The Full Flowpath Analysis of a Hypersonic Vehicle

对一种类X43-A吸气式高超飞行器全流道开展了M7一级的三维数值仿真研究,深入探索了进气道处于起动状态和不起动状态时全流道的冷流流场结构和和气动力特性,且部分结果与实验数据进行了对比。研究结果表明:(1)前体横截面上存在显著的展向压强梯度,使得经过预压缩的气流偏离了进气道进口,但同时也减少了进入内通道的边界层气流,提高了进口流场的品质;(2)后体喷流股的膨胀过程受到了周围外流的显著干扰,因而沿流动方向其截面形状不断发生变化,如在喷口附近为近似矩形,而在后体末端附近则演化为近似三角形;(3)当进气道处于不起动状态时,其全流道流动结构发生了显著变化,进气道的外部压缩波系往复振荡,尾喷管出口的喷流股也在不停的膨胀和收缩,具有极强的非定常特征;(4)当进气道处于不起动状态时,全机的气动力特性呈周期性变化,升阻比的变化幅度较大,在最大、最小值分别可达起动状态的2倍和1/4倍。另外,升力、阻力系数的变化曲线之间存在一定的相位差;(5)与实验结果的对照表明,所采用的数值仿真方法具有较高的精度。     

Ion dynamics associated with Alfven wave in the near-Earth magnetotail: Two-dimensional global hybrid simulation

Ion dynamics in the near-Earth magnetotail region is examined during periods of fast Earthward flow with a two-dimensional (2-D) global-scale hybrid simulation. The simulation shows that shear Alfven waves are generated at x ∼ −10R_E, where the strong earthward flow is arrested by the dipole field, and propagate along field lines from the equator to both southern and northern polar ionosphere. Non-gyrotropic ion velocity distributions occur where the large-amplitude Alfven waves are dominant. The simulation indicates that the Alfven waves are generated by interaction of the fast earthward flow with the stationary near-Earth plasma. Beam ions are found to be pitch-angle scattered and trapped in the wave field, leading to the non-gyrotropic ion distributions in the high-latitude plasma sheet boundary. In addition, significant particle heating and acceleration are found to occur behind the dipolarization front due to the effect of wave turbulence.     

Improvement in the GERB short wave flux estimations over snow covered surfaces

Because space-borne radiometers do not measure the Earth’s outgoing fluxes directly, angular distribution models (ADMs) are required to relate actual radiance measurement to flux at given solar angle, satellite-viewing geometries, surface, and atmospheric conditions. The conversion of one footprint broad-band radiance into the corresponding flux requires therefore one to first characterize each footprint in terms of surface type and cloud cover properties to properly select the adequate ADM.

A snow (and sea-ice) retrieval technique based on spectral measurements from the Spinning Enhanced Visible and Infrared Imager (SEVIRI) on board Meteosat 8 is presented. It has been developed to improve the scene identification and thus the ADM selection in the near-real time processing of the Geostationary Earth Radiation Budget (GERB) data at the Royal Meteorological Institute of Belgium. The improvement in the GERB short wave flux estimations over snow covered scene types resulting from angular conversion using dedicated snow ADMs (e.g., empirical snow ADMs and/or pre-computed theoretical snow ADM) instead of empirical snow-free ADMs is discussed.     

RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium

The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral distribution of natural plasma waves, and monitor dust and gas activities around the nucleus. The MIP instrumentation consists of an electronics board for signal processing in the 7 kHz to 3.5 MHz range and a sensor unit of two receiving and two transmitting electrodes mounted on a 1-m long bar. In addition, the Langmuir probe of the RPC/LAP instrument that is at about 4 m from the MIP sensor can be used as a transmitter (in place of the MIP ones) and MIP as a receiver in order to have access to the density and temperature of plasmas at higher Debye lengths than those for which the MIP is originally designed.     

分布式电能计量与计费系统中通信信道特性与实现方案的研究

本文介绍了分布式电能计量与计费系统中低压电力线作为载波通信信道时的信道特性，给出了实验数据和特性曲线，并选择了通信的基本方案。     

基于重复控制技术的航空静止变流器

针对航空静止变流器输出电压波形畸变的问题,提出了采用重复控制技术解决方案.重复控制的基本思想是控制理论中的内模原理,逐周期地消除控制误差.分析了重复控制补偿器的数学表达式;证明了重复控制系统的稳定性和收敛性;给出了控制器各环节参数的频域设计方法;并根据一台采用单极性倍频正弦脉宽调制(SPWM)的6kVA/50Hz/200V航空静止变流器的实际参数进行仿真验证.仿真结果表明了控制模型和参数设计方法的正确性,同时也验证了重复控制对解决逆变电源受基波整数倍周期性信号干扰或带非线性负载所造成的输出电压波形畸变是行之有效的.      

核辐射对透波材料介电性能影响

用加速老化试验的方法,在有氧存在的条件下,研究了TDE-85环氧树脂/E玻璃纤维体系、4501A双马来酰亚胺树脂/D3W玻璃纤维体系2种透波材料介电性能受核辐射影响的规律.用60Co辐射源在辐射量为50~800kGy范围内对样件进行辐射,用波导法测试样件的介电常数和介电损耗,测试频率为10GHz.结果发现2种体系透波材料介电性能受核辐射的影响较小,且后者比前者具有更好的抗辐射稳定性.同时利用IR,TGA等手段研究了材料介电性能变化的原因.      

闭口管内气体非线性振荡研究

采用新型的计算效率较高的ＥＮＯ差分模式,从一维非定常Ｅｕｌｅｒ方程出发,对受扰动气体在闭口管内的传播现象进行了数值模拟。计算发展小扰动情况下,当激振频率接近管内气体的固有频率时会发生非线性振荡,有激波产生;但当扰动较大时,激振频率的影响变得不明显。     

中高层大气行星波与惯性重力内波的非线性相互作用

在弱非线性理论基础上,将三维大气中行星波和惯性重力波从原始非弹性近似方程中分离出来,讨论了典型的2天行星波与惯性重力内波的非线性相互作用过程.从共振曲面和参量不稳定增长率来看,行星波倾向于与空间尺度较大的惯性重力波发生相互作用.利用潮汐波的等价重力波假设,讨论了2天行星波与半日潮及9.6h惯性重力波的相互作用,三波相互作用时能量守恒.非线性相互作用使2天波和潮汐波的波幅受到长期调制.      

SH波对结构表面上含有多个半圆形介质夹杂的散射

利用复变函数和多极坐标系的方法,研究了在结构表面上含有多个半圆形介质夹杂的散射问题,首先给出 SH波对多个半圆形介质夹杂的散射波函数,并利用多极坐标系的方法,来满足介质界面上的连续条件和表面上的边界条件,归结为对一组无穷代数方程组的求解,简化了问题的求解。作为算例,对结构水平面上含有 2个半圆形夹杂介质进行分析,并讨论了夹杂介质参数的变化及孔距对位移的影响。