M型恒星周围系外行星统计研究          下载免费PDF全文

潘梦睿  季江徽  王素 《天文学报》2021,62(4):38

M型恒星(M dwarf)是主序星中质量较小的恒星,也是银河系中数量最多的恒星类型,在其周围形成的行星通常距离主星较近,宜居带也比F、G、K型恒星更靠近主星,更有利于发现系外宜居行星.研究表明, M型恒星周围平均存在2.5颗小质量行星,约为F、 G、 K型恒星的3.5倍,但M型恒星周围巨行星的出现率(occurrence rate)则比F、 G、K型小一个量级.基于M型恒星周围发现的401颗行星的参数开展了统计研究,发现质量越大的行星平均轨道半长径越大.类地行星约占行星总数的74%,且轨道半长径均小于1 au,其中28颗行星具有潜在宜居性.根据行星质量-半径关系,在质量等于4倍地球质量(M⊕)处存在一拐点,除少数几颗行星外,大部分小于该质量的行星可能都是由约65%的硅酸盐和约35%的铁组成,大于该质量的行星半径则随质量增加而迅速增大.约60%的M型恒星周围的行星位于多行星系统且轨道分布紧密,相邻行星轨道在3:2、5:3及2:1等平运动共振位置处存在峰值. M型恒星的多行星系统形成与演化等问题对现今的行星形成理论提出了新挑战.  相似文献   

利用双视角消除太阳矢量磁场观测中的180◦不确定性          下载免费PDF全文

周茹芸  汪毓明  宿英娜  毕少兰  刘睿  季海生 《天文学报》2021,62(4):41

随着"环日轨道器"(Solar Orbiter, SO)的在轨运行,太阳磁场观测进入了双视角遥测的时代.对利用太阳磁场的双视角观测改正矢量磁图中存在的横场(垂直于视线方向的磁场分量) 180°不确定性进行了模拟,首先模拟了对解析解得到磁图的双视角观测,然后利用"日震学和磁学成像仪"(Helioseismic and Magnetic Imager, HMI)在不同时间观测到的一个老化黑子的磁图模拟了双视角观测.发现要改正一个磁图中横场方向的180°不确定性,在观测上只需要另外一个平行于视线方向的磁场即纵向磁场观测的协助.利用HMI的磁场观测模拟,估算显示30°的张角能够改正50 Gs磁场中的180°不确定性.更大的张角虽然更有利于更弱磁场的改正,但是考虑到投影效应的不利影响, 30°左右的张角应该是未来空间设备进行多视角观测太阳磁场的最佳张角.  相似文献   

Analysis and Comparison for Fusion Algorithms of Time Transfer     

WANG Wei-xiong  DONG Shao-wu  WU Wen-jun  GUO Dong  ZHANG Jian 《Chinese Astronomy and Astrophysics》2021,45(2):224-235

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射电望远镜多目标观测策略优化          下载免费PDF全文

翟楠楠  刘志勇  王娜  朱春花 《天文学报》2021,62(6):63

望远镜调度是望远镜运行中的关键组成部分, 用于辅助科研人员进行合理的观测计划安排, 提高望远镜的运行效率, 获取高质量的观测数据. 然而, 由于不同观测项目的科学需求不同, 望远镜的调度过程十分复杂. 针对短周期多目标的观测项目, 考虑望远镜换源时转动时长、观测高度角等因素进行建模, 采用贪心算法对中国科学院新疆天文台南山26m望远镜脉冲星到达时间观测列表进行调度. 通过模拟表明, 使用算法完成的观测列表可以有效地减少观测过程中的平均转动时长, 提升观测数据的质量, 提高望远镜时间利用率, 减少科研人员对观测列表编排的负担.  相似文献   

海洋效应对中国沿海地磁观测影响——以广州台站为例   总被引：2，自引：1，他引：1       下载免费PDF全文

李建平  翁爱华  李世文  杨悦  唐裕  张艳辉 《地球物理学报》2018,61(2):649-658

以广州台站为例，研究海洋效应对中国沿海地磁观测C-响应的影响.海洋效应的三维正演模拟采用球坐标系下交错网格有限差分方法，假设磁层环形电流源，正演电阻率结构模型采用"地表3-D电导+1-D层状背景"复合模型.数值模拟结果表明，中国地区沿海C-响应受海洋效应影响明显.在空间上，沿海岸线方向，受海洋效应影响，单周期的C-响应由无海洋效应的常值变形为平行于海岸线的等值线密集梯度带；在垂直海岸方向，海洋效应影响向内陆减小，其影响可达哈尔滨-贵阳一线.海洋效应影响采用比值法进行校正，以广州台站为例，在比值曲线上发现海洋效应对C-响应的影响最大周期可达20天左右，并且就中国沿海而言，相对全球平均一维模型，利用中国地区平均一维电导率模型作为背景模型的海洋效应校正结果更加合理.进一步对广州台站海洋效应校正前后的C-响应进行了1-D反演，由于校正前的C-响应在小周期时受海洋效应特别大，直接反演无法拟合数据；但校正后反演拟合明显变好，得到的1-D导电模型表明广州地区上地幔及地幔转换带的电阻率比中国平均电阻率高约一个量级，推测中国华南地区南部的地幔转换带可能处于相对冷的环境，该模型可能成为菲律宾海板块西向俯冲并滞留到华南大陆下方地幔转换带的电性证据.  相似文献   

张力腿平台筋腱支撑浮筒结构设计研究     

王火平  金文学  吕东  范志峰  王立权 《海洋工程》2018,36(3):69-75

在张力腿平台筋腱与海底桩基连接后,需要筋腱支撑浮筒为筋腱提供足够的浮力,保证筋腱在平台运抵工作海域之前不会发生倾覆。针对南海油田自主研发的张力腿平台筋腱实际尺寸及设计要求,设计了适用于1 061 mm(40英寸)筋腱、500米水深的张力腿平台筋腱支撑浮筒,并对筋腱支撑浮筒主要受力进行了分析计算,根据所计算的载荷情况对关键部件进行了有限元仿真分析,验证了结构强度的可靠性,并得到了结构的应力集中点与最大变形点,为筋腱支撑浮筒的结构设计提供了参考。  相似文献   

Research on the Application of Fast-steering Mirror in Stellar Interferometers     

Mei Rong  Hu Zhong-wen  Xu Teng  Sun Chang-sheng 《Chinese Astronomy and Astrophysics》2018,42(3):475-486

In stellar interferometers, the fast-steering mirror (FSM) is widely utilized to correct the wavefront tilt caused by the atmospheric turbulence and internal instrumental vibration, because of its high resolution and fast response frequency. In this study, the non-coplanar error between the FSM and the actuator deflection axis introduced by the manufacturing, assembly, and adjustment is analyzed systematically. Via a numerical method, the additional optical path difference (OPD) caused by the above factors is studied, and its effect on the fringe tracking accuracy of a stellar interferometer is also discussed. On the other hand, the starlight parallelism between the beams of two arms is one of the main factors for the loss of fringe visibility. By analyzing the influence of wavefront tilt caused by the atmospheric turbulence on fringe visibility, a simple and efficient real-time correction scheme of starlight parallelism is proposed based on a single array detector. The feasibility of this scheme is demonstrated by a laboratory experiment. The results show that after the correction of fast-steering mirror, the starlight parallelism meets preliminarily the requirement of a stellar interferometer on the wavefront tilt.  相似文献   

基于背景噪声研究青藏高原东北缘瑞利波相速度和方位各向异性   总被引：2，自引：1，他引：1       下载免费PDF全文

王琼  高原 《地球物理学报》2018,61(7):2760-2775

本研究收集了甘肃、青海、宁夏等118个宽频带数字地震台站的连续波形资料，利用噪声互相关，经过计算和筛选，在5~38 s范围内，共得到5773条瑞利波相速度频散曲线.然后采用1°×1°的网格划分，反演获得青藏高原东北缘相速度和方位各向异性分布.结果表明：短周期8~12 s内，鄂尔多斯从低速异常变为高速异常；该周期范围内各向异性结果与区域断裂走向有很好的一致性.18~25 s周期内，祁连地块、松潘-甘孜地块、羌塘地块低速异常范围逐渐变大，随周期增加地壳低速异常与人工探测结果相符；鄂尔多斯表现为速度随周期增加逐渐变大，说明其中下地壳速度相对偏高，不存在低速异常；该周期范围内的各向异性特征表现为，祁连地块和松潘甘孜地块大致呈NW-SE方向，而青藏高原内部快波方向显示了顺时针旋转的形态.在30~35 s范围内面波速度主要受莫霍面深度和莫霍面附近介质速度的影响，与地壳厚度分布有非常好的吻合.综合不同方法获得的各向异性研究结果，支持印度-欧亚板块的碰撞使青藏高原东北缘地壳发生缩短和逐渐隆升的观点，认为整个岩石圈的垂直缩短变形是青藏高原东北缘的主要形成机制.  相似文献   

Study on the Moment Magnitude of Small and Moderate Earthquakes Located in the Inner Mongolia Region     

Liu Fang  Zhang Fan  Li Bin  Na Re 《中国地震研究》2018,32(1):53-63

Based on digital seismic waveform data from Inner Mongolia Digital Seismic Network, the source spectrum parameters of 182 small and moderate earthquakes from January, 2009 to September, 2016 are derived, and the seismic moment M₀ and moment magnitude M_W of the earthquakes are calculated. The M_L-M_W relationship and the relationship between stress drop and magnitude are obtained using the linear regression method. It is clear that incorporating the moment magnitude into the seismic quick report catalog and the official earthquake catalog can enrich earthquake observation report content, thus providing better service for earthquake emergency and earthquake scientific research.  相似文献   

SIMULATION STUDY OF ROAD-CUT EFFECTS ON SLOPE STABILITY     

CHEN Xiao-li  WANG Ming-ming  ZHANG Ling 《地震地质》2018,40(6):1390-1401

Landslides and rock falls along the highway are common geological hazards in Southwest China. As an influencing factor on potential landslides behavior, roads or distance to roads have been successfully used in landslide susceptibility assessments in mountainous area. However, the relationship between the road-cut and the slope stability is not clear. Therefore, we performed two-dimensional slope stability calculation using the general limit equilibrium (GLE)method incorporated in the software SLOPE/W of GeoStudio for stability analysis of slopes. Our studies show that the man-made roads influence on the slope stability mainly exists in two ways:One is to create a new steep slope, which will result in rock falls and shallow landslides along the roads; the other is to influence the stability of the original slope, which will result in comparatively huge landslides. For the latter, our simulation study reveals that the road location, namely at which part of a natural slope to construct a road is important for the slope stability. For a natural slope with a potential slip surface, if a road is constructed at or near the slope toe where the potential slip surface surpasses, it will greatly degrade the slope's factor of safety (Fs) and make the slope unstable; however, if a rode-cut is near the top of the slope, it will increase the slope's Fs and make the slope more stable. The safety location is different for different slope angle, steeper slope needs a higher location for a safety road-cut in comparison with gentle slopes. Moreover, the slope stability decreases when loading a seismic force and it varies with the slope angle. Firstly, the Fs decreases when the slope angle increasing, and when the slope angle reaches 45°, the Fs then becomes greater with the slope angle increasing.  相似文献