The luminosity of γ-ray pulsars

We point out that in the polar cap model, the visible part is only part of the cap and this fact should be taken into account when calculating the pulsar luminosity. When this is done, the calculated luminosities are in basic agreement with the observed values. Based on our calculations we give a list of 12 possible γ-ray candidates.     

吉林省五凤-五星山金矿床地质特征与成矿条件

五凤一五星山金矿床属中生代陆相火山岩浅成热液型金矿床。侏罗系上统金沟岭组火山岩为其主要矿源层,矿体受火山机构的断裂、裂隙和次火山岩脉内外接触带的控制。碱长花岗岩侵入金沟岭组底部位,为金矿形成提供了主要热源。成矿作用主要进行于低压、中性介质和弱氧比、超浅成条件下。金矿一般富集于如下部位,即矿体上部;矿体转弯、膨大处及分支复合处;强冰长石绢云母硅化蚀变岩中;含细粒黄铁矿的方解石石英脉;辉银矿集中地段。     

川滇地区地震活动与地球自转速率变化之间的关系

利用川滇地区1962—2016年间发生的MS≥6.0地震资料,在去除余震的情况下,分析了其发生与地球自转速率变化极值点之间的关系。得到以下结果:川滇地区MS≥6.0地震的发生与地球自转速率变化极值点具有显著关系,对于不同震级范围的地震,其与不同周期的地球自转速率变化有关。对于MS≥7.0的地震,有90%发生在地球自转速率季节性变化极值点前14天至后37天时间段内;对于6.0≤MS≤6.4的地震,有80%发生在地球自转速率短周期变化极值点前68小时至后30小时的时间段内;对于6.5≤MS≤6.9的地震,有87.5%发生在地球自转速率短周期变化极值点前36小时至后64小时的时间段内。地震发生在特定时间段的显著性检验结果表明,川滇地区MS≥6.0地震与地球自转速率变化极值点的关系都可以在α=0.05的显著性水平下通过显著性检验。这个结果表明,在地球自转速率发生转折的期间容易触发地震,对川滇地区地震发生时间预测具有参考意义。     

安丘—莒县断裂小店—大店段断层活动证据及断层泥分布特征初步研究

郯庐断裂带最新活动的断层分布于潍坊至嘉山一带, 而安丘—莒县断裂是郯庐断裂带的重要活动断裂之一。 基于地质考察、 高密度电法探测和钻孔联合剖面, 对安丘—莒县断裂小店—大店段断层活动证据及断层泥分布特征进行研究。 地质考察发现紫红色砂砾岩逆冲到全新世耕植土上方, 两者之间发育断层泥带, 断层泥内含少量角砾岩, 为全新世活动逆断层。 高密度电法探测结果表明断层通过位置电阻率差异明显。 钻孔联合剖面揭露的地层: 全新世耕植土、 全风化砂质泥岩、 强风化砂质泥岩、 碎裂岩、 断层泥带及中风化砂质泥岩。 钻孔K1和K2揭露深灰色断层泥带, 倾向西, 倾角约为74°, 厚度约为13.9 m, 与南侧出露的断层泥带产状相协调。 工作区范围内, 发育多处褶皱、 破碎带和断层泥带, 断层表现为全新世逆断层性质。     

基于InSAR的海原—老虎山—毛毛山断裂带现今地壳形变特征

本文利用107景L波段2007年至2011年的ALOS/PALSAR卫星影像, 采用干涉图堆叠技术, 基于GAMMA软件, 利用影像数据公共区域的均值统计校正, 首次获取海原—老虎山—毛毛山断裂带整体地区的平均地壳形变速度场, 将大范围形变结果进行统一表达。 沿断层方向形变结果表明, 断裂带两侧存在明显差异运动, 断层的运动性质为左旋, 其中毛毛山-老虎山段的差异运动比较显著, 在震情跟踪工作中要给予重视。 另外, 结合研究区域内长期GPS水平速度场, 从多角度研究了区域现今地壳运动的特征。     

Radio Properties of BL Lac Object S5 2007+777

S5 2007+777 is a typical BL Lac object with a low peak frequency, and a kpc-scale extended X-ray jet. In the literature, the Doppler factor derived at the X-ray waveband by means of model estimation is about 13.0, then the intrinsic jet scale can reach the order of magnitude of 1 Mpc. In this work, we have studied the radio structure of the jet, the brightness temperature, proper motion and other properties of this source with the collected EVN (European VLBI Network) high-resolution archive data, and the American VLBA (Very Long Baseline Array) 15 GHz observed data, etc. It is found that the jet directions measured at the different wavebands of the VLBI (Very Long Baseline Interferometry) are consistent, but slightly different from the direction of the kpc-scale X-ray jet given by the literature and the direction of the VLA (Very Large Array) radio jet, which means that the Doppler brightening effect exists in the jet emission of the source. Both the mean value and median value of the radio Doppler factor of this source estimated from the brightness temperature that measured by the VLBI are 5.0, which is smaller than the Doppler factor at the X-ray waveband given by the literature, but consistent with the Doppler factor at the radio waveband obtained by using the other methods in the literature. Furthermore, by fitting the data observed in multiple epochs, it is found that the various components of the source at the same waveband do not have an evident proper motion in a long epoch, but the proper motion in short epochs exhibits even a super-luminal motion. This may be caused by the transfer of the central position of the component with a low surface brightness. Meanwhile, this also verifies the conclusion that the radio Doppler factor estimated previously is not very large, and smaller than the Doppler factor in the X-ray waveband. By using the obtained radio Doppler factor, it is found that the source has an intrinsic radio jet of rather large scale, which may reach 0.5 Mpc, because the mean value is adopted in this case, thus it indicates that the source also possibly possesses a jet close to the scale of a giant radio galaxy.     

Reliability Analysis of Main-axis Control System of the Antarctic Equatorial Astronomical Telescope Based on Fault Tree

The Antarctic astronomical telescopes work chronically on the top of the unattended South Pole, and they have only one chance to maintain every year. Due to the complexity of the optical, mechanical, and electrical systems, the telescopes are hard to be maintained and need versatile expedition teams, which means that an excessive awareness is essential for the reliability of the Antarctic telescopes. Based on the fault mechanism and fault mode of the main-axis control system for the Antarctic equatorial astronomical telescope AST3-3 (Antarctic Schmidt Telescope 3-3), the method of fault tree analysis is introduced in this article, and we obtain the importance degree of the top event from the importance degree of the bottom event structure. From the above result, the hidden problems and weak links of the system can be effectively found out, which will indicate the direction for improving the stability of the system and optimizing the design of the system.     

脉冲星TOA测量误差及几何精度分析

利用信躁比估算法对脉冲星数据库中适宜导航的脉冲星进行了脉冲到达时间测量误差计算。分析了测量误差随观测时间及探测器面积的变化情况。在此基础上,指出了在DOP值分析中脉冲星导航与GPS的不同点;按照脉冲到达时间TOA测量误差较小原则给出了10组脉冲星优选组合。分析了DOP值随观测时间及观测脉冲星数的变化情况。     

河北中山沟金矿含金石英脉中锆石U-Pb年代学及Hf同位素研究

热液石英脉型金矿石中锆石可以来自围岩,也可以由热液活动形成.因此,对其研究有助于揭示成岩成矿信息.中山沟金矿位于河北省张家口—宣化(张宣)地区,主要呈石英脉型产于水泉沟岩体西段,是张宣幔枝构造核部的典型金矿床之一.本文在矿区地质特征基础上,主要开展含金石英脉内锆石形态学特征、LA-ICP-MS U-Pb同位素测年以及H...     

从光速圆柱磁能的衰减研究毫秒脉冲双星的演化

本文用脉冲星光速圆柱附近磁能的衰减理论研究了毫秒脉冲星的演化。文中从理论上给出了脉冲星到达辐射截止线时的年龄和自转周期,及现在的辐射年龄和从现在辐射年龄到达辐射截止线所需的时间。并用此理论对7颗脉冲双星的演化作了数值计算。