新型塑合木制备研究

本文介绍了塑合木的新工艺,配方、产品性能和应用前景。利用本文研究的加热-催化法制备塑合木,其成本可大幅度降低．     

高速1553B智能通用总线测试平台设计

传统的1 Mbps 1553B由于总线带宽受限,在航天测量控制领域正逐步被4 Mbps高速1553B总线替代。一般的高速1553B总线测试仪不具备精准时序控制、动态消息插入和系统故障恢复的功能,难以模拟系统实际工况。因此,通过各模式下总线的初始化配置和数据收发控制,采用SDRAM动态读取和硬件定时触发技术,结合基于心跳和消息监测的冗余总线控制机制,设计了一种高速1553B智能通用总线测试平台。通过调整消息长度、消息内容和消息间隔,验证了总线测试平台BC-RT、RT-BC、RT-RT以及MT监视功能的正确性,满足了精准时序控制、动态消息插入和系统故障恢复的需求。本平台可用于半实物仿真、时序功能的验证和系统真实负载状态的测试。     

1553B总线控制系统时间同步设计

高准确度的时间同步是实时性现场总线控制系统正确运行的基础.本文介绍了几种现场总线系统软硬件时间同步机制,针对1553B总线控制系统,通过深入分析总线协议芯片的工作时序,利用芯片内部的时标寄存器,采用软件补偿的方法,设计了一种准确度与软件和网络延迟无关的高准确度、低通讯开销的软件时间同步机制.试验表明,这种同步机制准确度可达到μs数量级.     

Sq(H) field variations at Sonmiani geomagnetic observatory,Pakistan for solar cycle 24

In this study, Sq(H) field results for Sonmiani geomagnetic observatory (SON), Pakistan are presented first time for solar cycle i.e., Solar Cycle 24. Sonmiani observatory was established in 2008 and was included in the list of INTERMAGNET Magnetic Observatory (IMO) in 2012. The analysis of Sq(H) field is performed to examine diurnal, annual and seasonal behaviour of Sq(H) field at Sonmiani along with Honolulu which is used as reference observatory. Both the observatories lie at the Equatorial Ionisation Anomaly (EIA) crest. In general strong dependency of Sq(H) field on solar cycle has been observed. First peak of SC24 was visible in Sq(H) field at both observatories. However, at HON maximum Sq(H) was observed in 2015 instead of 2014, a year later than the year of solar maximum. Prominent longitudinal difference has been noted between both observatories. At HON, maximum Sq(H) was observed during equinox while at SON it was noted during equinox and summer as a consequence of shift in latitude of Sq focus. Phase shift of Sq(H) at SON followed a general trend, that is maximum Sq(H) shifted to later hours in solar maximum as compared to solar minimum. Whereas, an opposite trend was noted at HON which might be due to coastal effect. In case of seasonal phase shift, at both observatories maximum Sq(H) occurred at later hours in summer than in winter which is opposite to the results obtained by many workers. These points need further investigation and geomagnetic as well as wind, and electric field data of other observatories situated at the EIA crest region is required to interpret the Sq(H) phase shift extensively.     

Encounter trajectories for deep space mission ASTER to the triple near Earth asteroid 2001-SN263. The laser altimeter (ALR) point of view

In cooperation with Russia, the Brazilian deep space mission ASTER plans to send a small spacecraft to investigate the triple asteroid 2001-SN263. The nearest launch opportunities for this project include June 2022 and June 2025. One main exploration campaign is being planned with focus on the largest asteroid (Alpha). Among the instruments under development, a laser altimeter (named ALR) was preliminarily designed and presented in 2010–2011. Many studies to define mission and instruments requirements were performed aiming at the characterization of important issues for the successful realization of the mission. Among them, the identification of a suitable trajectory that could be followed by the ASTER spacecraft in the encounter phase, when the main campaign will take place. This paper describes the effort undertaken with focus on the laser altimeter operation. Possible encounter trajectories were modelled and simulated to identify suitable approach parameters and conditions allowing the accomplishment of the intended investigation. The simulation also involves the instrument operation, considering approach geometry, attitude, relative motion, time/date, and the dynamics of the main asteroid. From the laser altimeter point of view, keeping in mind the desired coverage results (50% minimum surface coverage of asteroid Alpha, complying with horizontal and vertical resolution requirements), results point out crucial features for the encounter trajectory, like the need for a small inclination (10^-6 degrees; with respect to the asteroid's orbit), the most favourable spacecraft positioning (between the Sun and the asteroid) and pointing condition (back to the Sun), the minimum amount of achievable surface coverage (58%, focused on central areas), and the most proper time to conduct the main campaign (January 2025). Concerning the instrument, results offer refined values for divergence angle (500 to 650 μrad, half-cone), pulse repetition frequencies (from 1/20 to 1 Hz), and consequent data generation rates. A simulation tool that can use any 3D generated trajectories as input data was created for the analyses presented here. Although created for the ALR in this mission, this simple analysis tool can be adapted to other instruments in this or other missions.     

基于FAA25-131修正案的飞机告警系统适航问题分析

FAA25.1322规定了飞机警告灯、戒备灯和提示灯颜色的使用要求。FAA25-131修正案在原有14CFR25.1322条款的基础上,对飞行显示与机组告警系统提出了新的要求。本文对该修正案进行分解与分析,明确了修正案要求的重点考虑事项,简单、客观地呈现了与这些条款项关联的技术问题的矛盾性争辩过程,进行了基于型号研制实践的符合性方法总结,为验证民用飞机飞行显示与机组告警系统对FAR25-131修正案的符合性提供了有效途径,具有工程实践意义。     

The post sunset equatorial F- region zonal drift variability and its linkage with equatorial spread F onset and duration over Indian longitudes

The seasonal and solar activity variation of the post sunset F- region zonal plasma drift, at the magnetic equatorial region over Indian longitudes is analyzed using the Republic of China Satellite-1 data from January 2000 to April 2004. The post sunset F- region zonal drifts are observed to be higher in the years of high solar activity in comparison with low solar activity, while seasonally the drifts are minimum in summer with much higher values in other seasons. The seasonal and solar activity variations of zonal plasma drift are attributed to the corresponding variations in the neutral winds. The dependences of the F region peak vertical drift on the zonal plasma drift at 18.5 IST (Indian Standard Time) and the time difference of the conjugate points sunset times, are quantitatively analyzed. Further an integrated parameter (incorporating the above mentioned two independent factors), which is able to predict the peak vertical drift and growth rate of Rayleigh Taylor instability is proposed. The other major outcome of the study is the successful prediction of the Equatorial Spread F (ESF) onset time and duration using the new integrated parameter at 18.5 IST. ESF irregularities and associated scintillations adversely affect communication and navigation systems. Hence, the present methodology for the prediction of the characteristics of these nocturnal irregularities becomes relevant.     

Spatial asymmetry in topside ion density and vertical E × B plasma drift velocity within 75°E–95°E

The ion density measured by the Ionospheric Plasma and Electrodynamics Instrument (IPEI) on board the ROCSAT -1 over the 75°E and 95°E meridian at 600km altitude has been utilized to examine the latitudinal and longitudinal distribution within the Indian sector, in particular, the north-south and east-west asymmetries of the equatorial ionization anomaly (EIA). A longitudinal gradient in ion density at 600?km higher towards 95°E develops during the noontime and afternoon hours when the EIA is at its peak. The density gradient persists till evening hours when pre-reversal enhancements occur. The vertical E?×?B plasma drift velocity measured simultaneously by ROCSAT -1 for the same space-time configuration has also been studied. In addition to diurnal, seasonal and solar activity variations in E?×?B drift velocity, the longitudinal gradient is also observed. The EIA at the altitude of 600?km peaks at different latitudes and are mostly asymmetric about the magnetic equator. From midnight till 0800 LT, the ion density across the equator is nearly uniform in the equinoxes. But in the solstices, the density exhibits a north-south gradient. In the June solstice, density is higher in the northern hemisphere and decreases gradually towards south. The gradient in density reverses in December solstice. Normally, the EIA peaks within 1200 LT and 1600 LT while around 2000 LT, pre-reversal enhancement of ionization occurs affecting the EIA evening structure. The strength of the EIA also exhibits seasonal, year-to-year and hemispheric variations. The longitudinal asymmetry of drift velocity along 75°E and 95°E longitude sectors is the contributing factor behind the observed longitudinal asymmetry in ion density. Significant positive correlation between the strength of the EIA and E?×?B drift is observed in both longitudes.     

集装箱甩挂运输模型与应用

描述了集装箱甩挂运输的作业流程.从车辆等待时间的角度及集装箱甩挂运输的特点,分析了集装箱甩挂运输在不同情况的适用性问题.使用0-1决策变量来描述集装箱甩挂运输的各个操作流程,建立了以提箱次数、放箱次数、行驶次数、等待时间及各项操作流程的发生顺序为约束条件、以完成全部作业的总时间最短为目标函数的集装箱甩挂运输模型.通过算例分析,算出传统集装箱运输与集装箱甩挂运输的车辆等待时间,验证了集装箱甩挂运输模型的可操作性.     

农业转移人口市民化过程中地方政府行为激励问题研究——基于多任务委托代理模型

推进农业转移人口市民化的过程从本质上看是实现基本公共服务均等化的过程,而事实上,农业转移人口在享受公共福利方面与城市居民有着巨大的差别。现有体制下,地方政府作为提供公共产品的主要主体,同时面临着财政能力与体制的双重约束,从而在提供公共产品时表现出财力不足和意愿不足。文章主要是在已有研究的基础上,从地方政府意愿方面,基于一个多任务委托代理分析框架,研究在推进农业转移人口市民化过程中如何激励地方政府做出合理行为的问题,并尝试给出政策建议。