国内外侧扫声纳测量标准比较研究

由于侧扫声纳应用领域不断扩大,用户要求不断提高,国际海道测量组织和世界测量技术发达国家相继发布了各自的新版测量规范和标准。本文将我国侧扫声纳现行测量标准与国际相关标准在系统探测能力、测线布设、数据采集、质量控制等方面进行比较详细的分析比较,指出了我国侧扫声纳测量规范在测线布设、数据采集要求等方面的不足,旨在推进我国测量标准尽快实现与国际接轨。     

亚太区域不同遮挡情形下多系统组合PPP定位效能分析

利用多测站实测GNSS观测数据,模拟四周遮挡（城市环境）、单侧遮挡（峡谷环境）和顶空遮挡（大型桥梁路基环境）3种遮挡环境,从可用卫星数、PDOP值、可用历元率、定位精度和收敛时间5个方面,综合分析多系统PPP技术的定位服务效能。结果显示,相比GPS单系统PPP定位结果,在无遮挡环境下,四系统融合PPP技术在可用卫星数、PDOP值、可用历元率、定位精度和收敛时间方面分别改进300%、40%、2%、20%和50%;在遮挡环境下,分别改进300%、60%、25%、39%和52%。     

Leak-off mechanism and pressure prediction for shallow sediments in deepwater drilling

Deepwater sediments are prone to loss circulation in drilling due to a low overburden gradient. How to predict the magnitude of leak-off pressure more accurately is an important issue in the protection of drilling safety and the reduction of drilling cost in deep water. Starting from the mechanical properties of a shallow formation and based on the basic theory of rock-soil mechanics, the stress distribution around a borehole was analyzed. It was found that the rock or soil on a borehole is in the plastic yield state before the effective tensile stress is generated, and the effective tangential and vertical stresses increase as the drilling fluid density increases; thus, tensile failure will not occur on the borehole wall. Based on the results of stress calculation, two mechanisms and leak-off pressure prediction models for shallow sediments in deepwater drilling were put forward, and the calculated values of these models were compared with the measured value of shallow leak-off pressure in actual drilling. The results show that the MHPS (minimum horizontal principle stress) model and the FIF (fracturing in formation) model can predict the lower and upper limits of leak-off pressure. The PLC (permeable lost circulation) model can comprehensively analyze the factors influencing permeable leakage and provide a theoretical basis for leak-off prevention and plugging in deepwater drilling.     

Electron acceleration behind a wavy dipolarization front

In this paper, with the in-situ observations from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes we report a wavy dipolarization front (DF) event, where the DF has different magnetic structures and electron distributions at different \(y\) positions in the Geocentric Solar Magnetospheric (GSM) coordinates. At \(y \sim2.1R_{E}\) (\(R_{E}\) is the radius of Earth), the DF has a relatively simple structure, which is similar to that of a conventional DF. At \(y \sim3.0R_{E}\), the DF is revealed to have a multiple DF structure, where the plasma exhibits a vortex flow. Such a wavy DF could be the results of the interchange instability. The different structure of such a wavy DF at different sites has a great effect on electron acceleration. Fermi acceleration can occur at the site of the DF with a simple or multiple DF structure, while betatron acceleration as a local process has the contribution to energetic electrons only at the site of the DF with a simple structure.     

SONG-China Project: A Global Automated Observation Networktwo

Driven by the technological advancements and scientific objectives, the data acquisition in observational astronomy has been changed greatly in recent years. Fully automated or even autonomous ground-based network of telescopes has now become a tendency for time-domain observational projects. The Stellar Observations Network Group (SONG) is an international collaboration with the participation and contribution of the Chinese astronomy community. The scientific goal of SONG is time-domain astrophysics, such as the astroseismology and the research of variable stars in open clusters. The SONG project aims to build a global network of one-meter telescopes equipped with high-precision and high-resolution spectrographs, and two-channel lucky-imaging cameras. It is the Chinese initiative to install a 50 cm binocular photometry telescope at each SONG node to share the network platform and infrastructure. This work is focused on the design and implementation of SONG/50BiN in technology and methodology, for the ground-based network composed of multiple sites and a variety of instruments.     

The use of automated coal petrography in determining maceral group composition and the reflectance of vitrinite

Using photometric and image analysis methods, a reasonable technique and procedure have been developed for the determination of maceral group composition and the reflectance of vitrinite. This procedure is introduced by an optimum method for seeking the interval values of each maceral group, i.e., from the “fingerprint” reflectance histogram, it seeks reasonable interval values and distribution values for vitrinite and other maceral groups. After checking and correction, these values can be put into a program and computerized. This method had advantages such as increased speed of analysis and reproducibility of the results.     

中美两套西北太平洋热带气旋资料集的差异分析

利用中国气象局(CMA)和美国联合台风预警中心(JTWC)两套西北太平洋热带气旋(TC)资料集,对比分析了两者在1951—2005年TC定位和定强方面的差异。结果表明:两套资料定位差在20世纪50年代至60年代初及1988年至90年代差异较大;地理分布上主要是在TC登陆后所在的地区及高纬度洋面上差别较大。定强方面,CMA资料在20世纪50年代及60年代末至70年代初TC强度明显大于JTWC资料,JTWC资料则在80年代末以后的时段TC强度显著大于CMA资料;地理分布上定强差大的区域在80年代以前分布较零散,之后随着JTWC资料定强增大,其在西北太平洋洋面上强度显著偏强,CMA资料同期则在亚洲大陆沿岸部分地区强度较强。进一步分析显示,两套资料集之间的差异和TC观测技术的变化之间存在密切关系。在气象卫星使用以前(1951年至60年代初),以及美国空军飞机观测终止之后(1988年以后),两者无论是在定位还是定强上都存在很大差异;而两者定强差最小的时期(1973—1987年)则正好对应了飞机观测和Dvorak技术在TC观测上同时被使用的时段。两套西北太平洋TC资料集总体差异明显,却又各具特点,目前很难判断哪一套资料集更加可靠。但对于影响中国TC,CMA资料集具有明显优势。     

激发态质子转移分子2-(2'-羟基苯基)苯并噻唑溶液的全光开关效应

研究了激发态质子转移(ESPT)分子2-(2'-羟基苯基)苯并噻唑(HBT)在不同极性溶剂中的光开关行为,探讨了溶剂极性对HBT分子光开光效应的影响.揭示了光开关脉冲信号的形成原因,建立了基于光诱导HBT分子激发态非线性折射效应的皮秒全光开关的理论模型.根据对时间响应函数的理论计算和实验结果分析,确定了光开关脉冲信号下降前沿和上升后沿的形成机理以及影响因素,并提出了增强光开关信号下降前沿的关断深度,提升上升后沿的恢复速度的有效途径和方法.本文工作为制成皮秒量级关断,微秒甚至纳秒量级重新打开的快速全光开关器     

双量子阱结构OLED效率和电流的磁效应

通过结构为ITO/NPB(60 nm)/ Alq₃ ∶1 wt% rubrene(20 nm)/ Alq₃(3 nm)/ Alq₃ ∶1 wt% rubrene(20 nm)/ Alq₃(20 nm)/LiF/Al的双量子阱的黄色有机电致发光器件,研究了不同磁场强度下的发光效率和电流变化特性. 研究结果表明该器件的电流是随着磁场强度的增加而单调下降的,显示了器件的电阻是随着磁场强度的增加而增加的. 同时也得到了该结构有     

银纳米杆高温熔化断裂弛豫性能的原子级模拟研究

采用分子动力学模拟方法,研究了不同长度银纳米杆在不同温度弛豫过程中的结构演变过程.结果表明:银纳米杆存在一与杆长相关的临界熔断温度,该临界熔断温度随杆长增加而显著降低.当温度大于熔点而小于临界熔断温度时,体系形成一个高度无序的球形团簇,而温度大于临界熔断温度时,体系则熔断成两个球形团簇.并给出了银纳米杆的产生该熔断现象的机理.