Design principle for parameters and interferences of tungsten carbide insert interface on roller bits

The lifetime of roll-bits with inserted tooth will be obviously decreased while drilling in strata and the tungsten carbide can be integrally separated from the roll-cone,which will need more trip out time to replace the roller bit.This study provides an entire analysis on stress as well as strength for teeth and tooth holes in loaded conditions.Qualities of tooth drop from matrix within roller bit.The optimized interferences of teeth inserted into the bit can be reasonably obtained by the critical interference derived from some relevant influence factors on the tooth-fixing quality of roller bits.     

Detection, excision and statistics of interference at the Mauritius radio telescope

A technique to detect man-made interference in the visibility data of the Mauritius Radio Telescope (MRT) has been developed. This technique is based on the understanding that the interference is generally ‘spiky’ in nature and has Fourier components beyond the maximum frequency which can arise from the radio sky and can therefore be identified. We take the sum of magnitudes of visibilities on all the baselines measured at a given time to improve detectability. This is then high-pass filtered to get a time series from which the contribution of the sky is removed. Interference is detected in the high-pass data using an iterative scheme. In each iteration, interference with amplitudes beyond a certain threshold is detected. These points are then removed from the original time series and the resulting data are high-pass filtered and the process repeated. We have also studied the statistics of the strength, numbers, time of occurrence and duration of the interference at the MRT. The statistics indicate that most often the interference excision can be carried out while post-integrating the visibilities by giving a zero weight to the interference points.     

强作用对奇异星观测效应的影响

奇异星是类似于中子星的曲奇异夸克物质组成的致密天体。本文研究了夸克这间的强作用对奇异星观测效应的影响。我们认为：（１）中子星转变为奇异星的行为是一种大的周期突变（ｇｌｉｔｃｈ）现象，这种现象取决于夸克间的强作用；（２）强作用使高温奇异星的振动阻尼也有效，这可能是驱动超新星爆发的新机制；（３）强作用加强了高温情形下奇异星和中子星在转动上的差别，奇异星的最小周期比中子星的小。     

射电望远镜远场区域强干扰源规避方法研究

随着频率使用率的提高, 射电天文台址地面或空间存在强电磁干扰致使望远镜接收机系统处于非线性状态. 为减少强电磁干扰的影响、提高天文观测效率, 提出了一种基于望远镜远场区域的强干扰源规避方法. 首先, 通过仿真分析确定的射电望远镜远场方向图, 结合望远镜与干扰源之间的位置关系, 分析了强电磁干扰到达射电望远镜焦点处的功率响应, 并依据接收机第2阶中频放大器性能参数, 确定射电望远镜处于非饱和状态的规避角度计算方法. 其次, 采用该方法计算分析了民航飞机对射电望远镜的影响, 若民航飞机上有主动发射的干扰源, 且不经过反射等传播现象, 当射电望远镜主波束轴偏开一定方向后, 可有效降低对射电望远镜的干扰强度.     

有序性分析与新疆7级强震预测

自然数可以视为反映世界客观本质的一种重要秩序，即信息，它不因加法处理而失真［１］。强地震在一定的时空范围内重复出现的现象称为有序性。自１７１６年以来，新疆及其邻区７级以上强震在时间上具有良好的有序性，有些强震在空间上亦表现出一定的有序性。强地震时间间隔值以６０、３０、４１、１９和１１年占据主导分布，并且相互之间关系密切。根据强震活动的有序性结构可进行预测：该地区未来Ｍ≥７强震可能发生在２００４年和２０１５年前后。     

超级喷发(超级侵入)后成矿作用

本文仿照超级喷发的概念定义了超级侵入,并将超级火山对应于大型岩基.文章聚焦于这样一个科学问题:为什么大规模成矿作用发生在紧接着超级喷发和超级侵入之后？为此,首先探讨了峨嵋山地幔柱系统的活动规律.尽管少数学者对玄武质岩浆大规模喷出之前的千米级地壳隆升提出了质疑,峨嵋山火山岩系第一旋回底部玄武岩直接覆盖在喀斯特之上的新观察支持千米级隆升的认识.这表明,峨嵋山地幔柱快速上涌之初期,岩石圈子系统在相当长一段时间没有作出伸展响应,尽管局部已经发生了地壳岩石的部分熔融.因此,岩浆通道形成之后,首先喷出了巨厚层玄武岩,并且后者裹挟了部分长英质岩浆.此后,岩浆喷发的规模振荡性减小,直至消失和地表沉降.斜长石巨斑玄武岩和苦橄岩中橄榄石斑晶与基质间的不平衡表明这些晶体属于循环晶,暗示岩浆曾经在深部岩浆房滞留了相当长的时间,这将导致岩石圈受热膨胀和再次隆升以及岩浆的冻结.因此,下一阶段岩浆活动的开始要求有一个冻结岩浆房的活化机制.依据野外地质学和岩相学观察,文章详细描述了流体活化机制,并强调了提出这种机制的必要性.虽然多数作者偏好升温活化机制,流体活化机制对长英质和镁铁质岩浆成矿系统都是必需的.进而,结合地幔名义无水矿物的H₂O丰度及其对岩浆产生过程的贡献,提出岩浆产量与减压速率正相关而与流体产量反相关的观点.尽管水流体可以有效降低地幔橄榄岩的固相线温度从而有可能提高岩浆产量,新生代玄武岩中橄榄岩包体依然含有未分解的角闪石和云母且名义无水矿物依然含有较多的H₂O,表明快速减压条件下含水暗色矿物的分解反应和名义无水矿物的脱水作用都是低效的.将这种认识与峨嵋山地幔柱系统的振荡性运动结合在一起,结合成矿作用的基本解是成矿金属从流体中析出的认识,可以得出超大型矿床必然形成于超级喷发和超级侵入之后.攀枝花式铁矿的观察表明,两类代表性矿床都具有铁矿浆侵位发生在成矿系统演化最后阶段的特点.因此得出结论:超大型矿床的形成取决于岩浆通道向流体通道的转换.如果岩浆通道在尚未完全封闭之前被含矿流体所利用,大规模流体快速上升将产生超大型矿床.含矿流体透过残留于通道中的熔体上升,不仅冲刷通道中的残留熔体并使其聚集在火山岩系之下或侵位于其下部形成含矿小岩体,而且持续注入于小岩浆体中的含矿流体可以导致岩浆强烈分异形成层状岩体.当通道中残留熔体被消耗殆尽,沿着通道上升的只有含矿流体.这些含矿流体充填在自生长裂隙中并强烈排气,最终可形成矿浆型富矿体.考虑到通道的规模与关闭速率的关系,推测超级喷发/侵入发生时的岩浆主通道更容易转换为含矿流体通道,因而是圈定找矿靶区的首选目标.该模型似乎与观察结果相吻合,并可与岩浆成矿系统的复杂性、小岩体成大矿理论、透岩浆流体成矿理论和通道成矿假说有机地结合在一起,较合理解释了超级喷发/侵入后成矿作用的地球动力学背景和成矿过程.由于长英质和镁铁质岩浆系统中均可见岩基,我们建议将这类成矿作用统称为岩基后成矿作用.     

基于矢量测量的在线载体磁补偿方法

针对传统载体磁补偿求解系数存在病态性的问题,本文研究了磁干扰的主要来源,忽略了涡流场的影响,在原有的模型基础上进行了简化,建立了三分量磁补偿模型,由此提出了磁场分量的在线载体补偿方法。通过与传统方法进行对比仿真,本文方法有效提高了约1.14 nT的补偿精度。同时利用现场可编程逻辑门阵列(field programmable gate array,FPGA)的高层次综合工具(high-level synthesis, HLS)对该方法进行了嵌入式硬件仿真,验证了方法在硬件系统的实时性和补偿精度。     

碳酸盐岩地区电磁波场的特性分析

形成岩溶的高阻碳酸盐岩对电磁波的吸收较弱，而且成层沉积的特定环境使碳酸盐岩地区岩石的各向异性现象较明显，由于地空界面的存在及岩溶洞壁两侧介质电性差异明显，界面清晰，又使电磁波出现强烈的反射及散射现象，从理论上对碳酸盐岩地区电磁波传播的特有现象进行了研究和分析，并给出结论。     

基于干扰试井技术的煤层气储层参数测定

为弥补传统注入压降试井测试结果以点代面的问题,提出基于煤层气干扰试井的储层参数测试方法,阐述了其基本原理、测试方法和数据分析依据。以沁水盆地南部1口激动井和4口检测井组成的井组为例,结合该井组前期注入压降法、历史拟合法测试结果,并与干扰试井测试结果进行对比分析。结果表明,煤层气干扰试井法各井测点渗透率接近利用排采数据的历史拟合值,且高于注入压降测值,但3种方法获得数据处于同一数量级之内;煤层气干扰试井技术方法可以反映试验5口井的区域渗透率分布特征,其区域东南方向渗透率较大,即为主裂隙发育方向。结合3种方法测得的参数值对比可知,煤层气干扰试井法既可获得离散点的参数值,又可以获得区域井组的连通性和优势渗流方向,结果有助于认识区域储层参数,为进一步的井网和排采井的布置提供比较直接的数据依据。     

Tsunami hazard in the Eastern Mediterranean: strong earthquakes and tsunamis in Cyprus and the Levantine Sea

A modern tsunami catalogue has been compiled for the region of Cyprus-Levantine Sea in which 24 certain or possible local tsunamis are listed from antiquity up to the present time, while six regional tsunamis, generated in the Hellenic arc, are documented which affected the region. Another set of 13 doubtful events not included in the catalogue are discussed. Tsunami intensities k and K were re-evaluated using the classic 6-grade and the new 12-grade intensity scales, respectively. The strongest tsunamis reported in the region of interest are those of 551 AD, 749, 1068, 1201, 1222, 1546 and 1759, all occurring along the Levantine coast from Gaza northward, with the exception of the 1222 wave which occurred in the Cyprean arc. The causative earthquakes, however, occur on land and are associated with the left-lateral strike-slip Levantine rift and, as such, remain unexplained. In this paper we speculate on the mechanism of these events. A second tsunami zone follows the Cyprean arc, where the situation of subaqueous seismogenic sources favours the generation of tsunamis by co-seismic fault displacements. Submarine or coastal earth slumping, however, may be an additional tsunamigenic component. Based on historical data, the average tsunami recurrence in the Cyprus-Levantine Sea region is roughly estimated to be around 30 years, 120 years and 375 years for moderate (k/K ≥ 2/3), strong (k/K ≥ 3/5) and very strong (k/K ≥ 5/8) events, respectively. The rate of tsunami occurrence equals 0.033, 8.3 × 10⁻³ and 2.7 × 10⁻³ events/year for intensity k/K ≥ 2/3, 3/5 and 5/8, respectively. For a Poissonian (random) process the probabilities of observing at least one moderate, strong or very strong tsunami are 0.28, 0.01 and 3 × 10⁻³ within 1 year, 0.81, 0.34 and 0.13 within 50 years and 0.96, 0.56 and 0.24 within 100 years, respectively. The tsunami potential in the Cyprus-Levantine Sea area is low relative to other Mediterranean tsunamigenic regions. However, the destructiveness of some historical events indicates the need to evaluate tsunami hazard by all available means. In addition, remote tsunamigenic sources, such as those of 1303 and 1481 in the eastern Hellenic arc, are able to threaten the coasts of the Cyprus-Levantine region and, therefore, such regional tsunamis should be taken into account in the evaluation of the tsunami risk of the region.