HS—19型肖氏硬度计故障分析

从结构原理来分析故障的产生、发展、现象以及产生故障的排除方法。     

一种用于ACSR的主从机并行处理系统

以微机、ＬＨ－ＳＣ１６Ａ型Ａ／Ｄ板、ＳＣ５０型Ｄ／Ａ板以及ＴＭＳ３２０Ｃ３０Ａ型ＤＳＰ板为基础，建立了时域结构响应主动控制的主从机并行处理系统。这一系统具有多通道快速运算能力，可提高控制系统的控制律，更新速率，改善控制系统的跟踪能力。     

AN IMPROVEMENT FOR LOWER－ORDER PANEL METHOD BASED ON THE DIRICHLET BOUNDARY CONDITION

ＡＮＩＭＰＲＯＶＥＭＥＮＴＦＯＲＬＯＷＥＲ－ＯＲＤＥＲＰＡＮＥＬＭＥＴＨＯＤＢＡＳＥＤＯＮＴＨＥＤＩＲＩＣＨＬＥＴＢＯＵＮＤＡＲＹＣＯＮＤＩＴＩＯＮＸｕＭｉｎｇｃｈｕ，ＧｕＷｅｎｙｉｎｇ（ＮｏｒｔｈｗｅｓｔｅｒｎＰｏｌｙｔｅｃｈｎｉｃａｌＵｎｉｖｅｒ...     

最小二乘滤波在某型火控系统信息处理中的应用

为了提高某型火控系统的反应时间和射击精度,需要对采集到的目标运动参数进行滤波。为了使算法易于实现,采用了最小二乘滤波方法。基于对最小二乘滤波的分析处理,增加了修正序列,实现了接近自适应最小二乘滤波的功能,在滤波效果上能够完全满足系统要求。最后,对滤波效果进行了检测。     

抑制直升机“地面共振”的优化设计

 本文研究抑制直升机“地面共振”的设计问题,根据控制理论中极点区配置与优化设计思想,提出了满足预定要求的系统刚度与阻尼参数的优化设计方法,并根据直升机“地面共振”的基理,提出了有效的设计方案。本文还以常见的三种计算模型作为算例,结果都是满意的。     

ExoMars 2016 Schiaparelli Module Trajectory and Atmospheric Profiles Reconstruction

On 19^th October 2016 Schiaparelli module of the ExoMars 2016 mission flew through the Mars atmosphere. After successful entry and descent under parachute, the module failed the last part of the descent and crashed on the Mars surface. Nevertheless the data transmitted in real-time by Schiaparelli during the entry and descent, together with the entry state vector as initial condition, have been used to reconstruct both the trajectory and the profiles of atmospheric density, pressure and temperature along the traversed path.The available data-set is only a small sub-set of the whole data acquired by Schiaparelli, with a limited data rate (8 kbps) and a large gap during the entry because of the plasma blackout on the communications.This paper presents the work done by the AMELIA (Atmospheric Mars Entry and Landing Investigations and Analysis) team in the exploitation of the available inertial and radar data. First a reference trajectory is derived by direct integration of the inertial measurements and a strategy to overcome the entry data gap is proposed. First-order covariance analysis is used to estimate the uncertainties on all the derived parameters. Then a refined trajectory is computed incorporating the measurements provided by the on-board radar altimeter.The derived trajectory is consistent with the events reported in the telemetry and also with the impact point identified on the high-resolution images of the landing site.Finally, atmospheric profiles are computed tacking into account the aerodynamic properties of the module. Derived profiles result in good agreement with both atmospheric models and available remote sensing observations.     

基于TOPSIS算法的空间快速响应发射方案评估

针对空间快速响应发射方案评估优选问题,通过分析空间快速响应发射任务规划过程得到发射方案组成要素,在此基础上构建了三级评估指标体系;综合考虑专家主观喜好和客观事实,同时为了有效避免个别专家个性意愿对于权重分配的影响,采用信息熵权法和群决策层次分析法相组合的方式完成了指标赋权;针对方案指标数据的多样性,通过逼近理想解排序法对方案进行了综合评估及优选排序.典型算例证明了该方法的科学性和实用性,可为空间快速响应发射方案评估优选提供理论支撑.     

The Delivery of Water During Terrestrial Planet Formation

The planetary building blocks that formed in the terrestrial planet region were likely very dry, yet water is comparatively abundant on Earth. Here we review the various mechanisms proposed for the origin of water on the terrestrial planets. Various in-situ mechanisms have been suggested, which allow for the incorporation of water into the local planetesimals in the terrestrial planet region or into the planets themselves from local sources, although all of those mechanisms have difficulties. Comets have also been proposed as a source, although there may be problems fitting isotopic constraints, and the delivery efficiency is very low, such that it may be difficult to deliver even a single Earth ocean of water this way. The most promising route for water delivery is the accretion of material from beyond the snow line, similar to carbonaceous chondrites, that is scattered into the terrestrial planet region as the planets are growing. Two main scenarios are discussed in detail. First is the classical scenario in which the giant planets begin roughly in their final locations and the disk of planetesimals and embryos in the terrestrial planet region extends all the way into the outer asteroid belt region. Second is the Grand Tack scenario, where early inward and outward migration of the giant planets implants material from beyond the snow line into the asteroid belt and terrestrial planet region, where it can be accreted by the growing planets. Sufficient water is delivered to the terrestrial planets in both scenarios. While the Grand Tack scenario provides a better fit to most constraints, namely the small mass of Mars, planets may form too fast in the nominal case discussed here. This discrepancy may be reduced as a wider range of initial conditions is explored. Finally, we discuss several more recent models that may have important implications for water delivery to the terrestrial planets.     

多故障转子-滚动轴承系统的动力学特性

为深入研究多故障转子-滚动轴承系统的机理,充分考虑了旋转部件的扭矩、剪切力、转动惯量及陀螺力矩等效应,采用Timoshenko梁单元和转盘单元建立了转子的有限元模型,集成了滚动轴承动力学模型,及不平衡、不对中、碰摩、裂纹及松动等故障模型,得到了多故障转子-滚动轴承系统的动力学方程。采用变步长龙格库塔法,获得了转子-滚动轴承系统的位移响应,研究了系统位移响应随转速变化的分岔图、庞加莱截面,以及故障特征处的时域波形图、轴心轨迹图、相平面图和频谱图,探究了多故障转子-滚动轴承系统的故障特征及其动力学特性和规律。仿真分析结果表明：多故障转子-滚动轴承系统在运行过程中存在周期运动,拟周期运动和复杂的类混沌运动等丰富的非线性行为,且在各非线性行为转速区间内,会呈现不平衡、不对中、碰摩、裂纹和松动等单一故障或耦合故障的特征和现象。     

Order out of Randomness: Self-Organization Processes in Astrophysics

Self-organization is a property of dissipative nonlinear processes that are governed by a global driving force and a local positive feedback mechanism, which creates regular geometric and/or temporal patterns, and decreases the entropy locally, in contrast to random processes. Here we investigate for the first time a comprehensive number of (17) self-organization processes that operate in planetary physics, solar physics, stellar physics, galactic physics, and cosmology. Self-organizing systems create spontaneous “order out of randomness”, during the evolution from an initially disordered system to an ordered quasi-stationary system, mostly by quasi-periodic limit-cycle dynamics, but also by harmonic (mechanical or gyromagnetic) resonances. The global driving force can be due to gravity, electromagnetic forces, mechanical forces (e.g., rotation or differential rotation), thermal pressure, or acceleration of nonthermal particles, while the positive feedback mechanism is often an instability, such as the magneto-rotational (Balbus-Hawley) instability, the convective (Rayleigh-Bénard) instability, turbulence, vortex attraction, magnetic reconnection, plasma condensation, or a loss-cone instability. Physical models of astrophysical self-organization processes require hydrodynamic, magneto-hydrodynamic (MHD), plasma, or N-body simulations. Analytical formulations of self-organizing systems generally involve coupled differential equations with limit-cycle solutions of the Lotka-Volterra or Hopf-bifurcation type.