光纤陀螺惯导稳定平台与旋转调制方法

光纤陀螺仪在随机误差方面表现出极佳的性能优势,但受限于其标度因数不理想的现实。针对航海用长航时、高精度光纤陀螺惯导系统的使用需求,设计了基于光纤陀螺数字信号实现载体三维角运动隔离的同时完成惯性测量装置的旋转调制功能,可有效减小光纤陀螺标度因数误差与载体运动角速度的耦合误差,同时充分发挥光纤陀螺随机游走小的精度优势。理论仿真验证了光纤惯导稳定平台加旋转调制方法的优越性和可行性,为光纤陀螺惯导系统在高精度导航领域中的应用提供了技术基础。     

基于交互式多模型的主被动站跟踪算法

在高斯白噪声下,使用交互式多模型算法融合主动站和被动站量测信息,在各类机动状态模型切换,完成对机动目标的定位跟踪。根据主动站到达目标然后到达被动站的距离和以及目标到达主被动站的方位角和俯仰角信息建立量测模型;在交互式多模型算法的基础上,在常规直线机动模型基础上引入Singer模型,模拟目标机动运动;以几何关系求解得到的目标位置作为目标初始解,相较于其他初始模型,算法具有更好的收敛性。仿真实验表明,在主被动站间距几十千米,目标与主被动站间距几百千米,到达角误差2°左右,到达时间误差20 m左右的情况下,使用交互式多模型算法跟踪目标,收敛误差在百米级别。     

Moving scanning emitter tracking by a single observer using time of interception: Observability analysis and algorithm

The target motion analysis (TMA) for a moving scanning emitter with known fixed scan rate by a single observer using the time of interception (TOI) measurements only is investigated in this paper.By transforming the TOI of multiple scan cycles into the direction difference of arrival (DDOA) model,the observability analysis for the TMA problem is performed.Some necessary conditions for uniquely identifying the scanning emitter trajectory are obtained.This paper also proposes a weighted instrumental variable (WIV) estimator for the scanning emitter TMA,which does not require any initial solution guess and is closed-form and computationally attractive.More importantly,simulations show that the proposed algorithm can provide estimation mean square error close to the Cramer-Rao lower bound (CRLB) at moderate noise levels with significantly lower estimation bias than the conventional pseudo-linear least square (PLS) estimator.     

跨声速自由滚转试验技术研究

采用中等展弦比、薄翼型、边条、锯齿、折叠翼等设计的先进作战飞机在跨声速易出现机翼突然失速现象,从而引起非指令性横滚运动。为研究该问题,在FL-3风洞中研制了一套跨声速自由滚转试验装置,设计某验证性模型,选取马赫数范围0.8~0.95的典型飞行状态进行了静态测力和自由滚转验证性试验。试验结果预测了某模型不同构型的机翼突然失速敏感范围,并评估了非指令性横滚运动的严重程度,从而验证了试验机构的可靠性,建立了评估方法,实现了跨声速自由滚转试验技术。     

活性粒子对航空煤油着火特性影响机理分析

为了研究等离子体中的活性粒子(OH自由基)对航空煤油着火特性的影响,选择正癸烷骨架机理作为航空煤油替代燃料.用零维均质完全混合模型和零维完全预混模型对等离子体点火和燃烧过程进行计算分析,计算敏感度和各组分摩尔分数来揭示活性粒子的添加对正癸烷着火特性的影响,并采用敏感性分析方法对反应机理进行了适当修正.结果表明:修正后机...     

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.     

直升机空中运动的数值模拟

建立以直升机运动模拟和直升机作战对策体系为基础的空战模型和空中运动仿真理论,并对两架直升机的空战中的运动进行了数值模拟,模拟结果验证了空战中运动仿真理论的合理性.     

Cosmic Rays at High Heliolatitudes

The Ulysses spacecraft has been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes. It has now completed two fast latitude scans, one at solar minimum and one at solar maximum. Since its launch in October 1990, this mission has led to several surprising discoveries concerning energetic particles, cosmic rays, Jovian electrons, the solar wind, the heliospheric magnetic field and the global features of the heliosphere. This review addresses mainly the propagation and modulation of cosmic rays and other charged particles, from both an observational and theoretical point of view, with emphasis on what has been learned from exploring the inner heliosphere to high heliolatitudes. This is done for solar minimum and maximum conditions. The review is concluded with a summary of the main scientific discoveries and insights gained so far from the Ulysses mission.     

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.     

波音757-200飞机引气系统故障分析

本文对波音757-200飞机引气系统的故障进行深入分析,并制定了相关的预防性措施.