弹上电子产品起飞前工作时间折算研究

基于MIL-STD-810F等效公式,给出了弹上电子产品在导弹发射前通电工作时间折算为飞行任务时间的环境因子计算方法;论述了因发射前振动量级极小,发射前工作时间可以忽略不计;提出了加速试验方式,使高可靠性、长时间工作电子产品可靠性试验验证成为可能。     

基于滤波估计的线控转向路感规划

线控转向系统取消了转向盘与转向轮之间的机械连接,路面状况无法通过转向盘传递给驾驶员,路感需要模拟产生。为此对驾驶员理想转向盘力矩影响因素进行分析,基于汽车动力学模型,采用卡尔曼滤波方法对回正力矩进行估计,计算转向阻力矩,研究转向路感与车速、变传动比及侧向加速度的一般规律,提出基于滤波估计路感规划策略。仿真结果表明：路感模拟方法可以使得驾驶员获得良好的路面信息,提高汽车的操纵性和舒适性。     

人椅组合模型肢体气动特性和局部气动载荷跨超声速风洞试验研究

为了研究弹射过程中人体肢体的气动特性和防护方案的有效性 ,在 1 .2m×1 .2m跨超声速风洞中进行了人椅组合模型肢体测力和局部压力测量试验研究 ,试验的M数范围为 0 .4～ 2 .0 ,迎角范围为 5°～ 30° ,侧滑角范围为 0°～ 90°。结果表明 ,这次试验是成功的 ,所研究的防护装置都是有效的 ,侧滑使背风侧肢体被吹开的趋势增强 ,抬腿对肢体气动特性的干扰影响是不利的     

船载惯性测量单元姿态信息优化方法

随着海洋卫星通信技术的广泛应用,船载通信系统的需求量与日俱增。基于微电子系统的惯性测量单元主要用于测量船体姿态信息,实现姿态反馈与控制补偿,是船载卫星通信设备的核心器件。实际应用中通过卡尔曼滤波处理的惯性测量单元的姿态信息并不完善,经过分析惯性测量单元在运动过程中存在干扰性的有害加速度。分析了有害加速度的产生原因和对测量姿态的影响并提出姿态信息的优化方法。通过此优化方法可提升惯性测量单元的测量精度,增强船载通信系统的控制精度。     

速度控制的前加减速控制算法研究

速度控制是提高数控机床加工精度和加工效率的关键技术.常用的速度控制有前加减速控制和后加减速控制,后加减速算法简单,但会产生轨迹偏差,前加减速算法控制准确,不存在轨迹偏差.分析前加减速控制的特点,采用迭代和前向预测的方法设计了前加减速控制算法,针对小线段加工时线段长度过小而无法满足加减速区间长度的问题,设计了拐点速度修正算法和指令速度修正算法.最后在开放式六轴数控系统上实现了前加减速算法,经过加工实验,取得了较好的加减速控制效果.     

Interplanetary Physics Research in China： 2006-2008

This brief report summarized the latest advances of the interplanetary physics research in China during the period of 2006-2007,made independently by Chinese space physicists and through international collaboration.The report covers all aspects of the interplanetary physics,including theoretical studies,numerical simulation and data analysis.     

Magnetic energy release near accreting black holes

The observed non-thermal emission from accreting compact objects is often understood in terms of the expected magnetic activity of accretion disks. This review discusses the constraints on this view point that can be obtained from, principally, the X-ray spectra and the X-ray variability of black hole candidates.Furthermore, the traditional view of an accretion disk corona, put forward as the source of the non-thermal emission, analogous to the solar corona is shown to be wrong on a few important points. Firstly, the density in the equilibrium accretion disk corona is extremely low. A reasonable plasma density is retained by pair production processes similar to those existing in the pulsar magnetosphere. Secondly, the dominant resistivity in the accretion the disk on the current carrying electrons.     

Particle acceleration and kinematics in solar flares – A Synthesis of Recent Observations and Theoretical Concepts (Invited Review)

We review the physical processes of particle acceleration, injection, propagation, trapping, and energy loss in solar flare conditions. An understanding of these basic physical processes is inexorable to interpret the detailed timing and spectral evolution of the radiative signatures caused by nonthermal particles in hard X-rays, gamma-rays, and radio wavelengths. In contrast to other more theoretically oriented reviews on particle acceleration processes, we aim here to capitalize on the numerous observations from recent spacecraft missions, such as from the Compton Gamma Ray Observatory (CGRO), the Yohkoh Hard X-Ray Telescope (HXT) and Soft X-Ray Telescope (SXT), and the Transition Region and Coronal Explorer (TRACE). High-precision energy-dependent time delay measurements from CGRO and spatial imaging with Yohkoh and TRACE provide invaluable observational constraints on the topology of the acceleration region, the reconstruction of magnetic reconnection processes, the resulting electromagnetic fields, and the kinematics of energized (nonthermal) particles. This revised version was published online in June 2006 with corrections to the Cover Date.     

Simulations of pickup-ion acceleration at quasi-perpendicular shocks

We present results from hybrid simulations (kinetic ion/fluid electron) of the interaction of interstellar pickup ions with collisionless shocks. Since cross-field transport is unphysically suppressed in the one-dimensional geometry used here, an ad hoc scattering algorithm is used to model this effect. This is a necessary step to accelerate the pickup ions from their initial low energies at quasi-perpendicular shocks to the high energies which are often observed associated with traveling interplanetary shocks by Ulysses.     

引射器引气与压气机抽气建立加力燃烧室喷口低压条件的综合分析

从建设投资、运行费用、设计、操作、维护等诸多方面对引射器引气与压气机抽气建立加力燃烧室高空模拟试验器喷口低压条件进行全面分析和对比,得出引射器引气方案优于压气机抽气方案。