电离层等效电流体系对行星际激波的响应研究

行星际激波是导致地球磁层-电离层系统发生扰动的重要原因之一,其可以通过对磁层-电离层系统电流体系的改变来影响地磁变化.本文采用全球三维磁流体力学数值模拟方法,分析了行星际激波作用下电离层等效电流体系的即时响应.模拟结果表明,在激波作用下伴随着异常场向电流对的产生,电离层在午前午后出现一对反向的等效电流涡.这对涡旋一边向极侧和夜侧运动,一边经历强度增强和减弱直至消失的过程.激波过后等效电流体系图像逐渐演化为激波下游行星际条件控制的典型图像.这个响应过程与行星际激波强度有关,激波强度越强,则反向的等效电流涡旋强度越大,寿命也就越短.      

分布式小卫星雷达系统误差估计的新方法

相干联合处理小卫星编队雷达接收的地面回波可在获得大的成像测绘带的同时获得较高的方位分辨力，具有非常重要的军事应用前景。然而复杂的分布式小卫星雷达系统误差尤其是三维基线误差和多通道幅相误差，严重影响了联合处理各卫星回波数据的效果，甚至使其失败。针对这一问题，提出了一种新的分布式小卫星系统误差补偿方法，该方法不需要迭代运算，可在基线误差控制在分米数量级的基础上对回波信号的空间导向矢量进行准确估计。计算机仿真验证了方法的有效性。     

基于小波和支持向量回归的高光谱遥感图像压缩

高光谱遥感成像技术能够获取探测对象丰富的空间信息和光谱信息,但所得图像海量数据的存储与传输制约了其应用。为此,提出了一种基于三维整数小波变换和小波支持向量回归的高光谱遥感图像压缩方法。首先采用三维整数小波变换把高光谱遥感图像分解成不同尺度的多个子带。然后对低频子带直接进行DPCM编码,而对高频子带则利用小波支持向量回归学习其小波系数之间的相关性,并采用小部分训练样本即支持向量来稀疏表示小波系数,以此达到压缩高频小波系数的目的。最后对支持向量及其相应的权重进行熵编码。文中给出了实验结果,并与基于3D SPIHT和JPEG2000的高光谱遥感图像压缩方法进行了比较,结果表明：所提出的方法在相同比特率下能够获得更高的峰值信噪比。     

空间运动体上梁的三维动力学建模和仿真

对附着在空间运动体上梁的动力学问题进行了研究,运用Lagrange方法建立了中心刚体作任意三维运动时,梁作横向振动和纵向振动的动力学方程,考虑了柔性梁的横向弯曲变形所带来的纵向位移,这种耦合变形使所得到的振动方程包含了动力刚化效应,这是与传统的梁振动模型的不同之处,最后通过仿真算例验证了该方法.      

An improved prediction model for corner stall in axial compressors with dihedral effect

Corner stall predictions are important and difficult in axial compressors. However, all of the prediction models have proved to be ineffective for advanced compressor blades, which tend to use the combined sweep and dihedral. As for the prediction parameter DL, although it effectively modeled the effects of the adverse pressure gradient and secondary flow, it failed to predict the corner stall of curved blades because the model failed to consider the intersection of the boundary layer at the corner region. In this paper, the shape factor gradient Ψ of the boundary layer at the corner region was investigated by numerically studying specially shaped expansion pipes under different adverse pressure gradients. The improved prediction parameter DJ was presented based on the model of Ψ and the circumferential pressure gradient ξ. A comparison of the critical range of the prediction parameters DL and DJ was investigated using the NACA65 cascade database, which was established by a numerical method. Then, the stall criterion was validated according to the experimental results of various test facilities with different blade geometries and experimental conditions. The results show that the improved prediction parameter is able to predict the corner separation/stall flows and is in good agreement with the experimental results for axial compressors with three-dimensional designed blades.     

法拉第型磁流体发电机试验和数值仿真

针对未来航空航天任务对大功率空间电源的迫切需求，开展了国内首次高温惰性气体法拉第型磁流体发电机试验研究。试验采用电弧加热器作为模拟热源，以氩气作为工质，添加铯作为电离种子以提高工质电导率，成功实现了对法拉第型磁流体发电机的原理性验证，在1 T磁场环境的试验条件下取得了最高194 W的发电功率，功率密度为866 kW/m³。根据试验条件对发电过程进行了三维数值模拟，分析结果表明：发电机输出性能受电极压降和工质速度的影响较大，需要在后续研究中改进发电机工艺以降低电极压降，并对加速喷管重新进行设计。     

Solar atmosphere wave dynamics generated by solar global oscillating eigenmodes

The solar atmosphere exhibits a diverse range of wave phenomena, where one of the earliest discovered was the five-minute global acoustic oscillation, also referred to as the p-mode. The analysis of wave propagation in the solar atmosphere may be used as a diagnostic tool to estimate accurately the physical characteristics of the Sun’s atmospheric layers.In this paper, we investigate the dynamics and upward propagation of waves which are generated by the solar global eigenmodes. We report on a series of hydrodynamic simulations of a realistically stratified model of the solar atmosphere representing its lower region from the photosphere to low corona. With the objective of modelling atmospheric perturbations, propagating from the photosphere into the chromosphere, transition region and low corona, generated by the photospheric global oscillations the simulations use photospheric drivers mimicking the solar p-modes. The drivers are spatially structured harmonics across the computational box parallel to the solar surface. The drivers perturb the atmosphere at 0.5?Mm above the bottom boundary of the model and are placed coincident with the location of the temperature minimum. A combination of the VALIIIC and McWhirter solar atmospheres are used as the background equilibrium model.We report how synthetic photospheric oscillations may manifest in a magnetic field free model of the quiet Sun. To carry out the simulations, we employed the magnetohydrodynamics code, SMAUG (Sheffield MHD Accelerated Using GPUs).Our results show that the amount of energy propagating into the solar atmosphere is consistent with a model of solar global oscillations described by Taroyan and Erdélyi (2008) using the Klein-Gordon equation. The computed results indicate a power law which is compared to observations reported by Ireland et al. (2015) using data from the Solar Dynamics Observatory/Atmospheric Imaging Assembly.     

Multi-point observations of earthward fast flow in the plasma sheet by virtual satellites located in the MHD simulation domain

Time profiles of some physical values in earthward fast flows in the plasma sheet are observed at three dimensionally different positions by employing virtual satellites located in the three-dimensional magnetohydrodynamic simulation domain, and these simulations are done on the basis of the spontaneous fast reconnection model. In the spontaneous fast reconnection evolution, the width of the flow channel is narrow in the dawn-dusk direction, and it does not spread until the plasma collides with the magnetic loop. The enhancements in B_z and V_x are larger at the center of the fast flow channel than those at its dawn and dusk edges, reflecting the differences in the reconnection rate in the diffusion region. The enhancement in V_x is shorter near the plasma sheet boundary layer than that near the neutral sheet, reflecting the changes in the thickness of the flow channel.     

Closing address

Impressions from the workshop are summarized. Difficulties within the present observational and theoretical context are outlined and directions for fruitful future work are indicated. The workshop subtitle, the interface between MHD and plasma physics, still appears to be a goal for the future, though some encouraging results have been reported at this workshop.     

Composite impact vector control based on Apollo descent guidance

A new three-dimensional missile guidance law to control the impact vector against a stationary target is proposed. The composite guidance law has two well-known components: Apollo descent guidance and trajectory shaping guidance. These respectively linear and planar guidance laws are combined to achieve a specified impact direction. The main idea is to define an impact plane and to steer the missile onto this plane using Apollo descent guidance while concurrently performing trajectory shaping wi...