海尔-波普彗星离子尾的间断和波动

给出海尔-波普彗星近日点附近大尺度观测的结果.指出:1997年2月16、17和18日海尔-波普彗星等离子尾部分有断尾事件发生.观测时刻的离子尾内物质运动速度约为50km／s;离子尾射线向主尾主轴的并拢速度约为0.080'／s.1997年3月3日海尔-波普彗星离子尾有波动现象发生.波动发生在距离彗星密度中心约130×104km,偏离主轴30°处,振幅约20×104km、其离子束宽度约8×104km、波动的相速度约为200km／s.      

等离子体彗尾流线断裂现象的讨论

等离子体Ⅰ型彗尾流线的断裂,已多次被人们见到.本文用MHD的理论,讨论和分析了这种现象,认为这是一种空间等离子体扰动所产生的结果.本文作了定性的分析,及定量的计算,比较满意地解释了这种彗尾中的观测现象.      

Design and application of an Electric Tail Rotor Drive Control (ETRDC) for helicopters with performance tests

With the development of electric helicopters’ motor technology and the widespread use of electric drive rotors, more aircraft use electric rotors to provide thrust and directional control. For a helicopter tail rotor, the wake of the main rotor influences the tail rotor’s inflow and wake. In the procedure of controlling, crosswind will also cause changes to the tail disk load. This paper describes requirements and design principles of an electric motor drive and variable pitch tail rotor system. A particular spoke-type architecture of the motor is designed, and the performance of blades is analyzed by the CFD method. The demand for simplicity of moving parts and strict constraints on the weight of a helicopter makes the design of electrical and mechanical components challenging. Different solutions have been investigated to propose an effective alternative to the mechanical actuation system. A test platform is constructed which can collect the dynamic response of the thrust control. The enhancement of the response speed due to an individual motor speed control and variable-pitch system is validated.     

金属微滴水平喷射关键参数调控机制及试验

均匀金属微滴喷射3D打印技术是一种极具应用前景的空间金属增材制造技术,明晰其重力敏感度是实现该技术空间化应用的前提。在地基条件下,将熔滴喷射沉积方向翻转至水平状态是直观反映其打印过程重力效应的有效方法。针对熔滴水平稳定喷射调控的难题,建立了熔滴水平喷射流体力学模型及压电激振动力学模型,通过试验,探究了熔滴水平喷射不稳定形成机制,明晰了不同喷射行为下的激振特性,揭示了熔滴水平稳定喷射调控规律。结果表明：压电模块驱动信号（脉宽、幅值）对激振杆振动特性影响极为显著,激振杆行程随幅值或脉宽的增加呈现出先增加后减小的变化规律;通过改变激振杆振动特性可调控熔滴直径、初始喷射速度及喷射稳定性,熔滴直径随幅值增大而减小,但受脉宽影响不大,而喷射速度与幅值及脉宽均正相关。基于此,试验得到了尺寸均匀的金属熔滴,并水平沉积打印出与设计模型一致的结构特征。     

Analysis on Potential Conflict Frequency of Intersected Air Routes in Terminal Airspace Design

In order to obtain accurate conflict risks in terminal airspace design, the concept and calculation model of potential conflict frequency for intersected routes are proposed. Conflict frequency is represented by the product of horizontal conflict frequency and vertical conflict probability. The horizontal conflict frequency is derived from the probability density distribution of conflicts in a period of time. Based on the recorded radar trajectory data, the concept and model of ROUTE distance are proposed, and the probability density function of aircraft height at a specified ROUTE distance is deduced by kernel density estimation. Furthermore, vertical conflict probability and its horizontal distribution are achieved. Examples of three intersected arrival and departure route design schemes are studied. Compared with scheme 1, the conflict frequency values of the other two improved schemes decrease to 53 % and 24%, respectively. The results show that the model can quantify potential conflict frequency of intersec ted routes.     

On the large-scale structure of the tail current as measured by THEMIS

The magnetic field structure and the spatial characteristics of the large-scale currents in the magnetospheric tail were studied during quiet and moderately disturbed geomagnetic conditions in 2009. The magnetic field of the currents other than the tail current was calculated in terms of a paraboloid model of the Earth’s magnetosphere, A2000, and was subtracted from measurements. It was found on the base of obtained tail current magnetic field radial distribution that the inner edge of the tail current sheet is located in the night side magnetosphere, at distances of about 10 R_E and of about 7 R_E during quiet and disturbed periods respectively. During the disturbance of February 14, 2009 (Dst_min ∼ −35 nT), the B_x and the B_z component of the tail current magnetic field near its inner edge were about 60 nT, and −60 nT that means that strong cross-tail current have been developed. The tail current parameters at different time moments during February 14, 2009 have been estimated. Solar wind conditions during this event were consistent with those during moderate magnetic storms with minimum Dst of about −100 nT. However, the magnetospheric current systems (magnetopause and cross-tail currents) were located at larger geocentric distances than typical during the 2009 extremely quiet epoch and did not provide the expected Dst magnitude. Very small disturbance on the Earth’s surface was detected consistent with an “inflated” magnetosphere.     

应用计算几何的月面太阳辐照度仿真模型

月面太阳辐照度对月面环境分析、月面巡视器设计具有重要意义。文章提出了一种应用计算几何的月面任意位置太阳辐照度仿真模型。首先,计算太阳、地球等天体相对月面点的位置;然后,将各天体投影至以月面点为球心的天球球面,并通过裁剪运算和二维布尔运算得到太阳未被遮挡的形状;最后,利用太阳可见面积对理想太阳辐照度模型进行修正,得到通用的模型。为验证提出模型的有效性,将仿真结果与STK软件进行比较。结果表明,文章中的模型综合考虑了地球、月面等多种因素对太阳辐射的耦合影响,其与STK软件获得的结果相比,更符合真实的太阳光照状态。     

采用差尾控制策略的某型机横滚操纵性

某型战机所采用的气动布局使得其横侧安定性较大,与同代其他现役飞机相比横滚操纵性能较差,飞行员在做横滚机动动作时飞机掉高度现象明显。分析了其在低速和高速飞行时横滚机动性能差的原因,研究了增加差动平尾控制提高横滚操纵性的问题。建立了采用差动平尾后飞机稳定横滚的数学模型,并通过定量分析计算说明了增加差动平尾控制,可以使该型战机的横滚机动性能提高近30%,而不会削弱其安定性。     

V形尾翼气动布局纵向力矩特性研究

针对某无人战斗机所采用的V形尾翼布局,通过求解N-S方程的数值计算方法,得到了上反与下反V形尾翼气动布局的纵向力矩值。对比分析结果表明,上反V形尾翼由于受翼身组合体产生的下洗和速度阻滞作用,随着迎角的增加力矩曲线有上翘现象,但随着马赫数的增加而减弱;下反V形尾翼布局力矩曲线的线性度良好。     

基于FGN输入流的G/D/1排队模拟

传统的排队理论不适于分析高速网络表现出的自相似流量.通过实验仿真,主要考察平均等待时间和在队列分别为无限和有限情形下的队列尾部特征等参数,并对以FGN为输入流的G/D/1排队模型作了定性分析.结果表明在输入流的强度和方差基本相等且系统利用律大于某一阈值的情况下,队列平均等待时间随Hurst参数增大而显著增长.同时指出在相同的条件下考察队列尾部特征,具有有限队列长度的G/D/1排队模拟结果要远优于无限队列长度下的理论分析结果.