平流层,中间层,低热层大气加热过程特性研究

本文计算了平流层、中间层和低热层大气中各种光化过程的加热率与大气的冷却率,并且给出了20—140km的大气净加热率的昼夜变化特征．为大气潮汐波的研究提供了基础．     

DIMENSION VARIATION OF FEATURE-BASED MODEL BY OPERATING DIRECTLY ON B-REP

A new algorithm for dimension variation of feature-based models is developed.The algorithm is based on B-Rep/CSG hybrid scheme and operates directly on B-Rep.Product information (including the features locating dimensions and other data for manufacture) will not lose after model variation and modification.Furthermore, the definition and solution of features constraints are also supported.The scheme of directly operating on B-Rep overcomes many drawbacks of other proposed methods, most of which need to redo all of the previous work to implement dimension variation, so the computational cost is expensive and product information will lose.What is presented in this paper makes a new way in the area of parametric design.     

垂直发射水下航行体的通气空化数值模拟研究

基于均相流模型对垂直发射水下航行体周围的通气空化流动进行了三维数值模拟,通过与试验得到的压力数据比较验证了数值方法的可靠性,并讨论了通气时序对通气空化流场的影响。结果表明:计算结果与试验吻合较好,通气能提高空泡内压力且不同位置压力一致,空泡末端存在回射高压;随着通气时刻提前,泡内压力和回射高压增大;空泡的发展过程伴随着旋涡的形成与演变,通入空泡的气体有3种流向,气体的运动导致空泡内产生多个旋涡,旋涡的种类可以分为3类。     

高精度两步TVD格式的构造及数值检验

基于通量分裂的思想,利用Taylor级数理论和第二步限制器函数的控制,构造了在光滑区域空间为三阶、时间为一阶精度的高分辨率全变差递减(TVD)格式.该格式在激波过渡点降为一阶迎风格式.并从单个线形方程推广到非线性方程及方程组情形.通过几个典型算例的计算,并与二阶TVD格式作了比较,表明该方法对流场中的激波有较高的分辨率,且是无波动的.     

前缘形状对可控扩散叶型性能影响

采用改进的形状函数变换技术(CST)造型方法对一个可控扩散叶型(CDA)的前缘进行优化设计,实现了叶片前缘与叶身连接之间的曲率连续,消除了设计状态下叶片前缘速度尖峰,使得叶片的气动性能得到了显著改善.利用不同的形状函数生成不同的曲率连续前缘,叶型的最小损失相同,可用攻角范围的差别却很大.研究表明,这是由于前缘速度尖峰在非设计工况下的发展变化过程不同造成的.过强的前缘尖峰会导致附面层迅速增厚甚至提前转捩.     

基于大弯角扩压静子叶栅的组合流动控制方法研究

为更好地控制叶中尾缘分离及角区分离,优化叶片吸力面流动分离结构,本文提出了全叶高槽道加全弦长端壁抽吸的组合流动控制方案。此外,本文还设置了全叶高开槽方案与端壁抽吸方案,以探究全叶高槽道射流与端壁附面层抽吸的相互作用机理。以一大弯角扩压静子叶栅为研究对象,本文对三种流动控制方案进行了详细的性能分析及对比。结果表明：组合控制方案对于原型叶栅叶中尾缘分离及角区分离的综合控制效果最佳,能够在全攻角范围内分别将原型叶栅的总压损失、气流转折角及静压升系数平均增大-38.4%、3.1°及16.2%。相比于全叶高开槽方案,组合控制方案的端壁抽吸槽有效抑制了全叶高槽道出口前端壁二次流的发展,进一步削弱了角区分离。相比于端壁抽吸方案,组合控制方案的全叶高槽道则有效消除了尾缘分离,避免了叶中流场的恶化。总体看来,组合控制方案有利于最大程度地拓宽叶片的可用攻角范围,提高其扩压能力。     

α–ω Effect and peculiarities of the 27-day variations of the galactic cosmic rays intensity,solar wind and solar activity parameters

We show that the amplitudes of the 27-day variations of galactic cosmic ray (GCR) intensity, solar wind and solar activity parameters have a periodicity with duration of three to four Carrington rotation periods (3–4 CRP). We assume that the general reason for this phenomenon may be related to similar cyclicity of topological structure of the solar magnetic field lines created owing to the asymmetry of turbulent solar dynamo and solar differential rotation transforming the Sun’s poloidal magnetic field to the toroidal (α–ω effect), and vice versa.     

Application of hybrid regularization method for tomographic reconstruction of midlatitude ionospheric electron density

Reconstructing ionospheric electron density (IED) is an ill-posed inverse problem, with classical Tikhonov regularization tending to smooth IED structures. By contrast, total variation (TV) regularization effectively resists noise and preserves discontinuities of the IED. In this paper, we regularize the inverse problem by incorporating both Tikhonov and TV regularization. A specific formulation of the proposed method, called hybrid regularization, is introduced and investigated. The method is then tested using simulated data for the actual positions of the GPS satellites and ground receivers, and also applied to the analysis of real observation data under quiescent and disturbed ionospheric conditions. Experiments demonstrate the effectiveness, and illustrate the validity and reliability of the proposed method.     

地基激光清除椭圆轨道空间碎片特性的计算分析

空间碎片对人类航天活动的危害很大,用高能激光减缓其危害性已受到广泛关注.针对地基激光清除椭圆轨道空间碎片问题,提出了单脉冲变轨和多脉冲变轨两种计算分析方法.仿真计算结果表明,碎片初始真近角在100°～150°附近降轨效果最佳;从激光器在地球表面可供布站的区域讲,在碎片真近角180°附近,布站区域最大;当推进激光总作用时间较短或作用距离较小时,单脉冲变轨计算模型和多脉冲变轨计算模型计算结果接近,因此可采用单脉冲变轨计算模型计算结果近似表示多脉冲作用效果.     

First observation of upper mesospheric semi annual oscillations using ground based airglow measurements from Indian low latitudes

We summarize two years of Mesosphere Lower Thermosphere Photometer (MLTP) operation of mesospheric OH and O₂ emission monitoring. The deduced mesospheric OH and O₂ temperatures show large variability. Nightly temperature variations over Gadanki (13.5°N, 79.2°E) are dominated by the short period wave features, while tidal amplitudes are relatively small. Our measurements are the first to report a long period seasonal variation at two upper mesospheric altitudes simultaneously over the Indian sector. Our observations reveal the presence of a dominant semi-annual oscillation (∼6 months periodicity) together with a shorter period (∼2.5  months periodicity) oscillation in both OH and O₂ data.