运载姿控系统负阻尼零点网络的特性研究

为在不同条件下由运载姿控系统校正网络实现系统的稳定,根据负阻尼零点网络幅值相同、相位滞后的特性,将其用于校正网络设计以替代常用的正阻尼零点网络。证明了箭机对负阻尼零点网络的可实现性,以及测试的重复性和稳定性。某运载一级姿控系统负阻尼零点校正网络的应用表明,可在速率陀螺安装处一阶振型斜率为正时实现系统的稳定。该方法对其他型号的设计有一定的参考价值。     

离散变量参数UMA限中均匀数取值的研究

本文用Jeffreys的无信息先验分布的Bayes方法与随机化的Fiducial方法，对UMA置信限中的均匀数u的取值问题进行了研究，结果表明，Mann建议u取1／2，对二项分布与有替换定时截尾的指数分布这是合适的，但对预定成功数或失败数的负二项分布，此值略为偏小，其相对误差与样本量n的关系为l／(2n 1).     

Acceleration at the termination shock: Anisotropies and spectra

Low-energy termination shock particle populations observed by the Voyagers upstream of the shock exhibited strong field-aligned beaming with anisotropies of the order of unity. The Parker transport equation is valid only for nearly isotropic phase space distributions and is inapplicable to these highly beamed populations. The usual approach is to revert to the more general focused transport equation retaining pitch-angle information. We developed a complimentary technique employing a three-moment expansion of the Skilling equation using Legendre polynomials. We investigate the effects of adiabatic focusing and reflection on the diffusive acceleration process at oblique shock waves. It is shown that low-energy particle intensities are discontinuous and sharply peaked at the shock, consistent with the observations. Particle spectra are not only harder than the power laws predicted from diffusive transport theory, but also exhibit spectral gaps near the low-energy acceleration threshold due to more efficient acceleration by scattering and mirroring. Our model also predicts upstream anisotropies as high as 100% for highly oblique shocks whereas downstream distributions are nearly isotropic.     

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

Cosmic-ray composition and its relation to shock acceleration by supernova remnants

An overview is given on the present status of the understanding of the origin of galactic cosmic rays. Recent measurements of charged cosmic rays and photons are reviewed. Their impact on the contemporary knowledge about the sources and acceleration mechanisms of cosmic rays and their propagation through the Galaxy is discussed. Possible reasons for the knee in the energy spectrum and scenarios for the end of the galactic cosmic-ray component are described.     

On the Differences in Composition between Solar Energetic Particles and Solar Wind

Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of ways, there are key differences which imply that solar wind is not the principal seed population for SEPs accelerated by coronal mass ejection (CME) driven shocks. This paper reviews these composition differences and considers the composition of other possible seed populations, including coronal material, impulsive flare material, and interplanetary CME material.     

影响高校德育工作的几个消极因素

本文市场经济、社会消极现象、应试教育、高等教育及德育教育自身缺陷等方面对高校德育工作的消极影响加以分析，立足现实，提出问题，与高等教育工作者，德育工作者共同探讨，以求改进完善高校德育工作。作者坚信，真正找到了问题所在，也就找到了解决问题的切入点。     

论加速可靠性增长试验(I)新方向的提出

在分析总结加速寿命试验 (ALT)及可靠性增长试验 (RGT)的基础上 ,首次提出了加速可靠性增长试验 (ARGT)这个新方向 ,并指出了在研究ARGT时将会遇到的主要问题以及解决这些问题的途径     

加速度对固体火箭发动机内弹道性能的影响

用片型装药火箭发动机和含铝复合推进剂,研究了加速度对固体火箭发动机内弹道性能的影响。研究结果表明,在加速度７０ｇ的条件下,２０１０推进剂的平均效应燃速比ｒ＾－ａ／ｒ＾０高达１．５１５,固体火箭发动机的内弹道性能呈现明显的变化。该项研究对发动机设计有实际意义。     

Particle acceleration by stochastic fluctuations and dawn-dusk electric field in the Earth’s magnetotail

This work is devoted to investigate the interaction between protons and stochastic time-dependent electromagnetic fields generated by oscillating clouds of finite size, randomly positioned in the x–y  -plane. The geometry of the system is two-dimensional and, beside the time-dependent electromagnetic fluctuations, a steady-state, dawn-dusk electric field, _Ey$E_y$, has been added along the y-direction. The simultaneous presence of the stochastic time-dependent fluctuations and of the constant electric field component in the same system gives rise to two types of acceleration mechanisms operating on test particles: a second order Fermi-like process and a direct acceleration. By performing a parametric study, we extensively study the contribution of the two processes to proton acceleration. The energy values reached by test particles in this simple model are in good agreement with those observed in the Earth’s magnetotail region. Possible applications to the problem of particle acceleration in the terrestrial magnetosphere are widely discussed, and guidelines for future works are drawn.