螺寻北定向精度。     

The Relationship Between Abnormal Meiyu and Medium-Term Scale Wave Perturbation Energy Propagation Along the East Asian Subtropical Westerly Jet

The East Asian subtropical westerly jet(EASWJ) is one of the most important factors modulating the Meiyu rainfall in the Yangtze-Huaihe River Basin, China. This article analyzed periods of the medium-term EASWJ variation,wave packet distribution and energy propagation of Rossby waves along the EASWJ during Meiyu season, and investigated their possible influence on abnormal Meiyu rain. The results showed that during the medium-term scale atmospheric dynamic process, the evolution of the EASWJ in Meiyu season was mainly characterized by the changes of3-8 d synoptic-scale and 10-15 d low-frequency Rossby waves. The strong perturbation wave packet and energy propagation of the 3-8 d synoptic-scale and 10-15 d low-frequency Rossby waves are mostly concentrated in the East Asian region of 90°-150°E, where the two wave trains of perturbation wave packets and wave-activity flux divergence coexist in zonal and meridional directions, and converge on the EASWJ. Besides, the wave trains of perturbation wave packet and wave-activity flux divergence in wet Meiyu years are more systematically westward than those in dry Meiyu years, and they are shown in the inverse phases between each other. In wet(dry) Meiyu year, the perturbation wave packet high-value area of the 10-15 d low-frequency variability is located between the Aral Sea and the Lake Balkhash(in the northeastern part of China), while over eastern China the wave-activity flux is convergent and strong(divergent and weak), and the high-level jets are strong and southward(weak and northward). Because of the coupling of high and low level atmosphere and high-level strong(weak) divergence on the south side of the jet over the Yangtze-Huaihe River Basin, the low-level southwest wind and vertically ascending motion are strengthened(weakened), which is(is not)conducive to precipitation increase in the Yangtze-Huaihe River Basin. These findings would help to better understand the impact mechanisms of the EASWJ activities on abnormal Meiyu from the perspective of medium-term scale Rossby wave energy propagation.     

地温异常数据原因分析及处理方法

针对地温异常数据种类,结合天气学原理、气象要素的时间、空间变化规律和各要素间相互联系的规律进行分析,找出导致异常数据原因,提出相应的处理方法,尽可能使缺测的要素及缺测时次减小到最小值,最大限度地保证资料的完整.     

Chemical enrichment in the early galaxy

New, precise abundance data for a large number of elements in a growing sample of extremely metal-poor stars are accumulating from the new 8-m telescopes. Combined with theoretical models, these results advance our understanding of the first generations of stars, whose nucleosynthesis products are fossilised in the oldest stars we see today and thus give clues to the earliest phases of evolution in the Galaxy. In particular, the heaviest elements give us insight into the different neutron capture mechanisms and the stellar sites where such elements could be produced. They also afford an independent way to determine the age of the Galaxy, by radioactive chronology. This revised version was published online in August 2006 with corrections to the Cover Date.