一种基于误差四元数的战术导弹垂直发射姿态调转控制器

针对战术导弹垂直发射姿态调转时的快速性要求，研究了垂直发射快速姿态调转的控制问题。首先基于误差四元数并结合垂直发射的具体特点，建立了战术导弹垂直发射的非线性数学模型；然后通过李亚普诺夫第二方法进行控制系统设计，得出了基于误差四元数反馈控制器。分析了系统的稳定性和鲁棒性。该控制器实现了绕欧拉特征轴的旋转，缩短了姿态调转的时间，最后通过仿真验证其有效性。     

地球同步卫星远地点变轨期间的三轴姿态稳定

本文提供了地球同步三轴稳定卫星在远地点变轨机动过程中的卫星动力学模型,其中考虑了刚体、液体晃动和帆板振动的耦合,这些模型经过实际工程验证,证明是正确的。本文还给出了控制器结构,它由PID和各种晃动滤波器及帆板挠性滤波器组成。工程设计证明,这种控制器结构可满足设计要求且简单可靠。本文还给出了系统稳定性分析结果及数字仿真结果。     

三轴飞行仿真转台频带拓宽技术研究

将广泛应用于机器人手臂控制等其它柔性控制系统的输入指令整形减振技术移植到转台应用中,并对输入指令整形器的设计方法、对系统参数变化的鲁棒性进行了探讨和研究,最后以某单轴台控制系统为对象进行了实验,结果表明,输入指令整形器以前馈的形式应用于单轴台的控制系统时,既不影响系统的稳定性,又可以很好地抑制频带拓宽时的机械谐振,而且对系统参数变化具有较高的鲁棒性.此外,因其算法简单,且容易实现和调试,所以可作为拓宽飞行仿真转台频带的一种新途径.     

1989年3月大宇宙线暴事件的特征

本文分析了1989年3月一系列大耀斑等离子体抛射引起的宇宙线强度变化的特征.除对中子成分分析外,还对μ介子成分及其各向异性特征作了分析,讨论了宇宙线强度变化与太阳耀斑特性和地磁扰动之间的关系。分析发现,宇宙线的Forbush下降不仅与太阳耀斑的级别、持续时间,以及在日面上的位置有关,而且还与光学耀斑是否伴有强的X射线暴、是否有强的射电爆发,以及是否引起强的地磁暴紧密有关.各向异性分析表明,3月大事件的各向异性明显小于宁静时的各向异性,这可能是因为受到太阳活动强烈调制之后,宇宙线各向异性趋于减小的原因.     

Prompt effects of solar wind variations on the inner magnetosphere and midlatitude ionosphere

It is well known that the solar wind can significantly affect high-latitude ionospheric dynamics. However, the effects of the solar wind on the middle- and low-latitude ionosphere are much less studied. In this paper, we report observations that large perturbations in the middle- and low-latitude ionosphere are well correlated with solar wind variations. In one event, a significant (20–30%) decrease of the midlatitude ionospheric electron density over a large latitudinal range was related to a sudden drop in the solar wind pressure and a northward turning of the interplanetary magnetic field, and the density decrease became larger at lower latitudes. In another event, periodic perturbations in the dayside equatorial ionospheric E × B drift and electrojet were closely associated with variations in the interplanetary electric field. Since the solar wind is always changing with time, it can be a very important and common source of ionospheric perturbations at middle- and low-latitudes. The relationship between solar wind variations and significant ionospheric perturbations has important applications in space weather.     

太阳宁静及耀斑期间1AU附近等离子体轫致辐射研究

在太空等离子体中，尤其在等离子体内部磁场较弱时，轫致辐射是等离子体能量损失的主要机制．本文对太阳宁静及耀斑期间1AU处等离子体轫致辐射计算表明，等离子体辐射强度If的变化与辐射的电磁波频率有直接的关系．当辐射频率，接近于等离子体频率，fpe时，辐射强度显著增大．随着电磁波辐射频率的增大，辐射强度随频率增大作缓慢对数下降．辐射亮温Tb与等离子体电子温度Te、介质光深成正比．Tb与If随辐射频率变化的整体趋势一致．在相同的辐射频率情况下，太阳宁静期间If值、Tb值低于太阳耀斑期间If值、Tb值．     

Progress on Space Solar Telescope in 2004 - 2006

The progress on Chinese Space Solar Telescope (SST) in 2004-2006 is introduced. The scientific objectives are further clarified and the ground operation system has been planned. The 7 key technical problems of SST satellite platform and payloads have been tackled, which lay solid scientific and technological foundations for engineering prototype phase of the SST project. At present the SST project undergoes evaluation by CNSA and CAS so as to enter the engineering prototype phase of the SST project if it is finally approved.     

A first step towards proton flux forecasting

We present a preliminary version of a potential tool for real time proton flux prediction which provides proton flux profiles and cumulative fluence profiles at 0.5 and 2 MeV of solar energetic particle events, from their onset up to the arrival of the interplanetary shock at the spacecraft position (located at 1 or 0.4 AU). Based on the proton transportation model by Lario et al. [Lario, D., Sanahuja, B., Heras, A.M. Energetic particle events: efficiency of interplanetary shocks as 50 keV E < 100 MeV proton accelerators. Astrophys. J. 509, 415–434, 1998] and the magnetohydrodynamic shock propagation model of Wu et al. [Wu, S.T., Dryer, M., Han, S.M. Non-planar MHD model for solar flare-generated disturbances in the Heliospheric equatorial plane. Sol. Phys. 84, 395–418, 1983], we have generated a database containing “synthetic” profiles of the proton fluxes and cumulative fluences of 384 solar energetic particle events. We are currently validating the applicability of this code for space weather forecasting by comparing the resulting “synthetic” flux profiles with those of several real events.     

太阳风质子束流的演化

太阳神飞船观测表明，太阳风高速流中质子束分量相对于核分量的密度随日心距离增加而增加．提出解释这一观测现象的机理并给出二维数值模拟结果．由于阿尔芬波速随日心距离增加而减少，第二支左旋波将与更多的质子共振，把部分原来属于核分布的质子拉到束分布中来．用数值模拟方程方法求解回旋波共振导致的准线性扩散方程，数值结果与观测结果相符合．     

地磁急始年发生数周期特征的小波分析

采用小波分析方法分析了急始年发生数的时间序列的周期特征，并对急始发生数的特征与太阳黑子相对数的特征进行了简要的对照分析，分析结果表明，急始发生数的周期规律与太阳黑子相对数的周期规律是有差异的．还进行了太阳黑子相对数与急始数的相关性，太阳黑子相对数与急始磁暴的相关性研究，分析结果表明它们之间显著相关．还对急始数与急始磁暴致以及其他的一些参数之间的相关性进行了分析，最后对分析结果进行了讨论．