变几何参数对变循环发动机过渡态性能的影响分析

为了研究变几何参数对变循环发动机(Variable Cycle Engines,VCE)过渡态性能的影响,对功率提取法(Virtual Power Extraction Method,VPEM)进行了总结与发展,并以双轴混排涡扇发动机的VPEM模型为工具,研究了尾喷管喉部面积和涡轮导向器喉部面积对双轴混排涡扇发动机过渡态性能的影响,建立了应用于双外涵VCE的VPEM模型,并以此为工具研究了高低压涡轮导向器喉部面积、尾喷管喉部面积和后可变面积涵道引射器面积对VCE过渡态性能的影响。结果表明,变几何参数对涡扇发动机和VCE过渡态性能的影响规律一致,尾喷管喉部面积和高低压涡轮导向器喉部面积增加5%带来高压转子的功率变化分别为1.9%,6%和3.5%,低压转子功率变化分别为-3%,22%和-7%,RVABI面积对过渡态性能的影响并不显著。     

Cosmos 2421卫星解体事件分析

2008年上半年俄罗斯的Cosmos 2421卫星接连发生了三次不同程度的解体, 并产生了数百颗碎片. 本文利用美国公布的Cosmos 2421卫星及其碎片的两行根数系列, 对三次解体事件发生的时间, 解体碎片的轨道分布、速度分布和面积质量比以及寿命等进行了分析, 并对解体碎片对航天器的影响进行了评估. 分析结果表明, Cosmos2421卫星的三次解体事件分别发生在2008年3月14日、4月28日、6月9日; 解体碎片分布在200~1400 km 的高度范围内; Cosmos 2421卫星解体导致的碎片在空间三个方向上的速度增量均值分别为-8.4m/s, 8.6m/s, -8.3m/s; 67\%的解体碎片的寿命都在1年以内, 解体事件造成500 km以下的空间碎片空间密度增加, 对载人航天器产生了影响. 通过对Cosmos 2421卫星解体事件的分析可以看出, 利用解体碎片的轨道信息可以反演解体事件特性, 根据解体碎片的寿命和空间密度分布的计算结果可以评估解体事件对未来发射活动和在轨卫星的影响.      

取样示波器瞬态响应的光电校准技术研究

本文介绍了一种使用光电方法对取样示波器瞬态响应进行校准的技术。该技术基于飞秒激光和光导开关原理,实现了超快电压脉冲的产生和探测,获得可用于取样示波器校准的信号,之后利用时基修正、抖动修正、反卷积等处理手段,实现了取样示波器瞬态响应的校准。本技术能够获得取样示波器完整的冲激响应和阶跃响应,具有非常重要的意义。     

动力系统精细算法的逼近机理与误差分析

发现以下３者的协同作用是实现精细算法高精度,高效率的内在机制和根本原因：１）Ａ│ｘ│〈∞,指数矩阵ｅ＾Ｈｘ的Ｍａｃｌａｕｒｉｎ级数展开式绝对收敛;２）初始Ｍａｃｌａｕｒｉｎ级数展开式中的有效展开项总数能够通过递推算法以指数方式扩展;３）新增有效展开项的系数能够通过递推算法以指数或拟指数方式逼近其真值。     

Energization of charged particle in a time-dependent chaotic magnetic field with an implication of the production of seed particles in solar energetic particle events

We investigate the acceleration of charged particles in a time-dependent chaotic magnetic field in this work. In earlier works, it has been demonstrated that in an asymmetric wire-loop current systems (WLCSs), the magnetic field is of chaotic in nature. Furthermore, observations also showed that there exist time-varying current loops and current filaments in solar corona. It is therefore natural to conceive that the magnetic field on the solar surface is chaotic and time-dependent. Here, we develop a numerical model to study the acceleration process of charged particles in a time-varying chaotic magnetic field that is generated by an ensemble of 8 WLCSs. We found that the motion of energetic particles in the system is of diffusive in nature and a power law spectrum can quickly develop. The mechanism examined here may serve as an efficient pre-acceleration mechanism that generates the so-called seed particles for diffusive shock acceleration at a coronal mass ejection (CME) driven shock in large solar energetic particle (SEP) events.     

Coupling Magneto-Electro-Elastic node-based smoothed radial point interpolation method for free vibration and transient analysis of Functionally Graded Magneto-Electro-Elastic structures

A Coupling Magneto-Electro-Elastic (MEE) Node-based Smoothed Radial Point Interpolation Method (CM-NS-RPIM) was proposed to solve the free vibration and transient responses of Functionally Graded Magneto-Electro-Elastic (FGMEE) structures. By introducing the modified Newmark method, the displacement, electrical potential and magnetic potential of the structures under transient mechanical loading were obtained. Based on G space theory and the weakened weak (W²) formulation, the equations of the multi-physics coupling problems were derived. Using triangular background elements, the free vibration and transient responses of three numerical examples were studied. Results proved that CM-NS-RPIM performed better than the standard FEM by reducing the overly-stiff of structures. Moreover, CM-NS-RPIM could reduce the number of nodes while guaranteeing the accuracy. Besides, triangular elements could be generated automatically even for complex geometries. Therefore, the effectiveness and validity of CM-NS-RPIM were demonstrated, which were valuable for the design of intelligence devices, such as energy harvesters and sensors.     

狭缝斜肋内冷通道流动和换热特性的数值研究

为了探究狭缝斜肋的流动和换热特性,进一步挖掘传统斜肋的性能,采用数值模拟的方法,研究了五种不同位置和倾斜角度的狭缝对45°斜肋流动和换热特性的影响,计算的进口雷诺数为2×104～8×104,并与传统的实心肋进行了对比分析。结果表明,狭缝的存在显著改变了冷却通道的流动结构以及换热分布,降低了冷却通道的阻力损失,减小了通道整体的强化换热系数,但同时增加了肋片表面的强化换热系数,且狭缝的位置和倾斜角度的不同对通道性能也存在一定的影响。对比综合热效率,狭缝斜肋相比实心肋增加了约12%～15%。     

带有加强肋的涡轮机匣排孔冲击连腔结构内部换热特性研究

为获得涡轮机匣内部表面换热系数分布数据,以带有加强肋的排孔冲击连腔结构为对象进行了瞬态液晶实验。研究了不同射流雷诺数（Re=5.1×10³~1.1×10⁴）、冲击间距比（2.5,5.0,7.5）及轴向间距比（4.0,9.0,14.0）对靶面努塞尔数的影响规律。实验结果表明：增大射流雷诺数对靶面平均努塞尔数的提升最显著。随着冲击间距比的增大,靶面平均努塞尔数逐渐减小,但这种换热削弱效果局限在距冲击驻点2D~3D（D为冲击孔直径）范围内,其它区域的变化很小。在靠近前后端壁的局部区域,表面努塞尔数随冲击间距比的增大而增大。轴向间距比的改变不会影响无出流孔靶面的换热情况,对于有出流孔靶面而言,轴向间距比为9.0的结构换热效果最好。Re=5.1×10³条件下,轴向间距比为9.0结构在有出流孔靶面上的平均努塞尔数相比4.0和14.0结构分别增大了5.7%和8.1%,并且随雷诺数增大,增幅越大。     

Cone model-based SEP event calculations for applications to multipoint observations

The problem of modeling solar energetic particle (SEP) events is important to both space weather research and forecasting, and yet it has seen relatively little progress. Most important SEP events are associated with coronal mass ejections (CMEs) that drive coronal and interplanetary shocks. These shocks can continuously produce accelerated particles from the ambient medium to well beyond 1 AU. This paper describes an effort to model real SEP events using a Center for Integrated Space weather Modeling (CISM) MHD solar wind simulation including a cone model of CMEs to initiate the related shocks. In addition to providing observation-inspired shock geometry and characteristics, this MHD simulation describes the time-dependent observer field line connections to the shock source. As a first approximation, we assume a shock jump-parameterized source strength and spectrum, and that scatter-free transport occurs outside of the shock source, thus emphasizing the role the shock evolution plays in determining the modeled SEP event profile. Three halo CME events on May 12, 1997, November 4, 1997 and December 13, 2006 are used to test the modeling approach. While challenges arise in the identification and characterization of the shocks in the MHD model results, this approach illustrates the importance to SEP event modeling of globally simulating the underlying heliospheric event. The results also suggest the potential utility of such a model for forcasting and for interpretation of separated multipoint measurements such as those expected from the STEREO mission.     

Exploring the global shock scenario at multiple points between sun and earth: The solar transients launched on January 1 and September 23, 1978

We revisit the transient interplanetary events of January 1 and September 23, 1978. Using in-situ and remote sensing observations at locations widely separated in longitudes and distances from the Sun, we infer that in both cases the overall shock surface had a very fast “nose” region with speeds >900 and >1500 km⁻¹ in the January and September events, respectively, and much slower flank speeds (∼600 km⁻¹ or less), suggesting a shock surface with a strong speed gradient with heliospheric longitude. The shock-nose regions are thus likely efficient acceleration sites of MeV ions, even at 1 AU from the Sun. Our 3D magnetohydrodynamics modeling suggests that a 24° × 24° localized disturbance at 18 solar radii injecting momentum 100 times the background solar wind input over 1 h can produce a disturbance in semi-quantitative agreement with the observed shock arrival time, plasma density and velocity time series in the January 1978 event.