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。     

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.     

逼近无控旋转目标航天器的混合势函数安全制导

研究了追踪航天器逼近无控旋转目标航天器的安全制导问题，逼近过程中，追踪航天器需要躲避空间中的障碍物，同时需要避免与目标航天器的太阳能电池帆板和天线等附件发生碰撞。建立了视线坐标系下的两航天器间的相对运动方程，采用四元数描述目标航天器的姿态运动。将参考位置设为引力源，设计了吸引势函数。针对安全逼近问题，建立了球面安全区和锥面安全走廊，设计了安全势函数。将障碍物假设为具有一定半径的球体，设计了障碍物势函数。吸引势函数、安全势函数和障碍物势函数一起组成了混合势函数。为了解决整个势场中除参考位置外还可能存在其他局部极小点问题，对混合势函数进行了修正，保证参考位置位于混合势函数的最低点。利用Lyapunov稳定性理论对混合势函数进行了稳定性分析，推得符合要求的控制加速度，使追踪航天器沿着混合势函数的负梯度方向逼近无控旋转目标航天器。最后通过数值仿真验证了该方法的有效性。     

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。     

Space debris observations with the Slovak AGO70 telescope: Astrometry and light curves

The Faculty of Mathematics, Physics and Informatics of Comenius University in Bratislava, Slovakia (FMPI) operates its own 0.7-m Newtonian telescope (AGO70) dedicated to the space surveillance tracking and research, with an emphasis on space debris. The observation planning focuses on objects on geosynchronous (GEO), eccentric (GTO and Molniya) and global navigation satellite system (GNSS) orbits. To verify the system’s capabilities, we conducted an observation campaign in 2017, 2018 and 2019 focused on astrometric and photometric measurements. In last two years we have built up a light curve catalogue of space debris which is now freely available for the scientific community. We report periodic signals extracted from more than 285 light curves of 226 individual objects. We constructed phase diagrams for 153 light curves for which we obtained apparent amplitudes.     

Spectra of the two official GLEs of solar cycle 24

Based on ground-level data and on satellite data we determine in this work the observational spectrum of both, the Ground Level Enhancement of May 17, (2012) the so-called GLE71 and the Ground Level Enhancement of September 10, 2017 (GLE 72). We describe a simplified method to obtain the experimental spectrum at ground level. Data of the GLE71 and GLE72 indicate the presence of two different populations, each one with a different energy spectrum. On the other hand, we explore the kind of phenomena that take place at the source in these two particular events. In contrast with other methods based on the temporal synchronization between electromagnetic emissions of flares and coronal mass ejections (CME), here we develop an alternative option based on the study of the accelerated particles, by adjusting our theoretical spectra to the observational spectra. The main results of this work are the derivation of the source and acceleration parameters involved in the generation process. These results lead us to construct possible scenarios of particle generation in the source for each one of the two studied GLEs.     

基于BP神经网络和遗传算法对再循环风扇性能参数的确定

环控系统再循环风扇主要采用轴流风机。全压效率是衡量风机性能的重要指标,轮毂比和叶片数是影响风机全压效率的重要参数。因此,为了使全压效率最大,需要确定最佳的轮毂比和叶片数。利用ANSYS软件中的CFX模块,对不同轮毂比和叶片数下的风机模型进行计算,得到这些风机模型的性能曲线和全压效率。再通过神经网络和遗传算法,对这些风机模型的全压效率进行寻优计算,最终确定风机最佳的轮毂比和叶片数。