飞机反区时的操纵策略特性及物理机理研究

针对飞机在低动压飞行(如着舰)时处于阻力曲线反区所采用的Frontside操纵和Backside操纵方式,分别从指令控制、风扰抑制、执行机构影响三种情况对两种操纵策略的性能进行了仿真比较,得出相关结论,并分析了其内在物理原因。研究结果表明,Backside操纵性能优于Frontside操纵,具有响应快、超调小、无初始负调、抗风鲁棒性强,以及俯仰角、迎角和升降舵变化小等特点,但同时速度和推力变化大,且执行机构相位滞后对Backside操纵性能影响较大。     

提高飞行器升力的若干方法研究

本研究用数值模拟方法研究了四种增升方法。数据模拟的出发方程是可压流的Ｎ－Ｓ方程，格式为Ｂｅａｍ－Ｗａｒｍｉｎｇ格式的改进型。通过上述方法分别研究了：（１）动界效应对提高升力的作用；（２）涡的有利干扰对主升力面的影响；（３）吸气的驻涡增效应；（４）升力面下表面向下喷气的增升作用。研究结果表明，采用上述四种方法可有效地提高飞行器的升力，对改善飞行器的性能有着十分重要的意义。     

运用GPS空中校正飞机无线电罗差误差分析

针对某些特种飞机无线电罗差无法沿用传统校正方法在地面进行校正的状况 ,首次提出了运用 GPS接收机在空中校正飞机无线电罗差的方法。本文对影响该校正方法校正精度的各项误差因素进行了分析。     

重量的一种遥测式监测系统

本文提出一种重量信号的无线传输和测量方法。重量信号经传感顺转换成电信号，再经Ｖ／Ｆ变换后调频发射，接收信号解调后单片机处理。单片机的信号处理采用电子计数器测频方法，经过计算送显示单元，实现重量信号的遥测。     

Can Surface Flux Transport Account for the Weak Polar Field in Cycle 23?

To reproduce the weak magnetic field on the polar caps of the Sun observed during the declining phase of cycle 23 poses a challenge to surface flux transport models since this cycle has not been particularly weak. We use a well-calibrated model to evaluate the parameter changes required to obtain simulated polar fields and open flux that are consistent with the observations. We find that the low polar field of cycle 23 could be reproduced by an increase of the meridional flow by 55% in the last cycle. Alternatively, a decrease of the mean tilt angle of sunspot groups by 28% would also lead to a similarly low polar field, but cause a delay of the polar field reversals by 1.5 years in comparison to the observations.     

锅炉分层给煤装置的机理及效果分析

影响锅炉热效率的因素有多种，其中最主要的有两点：一是煤的燃烧状况，一是炉膛的换热环境。本文从煤层结构对燃烧状况的影响这个角度分析了分层给煤装置的优点和不足，并提出了几点改进方法。     

三硝基间苯二酚中硫酸测定的研究

本文研究了硫酸钡在氨水溶液中与ＥＤＴＡ的反应条件，提出用ＥＤＴＡ滴定法测定三硝基间苯二酚中的硫酸。本法准确度较高，稳定性好，操作简单，与样品标准值对照，结果满意。     

A joint mid-course and terminal course cooperative guidance law for multi-missile salvo attack

Salvo attacking a surface target by multiple missiles is an effective tactic to enhance the lethality and penetrate the defense system. However, existing cooperative guidance laws in the mid-course or terminal course are not suitable for long- and medium-range missiles or stand-off attacking. Because the initial conditions of cooperative terminal guidance that are generally generated from the mid-course flight may not lead to a successful cooperative terminal guidance without proper mid-course flight adjustment. Meanwhile, cooperative guidance in the mid-course cannot solely guarantee the accuracy of a simultaneous arrival of multiple missiles. Therefore, a joint mid-course and terminal course cooperative guidance law is developed. By building a distinct leader-follower framework, this paper proposes an efficient coordinated Dubins path planning method to synchronize the arrival time of all engaged missiles in the mid-course flight. The planned flight can generate proper initial conditions for cooperative terminal guidance, and also benefit an earliest simultaneous arrival. In the terminal course, an existing cooperative proportional navigation guidance law guides all the engaged missiles to arrive at a target accurately and simultaneously. The integrated guidance law for an intuitive application is summarized. Simulations demonstrate that the proposed method can generate fast and accurate salvo attack.     

圆柱形霍尔推力器的内磁极刻蚀研究

由实验后的圆柱形霍尔推力器来看,内磁极刻蚀是影响霍尔推力器寿命以及效率的主要因素之一.主要结合实验结果,从理论卜分析刻蚀以及刻蚀形貌形成的原因.并利用PIC粒子模拟跟踪离子的轨迹来解释内磁极的刻蚀问题.结果表明:推力器的工作状态、电磁场位形是影响内磁极刻蚀及刻蚀形貌的主要囚素.最后针对刻蚀原因提出了相应的减小刻蚀的方法,并比较了各种方法所起的作用.     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.