2021年5月云南漾濞MS 6.4地震序列发震构造及破裂过程初探

北京时间2021年5月21日21时48分36秒,云南省大理州漾濞县发生M_S 6.4地震。利用云南数字地震台网2021年5月18日至8月22日的震相报告,采用双差地震定位法,对漾濞M_S 6.4地震序列进行重新定位。重新定位结果显示序列呈NW向优势分布,破裂长约20 km,宽约7 km,对重新定位结果进行误差分析,水平方向定位误差约为0.8 km,垂直方向定位误差约为1.0 km,定位结果具有较好的稳定性。依据震中分布的走向将序列划分为NW向的主断层与NNW向的分支断层,主断层存在较为明显的分段现象,分支断层呈雁列状分布。根据小震丛集性发生在大震断层面及其附近的原则,利用重新定位后的小震震源位置反演得到漾濞M_S 6.4序列主断层走向约320°,倾角约89°,深度范围3～13 km。根据拟合得到的断层在地表的投影位置,推测本次地震的发震断层为维西-乔后断裂西侧的草坪断裂。基于断层滑动量分布识别出3个凹凸体,结合序列时空演化特征,分析了漾濞M_S 6.4地震序列的破裂过程,结果显示断层中段的凹凸体发生初始破裂...     

基于CPⅢ控制网进行仪器加乘常数的计算方法研究

针对仪器加乘常数计算方法进行研究,旨在基于高精度CPⅢ控制网和六段法得出一种便于计算仪器加乘常数的方法.首先,本文对CPⅢ控制网自由网平差中四参数转换尺度因子的主要影响因素进行分析;接着,对铁路工程控制网独立坐标系进行变形分析,表明以铁路坐标系统设计上相对应的投影变形值可以进行严格的投影改正;之后,通过以严格投影改正后数据处理得到的CPⅢ控制网结果为基础构建六段法求解仪器加乘常数;最后,对本文提出的方法进行实验验证,其结果表明:在进行严格投影改正后,由测距误差综合引起的自由网平差中四参数转换中的尺度因子值大小相当;基于高精度CPⅢ控制网构建六段法计算仪器加乘常数的方法正确、可行.     

基于坐标转换的高铁平面精测网复测稳定性分析方法探讨

首先介绍了现有各级平面精测网复测稳定性分析的常规方法,然后结合GRP网中判别CPⅢ点稳定性的方法,尝试使用三参数坐标转换进行高铁平面精测网复测稳定性分析,最后以某高铁CPI控制网实测数据为例进行分析。结果表明,不能完全使用三参数坐标转换代替常规方法进行精测网的稳定性分析,但可在使用坐标转换后的点位残差进行稳定性评价时,结合常规法进行综合分析,可提高常规法分析判别效率。     

顾及对中误差影响的洞内导线网精度仿真计算方法研究

各种形式的导线网是长大隧道洞内平面控制测量的主要方法,但是导线测量精度不可避免地会受到全站仪和棱镜对中误差的影响.以往的洞内导线网精度仿真计算均无法顾及对中误差的影响,本文提出通过在测站和棱镜点设计坐标中添加可控随机误差的方式,实现顾及测站点和棱镜点对中误差影响的洞内导线网精度仿真计算.通过对含有对中误差的导线网仿真观测数据的平差计算,验证了本文添加对中误差方法的正确性,说明了对中误差对于导线网精度仿真计算的重要性.本文介绍的方法,可用于长大隧道洞内平面控制网精度设计和横向贯通误差预计,是一种洞内导线网精度仿真计算技术的创新方法,值得在工程实际应用中推广.本文的仿真计算结果还表明,可以通过缩短洞内导线网点对间的横向距离减弱旁折光的影响.     

Complex organics in space from Solar System to distant galaxies

Recent observational and experimental evidence for the presence of complex organics in space is reviewed. Remote astronomical observations have detected \(\sim \)200 gas-phased molecules through their rotational and vibrational transitions. Many classes of organic molecules are represented in this list, including some precursors to biological molecules. A number of unidentified spectral phenomena observed in the interstellar medium are likely to have originated from complex organics. The observations of these features in distant galaxies suggests that organic synthesis had already taken place during the early epochs of the Universe. In the Solar System, almost all biologically relevant molecules can be found in the soluble component of carbonaceous meteorites. Complex organics of mixed aromatic and aliphatic structures are present in the insoluble component of meteorites. Hydrocarbons cover much of the surface of the planetary satellite Titan and complex organics are found in comets and interplanetary dust particles. The possibility that the early Solar System, or even the early Earth, have been enriched by interstellar organics is discussed.     

夏季两次低槽冷锋型暴雨成因对比分析

利用常规观测资料和NCEP 1°×1°再分析资料,对对流层低层无低涡、无低空急流配置的低槽和冷锋影响下2004年7月29—30日后倾槽和2004年8月3—4日前倾槽两次暴雨过程的成因进行了对比分析,结果表明: 虽然两次过程对流层中低层形势非常相近,但在空间结构上却存在显著差异。后倾槽锋区向冷空气倾斜且成3段锋,其中,第1段锋在850 hPa以下,冷空气虽较弱,但对整个降水过程起抬升触发作用,暴雨区出现在该段锋移动方向的前沿,即地面辐合线呈气旋性弯曲的流线密集处;前倾槽锋区完整,湿斜压锋区向暖区倾斜,暴雨区出现在锋前1～2个纬距处,即地面辐合线右侧偏南气流密集带中。两次过程低层均有强的水汽输送,存在高温高湿区,925 hPa比湿均达15 g〖DK〗·kg-1以上,所不同的是,后倾槽暴雨区位于水汽通量大值区、等〖WTBX〗θe〖WTBZ〗密集线前沿及风场辐合明显的水汽辐合区内,而前倾槽暴雨区则位于水汽通量等值线密集带中的水汽辐合区、〖WTBX〗θe〖WTBZ〗暖舌的舌尖和风场辐合处,但更偏向暖空气一侧。此外,暴雨易发生在山区或海岸线等特殊地形抬升的区域。     

Simulation of the equatorially asymmetric mode of the Hadley circulation in CMIP5 models

The tropical Hadley circulation (HC) plays an important role in influencing the climate in the tropics and extra-tropics. The realism of the climatological characteristics, spatial structure, and temporal evolution of the long-term variation of the principal mode of the annual mean HC (i.e., the equatorially asymmetric mode, EAM) was examined in model simulations from the Coupled Model Intercomparison Project Phase 5 (CMIP5). The results showed that all the models are moderately successful in capturing the HC's climatological features, including the spatial pattern, meridional extent, and intensity, but not the spatial or temporal variation of the EAM. The possible reasons for the poor simulation of the long-term variability of the EAM were explored. None of the models can successfully capture the differences in the warming rate between the tropical Southern Hemisphere (SH) and Northern Hemisphere (NH), which is considered to be an important driver for the variation of the AM. Most of the models produce a faster warming in the NH than in the SH, which is the reverse of the observed trend. This leads to a reversed trend in the meridional gradient between the SH and NH, and contributes to the poor simulation of EAM variability. Thus, this aspect of the models should be improved to provide better simulations of the variability of the HC. This study suggests a possible reason for the poor simulation of the HC, which may be helpful for improving the skill of the CMIP5 models in the future.