矩形波导宽边纵向裂缝的分析

利用缝隙口面切向磁场连续的条件建立关于未知电场的联立积分方程,将波导内外部的互耦、波导壁厚及波导内高次模的影响全部考虑进去,然后运用矩量法求解得到一端短路和两端开路时的波导单缝中的电场分布。该结果与文献结果和HFSS仿真结果作比较,两者吻合良好,证明理论推导和编程计算的正确性。根据缝隙等效导纳和反射系数的关系计算波导一端短路时不同偏距纵缝的谐振长度,进行矩形端头与半圆端头的等效转化并给出了与仿真结果的比较。单个缝隙参数的确定为采用HFSS软件仿真法、等效电路法或场分析法进行波导裂缝阵列天线的分析和设计奠定了基础。     

SEP events and multi-spacecraft observations: Constraints on theory

Fifteen solar energetic particle (SEP) events have been analyzed using proton flux data recorded by the Helios 1, Helios 2, and IMP 8 spacecraft in the energy range ∼4–40 MeV during 1974–1982. For each of the events at least two of the spacecraft have their nominal magnetic footpoint within 20° in heliocentric longitude from each other. The SEP events are sub-grouped as a function of their heliocentric longitudinal separation and heliocentric radial distance from the SEP associated solar flare and several case studies are presented in this paper. Main results concerning their usage in estimating the SEP radial dependence are given. Moreover, we investigate the behavior of the third not connected spacecraft in order to study the dependence of the proton flux as a function of flare location. It is found that the contribution of the longitudinal gradient in determining variations in the SEP proton flux is particularly relevant for spacecraft having their magnetic connection footpoint separated from the flare between 30° and 50°.     

由稳态飞行确定纵向气动导数

研究了从稳态对称飞行数据估计气动导数的一种方法，要估计的导数是纵向静稳定性和操纵性导数，尾翼产生的阻尼导数、速度对升力和俯仰力矩系数影响的导数，其方法是基于扩展的纵向静稳定性和操纵性理论以及相应的飞行试验数据表示方法，对于大多数气导数，假设飞行测量数据是以平衡曲线和ＣＬ（α）曲线形式给出的，导数估计表达式是由已知常数，直接或非直接测量量的代数关系式构成，估计精度用结果标准误差或系统误差带表示。所研     

大气中激光等离子体通道的传播特性分析

对大气中激光等离子体通道的传播终端特性进行了研究。建立了大气中激光等离子体通道的近似电磁模型,基于圆柱坐标系中纵向分量所满足的波动方程,给出了纵向场与横向场的关系,由边界条件导出了大气中激光等离子体通道的特征方程。特征方程的数值解获得了相应色散曲线。     

电离层离子丰度对哨声传播经度效应的影响

Iss-b卫星探测结果表明,|电离层离子丰度呈现经度变化.本文选取较真实的电离层模型参数,对130°E和114°E两个子午面内传播的低纬哨声进行了射线跟踪.我们发现,由于[O~+],[He~+]和[H~+]决定的电子浓度垂直梯度的经度变化,导致哨声传播特性的经度效应,使得130°E比114°E内传播的低纬哨声更好地满足透射条件:|μsinδ|≤1.与电子浓度的水平梯度的影响比较,离子丰度决定的电子浓度垂直梯度随经度的变化使哨声传播产生的经度效应明显得多.武昌(地理30.5°N,114.6°E;地磁19.3°N).和鹿儿岛(31.5°N,130.8°E;20.5°N)两台站观测到的哨声出现率的经度效应证实了本文的理论预言.     

基于Riccati方程解的再入飞行器制导律设计

提出一种再入飞行器纵向制导律设计方法。首先对纵向运动方程沿着实际轨道线性化,然后利用线性最优调节器原理设计制导律。在每个制导周期内求解代数R iccati方程,利用其正定解构造反馈控制律,与标准轨道的控制量叠加后形成全量控制,用于实际再入轨道的制导。仿真结果表明,所设计的制导律对再入初始偏差具有较强的鲁棒性,同时它也能较好地补偿由于气动参数和大气密度摄动造成的航程误差,从而保证落点精度。     

Longitudinal variations of the ionospheric trough position

For the first time a comprehensive pattern of the longitudinal effect of the ionospheric trough position was obtained. We present new results with longitudinal variations of the winter trough position as a function of geomagnetic latitude for both hemispheres and conditions of high and low solar activity and all local time hours. We used a large observational data set obtained onboard the Kosmos-900, Interkosmos-19 and CHAMP satellites for quiet geomagnetic conditions. We found that a magnitude of the trough position longitudinal effect averaged for a fixed local time is greater in the daytime (6–8°) than in the nighttime (3–5°). The longitudinal effect magnitude reaches its maximum (16°) in the morning (at 08 LT) in the Southern hemisphere at high solar activity. But on certain days at any solar activity the longitudinal effect magnitude can reach 9–10° even at night. The shape of the longitudinal effect was found to differ significantly in two hemispheres. In the Northern hemisphere the trough is usually closest to the pole in the eastern (American) longitudinal sector, and in the Southern hemisphere the trough is closest in the western (Eurasian) longitudinal sector. The magnitude and shape of the longitudinal effect is also different during low and high solar activity. The Global Self-consistent Model of the Thermosphere, Ionosphere, and Protonosphere (GSM TIP) simulations demonstrate that during low solar activity, the longitudinal variations of the daytime trough position is mainly determined by longitudinal variations of the ionization function, formed due to the longitudinal variations in the solar zenith angle and the atomic oxygen density distribution. The longitudinal variations of the nighttime trough position is formed by the longitudinal variations in ionization of precipitating auroral particles, neutral atmosphere composition, and electric field.     

某型机马鞍形蒙皮的拉形加工

对马鞍形蒙皮零件进行了工艺分析,并根据数控蒙皮拉形机适用性广和加工能力强的特点,突破传统的蒙皮拉形工艺思路,首次将马鞍形蒙皮的凹模作为拉形模具,采用纵向拉形的方法,顺利地完成了某型机关键零件——进气道马鞍形蒙皮的试制任务。     

Bifurcation analysis of polynomial models for longitudinal motion at high angle of attack

To investigate the longitudinal motion stability of aircraft maneuvers conveniently, a new stability analysis approach is presented in this paper. Based on describing longitudinal aerodynamics at high angle-of-attack (a < 50 ) motion by polynomials, a union structure of two-order differential equation is suggested. By means of nonlinear theory and method, analytical and global bifurcation analyses of the polynomial differential systems are provided for the study of the nonlinear phenomena of high angle-of-attack flight. Applying the theories of bifurcations, many kinds of bifurcations, such as equilibrium, Hopf, homoclinic (heteroclinic) orbit and double limit cycle bifurcations are discussed and the existence conditions for these bifurcations as well as formulas for calculating bifurcation curves are derived. The bifurcation curves divide the parameter plane into several regions; moreover, the complete bifurcation diagrams and phase portraits in different regions are obtained. Finally, our conclusions are applied to analyzing the stability and bifurcations of a practical example of a high angle-of-attack flight as well as the effects of elevator deflection on the asymptotic stability regions of equilibrium. The model and analytical methods presented in this paper can be used to study the nonlinear flight dynamic of longitudinal stall at high angle of attack.     

捆绑型火箭助推段扭转与纵向振动耦合的分析

捆绑型运载火箭助推段普遍存在着扭转抖动现象 ,这里分析了造成捆绑火箭助推段扭转抖动的原因 ,提出了进一步研究的方向