Saw-tooth substorms: Inconsistency of repetitive bay-like magnetic disturbances with behavior of aurora

The relationships between the magnetic disturbance onsets, aurora dynamics and particles injections at the geostationary orbit have been analyzed in detail for 25 sawtooth substorms. It is shown that inconsistency between the above signatures of the substorms onset is typical of the powerful sawtooth substorms, unlike the isolated (“classical”) magnetospheric substorms. The distinguishing feature of the aurora in case of saw-tooth substorms is permanently high level of auroral activity irrespective of the magnetic disturbance onsets and the double oval structure of the aurora display. The close relationship between the aurora behavior and the particle injections at geostationary orbit is also broken. The conclusion is made, that the classical concept of the substorm development, put forward by Akasofu (1964) for isolated substorms, is not workable in cases of the sawtooth disturbances, when the powerful solar wind energy pumping into the magnetosphere provides a permanent powerful aurora particle precipitation into the auroral zone.     

Effects of sector structure of the interplanetary magnetic field on the upper mesosphere–lower thermosphere dynamics

In this paper we study the influence of the interplanetary magnetic field (IMF) polarity changes caused by the Earth passing through the IMF sector boundary on the dynamic processes taking place in neutral atmosphere within the altitude interval of the upper mesosphere–lower thermosphere (83–101 km). The analysis has revealed the influence of the IMF sector structure on dynamics of the upper mesosphere–lower thermosphere. There has been a significant seasonal variation of the wind reaction to the IMF polarity changes observed. The influence of the IMF polarity changes on neutral atmosphere dynamics within the altitude range of 83–101 km is most pronounced in the zonal component of neural wind when the IMF polarity changes from negative to positive in all the seasons except for spring and when IMF polarity changes from positive to negative – in spring only.     

Multi-station observation of ionospheric disturbance of March 9 2012 and comparison with IRI-model

The magnetic storm of 9 March 2012 is a single step intense storm (Dst = −143 nT) whose main phase begins around 0100 UT and lasted for almost 11 h. The increases in NmF2 recorded 33% and 67% incidence respectively during the main and the recovery phase of the storm at the stations considered. The increase in hmF2 occurred concurrently with the increase in thickness parameter B0 between 0000 and 1100 UT, and a simultaneous decrease in the shape parameter B1 for the entire mid-latitude stations. Generally, B1 responded to the storm with a decrease away from the quiet day average, and decreased simultaneously with the increase in NmF2. B0 displays higher variability magnitude during daytime than the nighttime period. The occasional differences in the response of the ionospheric parameters to the storm event are attributed to longitudinal differences. Variation in hmF2 and NmF2 is projected to change in B1, but the rationale behind this effect on B1 is still not known and therefore left open. The two IRI options over-estimate the observed values with that of URSI higher than CCIR. The over-estimation was higher during the nighttime than the daytime for NmF2 response for the mid-latitude stations and the reverse for the equatorial station. A fairer fit of the model with the observed for all parameters over Jicamarca suggests that equatorial regions are better represented on the model. Extensive study of B1 and B0 is recommended to arrive at a better performance of IRI.     

最小二乘法在计量经济模型中的应用

本文从古典计量经济模型的建立谈起，又从异方差模型，自相关模型和联立方程模型中，论述了由最小二乘法派生出的加权最小二乘法、广义最小二乘法和间接最小二乘法等。     

新型三阶TVD限制器性能分析

在计算流体力学(CFD)方法中,限制技术是影响计算精度和计算稳定性的重要因素,目前应用较广的经典二阶总变差衰减(TVD)限制器虽能较好地满足计算要求,但性能差异大且分辨率和耗散的性能间并未得到良好权衡。对一种新型的三阶TVD插值限制器(T-3限制器)进行了研究并将其与3种经典限制器进行对比。首先通过一维黎曼问题,得出T-3限制器兼顾较高间断分辨率和良好稳定性的特点;接着通过高超声速双锥绕流和X-33外形飞行器的数值实验,得到T-3限制器具有刻画复杂流动的能力以及较优的气动热计算性能。     

Robustness of multiple-limb manipulation systems

Ｄｕｒｉｎｇｒｅｃｅｎｔｙｅａｒｓ，ｃｏｎｓｉｄｅｒａｂｌｅｒｅｓｅａｒｃｈｅｆｏｒｔｈａｓｂｅｅｎｄｅｖｏｔｅｄｔｏｔｈｅｓｔｕｄｙｏｆｔｈｅｍｕｌｔｉ－ｐｌｅ－ｌｉｍｂｍａｎｉｐｕｌａｔｉｏｎｓｙｓｔｅｍｓｗｉｔｈｔｈｅａｂｉｌｉｔｙｔｏｕｓｅａ...     

抗垂风干扰直接升力控制系统设计

一、引言 在垂风干扰作用下,常规飞机往往不能保持航迹角不变,从而使得航迹变化越来越大,这在很多情况下是不符合飞机飞行要求的。而直接升力控制系统,由于实现了对应状态的解耦,在垂风干扰作用下,则可以基本保持航迹角不变。如果采用抗干扰调节器设计方法设计直接升力控制系统,则可以始终保持航迹角为0,从而保证航迹不变。本文以某型飞机为背景讨论了上述问题。采用离散域直接设计。     

箭上电磁环境检测接收天线研究

针对目前运载火箭舱内电磁环境愈发复杂且没有有效的测量手段的问题,研制了一种超宽带无源小型化接收天线。该天线采用多个整形单极子的方式拓展带宽并达到小型化目的。接收天线的测量频率范围覆盖500 MHz～6 GHz,尺寸约为60 mm×60 mm×100 mm。通过加入低噪声放大器,使可测量的最低电场强度不高于1 mV/m。由于多个整形极子天线存在相互干扰情况,因此接收天线在频率响应上与理论值存在差异,该差异可以通过校准进行消除。通过数值仿真和样机试验测试,该天线系统的测量能力良好,符合设计预期。将该接收天线应用装载在运载火箭舱内,可以对目前已知的箭上无线系统发射频段进行有效测量,对飞行过程中箭上真实电磁环境的确认、舱内电磁兼容设计、箭地无线链路设计具有重要作用。     

基于串级线性自抗扰的四旋翼姿态控制方法

针对四旋翼无人机姿态调整过程中,由于参数不确定性及外界环境干扰,往往给姿态控制带来一定困难。本文研究提出一种基于串级线性自抗扰的四旋翼姿态控制方法。首先建立四旋翼无人机的动力学姿态模型,提出采用串级PID双环路控制架构,将姿态控制任务分解为内外两个环路。采用Levant微分器提取控制参量,以强化跟踪能力。此外,对原线性自抗扰控制器进行优化,旨在更好地消除外界随机扰动对系统的影响。利用MATLAB Simulink环境对提出的控制方法进行模拟,结果表明相比传统方法,该方法能更好地抑制系统受扰动引起的影响,增强系统对期望信号的跟踪能力,从而明显提高了四旋翼无人机姿态调整的精度与稳定性,以及四旋翼无人机姿态控制的精度和鲁棒性。     

飞机地形跟踪／回避突防飞行解耦控制的人机半物理仿真研究

本文利用人机半物理仿真法,研究了大气紊流对飞机突防飞行的解耦控制特性、驾驶员的操纵性及乘坐品质的影响,检验了非线性解耦控制系统对驾驶员实时操纵指令的跟踪特性。结果表明：解耦控制律能够在大气紊流扰动下解除飞机纵横向运动的非线性交叉耦合,＿有良好的解耦操纵性能和乘坐品质,减轻了驾驶员的操纵负担,从而提高了低空突防飞行的安全性,也验证了理论研究的结果。