GaInP2外延膜中施主—受主对复合发光带的能量关量

通过变温与变激发强度的近红外光致发光研究了用ＭＯＣＶＤ方法、生长在ＧａＡｓ衬底上的Ｇａ０．５Ｉｎ０．５Ｐ（ＧａＩｎＰ２）外延薄膜的１．１７ｅＶ发射带的发光特性。１．１７ｅＶ发光带性质与０．９９ｅＶ及０．８５ｅＶ发光带的性质有着明显的差别。１．１７ｅＶ发光带的机理可用施主－受主对的复合发光来解释，其中施主－受主对系白处在Ｇａ格位上的Ｓｉ（ＳｉＧａ）及其最邻近的Ｇａ空位（ＶＧａ）所组成，记作ＳｉＧａ－ＶＧａ。考虑到ＧａＩｎＰ２中存在着很强的电子－格子耦合作用及其Ⅲ族子格子为部分有序，所以在施主－受主对复合发光中应计及Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ位移△ＦＣ及该对在等效的部分有序势场中的相互作用能Ｅｓ（ＤＡＰ）。Ｘ—射线衍射实验表明，部分有序结构相当于成分调制，因而可用Ｋｒｏｎｉｇ－Ｐｅｎｎｅｙ模型来计算Ｅｓ（ＤＡＰ）值。这样，我们就导出了施主－受主对复合发光的新的能量表示式。     

基于正弦基础激励的航天器结构模型修正方法

正弦振动试验是航天器系统级和单机产品需要开展的常规试验,充分利用工程中积累的正弦试验数据进行结构模型修正具有重要的工程意义。文章首先介绍了基础激励下结构模型修正方法,通过矩阵分块、待修正参数归一化、参与修正的频率点选择等步骤,推导出基于基础激励的模型修正公式;然后对国际通用算例GARTEUR桁架结构的有限元模型进行修正,分析修正后模型在修正频段内和修正频段外计算所得模态频率,验证修正后模型对模态频率的复现和预示能力,通过对比试验模型、分析模型和修正后模型中4个典型节点的响应曲线,检验修正后模型精度。结果表明:修正后模型的模态频率和响应曲线均与试验模型趋于一致,证实了该修正方法对GARTEUR结构修正的有效性。     

快速阀门同步控制系统

本文阐述了自在由飞弹道靶试验中,利用微波相干原理,取得模型运动的起步信号,经过与模型运动速度相对应的延时后,去触发控制电路,引爆阀体内的电雷管,控制阀门的开启和关闭的同步控制系统。     

Injection of 40-kHz-modulated electron beam from the satellite: II. Excitation of electrostatic and whistler waves

Beam-plasma interaction effects are studied during the active space experiment with electron and Xe-ion beam injections in an ionospheric plasma. Permanent 40-kHz-modulated electron beam injection occurs simultaneously with a xenon-ion beam injected by the Hall-type plasma thruster operating in a square-pulse mode (100/50 s for a job/pause duration). The unusual behavior of the background charged particle fluxes and wave activity stimulated during the beam-plasma interaction have been registered by the scientific instruments onboard Intercosmos-25 station (IK-25) and Magion-3 subsatellite. The longitudinal and electromagnetic wave instabilities and their mutual relationship are considered in order to explain the observed effects. The excitation of electrostatic waves by the electron injection has been considered for different resonance conditions near the linear stability boundary. Beam-driven electromagnetic instability is responsible for the backward-propagating whistler waves excited via cyclotron resonance. Competition of these two beam instabilities is one of the subjects of the present study.     

Analysis of the data processing strategies of spherical harmonic expansion model on global ionosphere mapping for moderate solar activity

Spherical harmonic (SH) expansion is widely used to model the global ionosphere map (GIM) of vertical total electron content (VTEC). According to the impact of different data processing methods of the SH expansion model on the VTEC maps, we specifically performed comprehensive analysis in terms of the data sampling rate, the time resolution, the spherical harmonic degree, and the relative constraint. One month of GPS data (January in 2016) from the International GNSS (Global Navigation Satellite System) Service (IGS) network in a moderate ionospheric activity period at the descending phase of Solar Cycle 24 was processed. To improve the computational efficiency of the daily GIM generation, the data sampling rate of 5?min was recommended allowing the GIM precision loss within 0.10 TECU (total electron content unit). The global VTEC map could be better represented in temporal and spatial domains with higher time resolution and higher spherical harmonic degree, especially at low latitude bands and in the southern hemisphere. The GIM precision improvement was about 10.91% for 1-h and about 15.15% for 0.5-h compared with the commonly used 2-h time resolution. The use of spherical harmonic degree 17 or 20 instead of 15 could improve the precision by 3.19% or 6.06%. We also found that an optimal relative constraint had to be found experimentally considering both the GIM precision and the GIM root mean square (RMS) map.     

电传系统的谐波振荡

从舵回路非线性特性的研究入手,通过频谱分析和实验验证,揭示了高增益电传系统中三角波的高频奇次谐波激发舵面抖振的物理本质,并给出电传系统谐波振荡的必要条件、抖振的频率特征以及防排措施,对现代飞行控制系统的设计具有重要参考作用。     

裂纹转子非线性振动特征的谐波小波与分形识别

通过对谐波小波的分析研究,指出了谐波小波对振动信号局部频段分析的优良特性。采用谐波小波对裂纹转子的非线性振动信号在低频段进行了分析。理论分析与实验结果表明:对实际裂纹转子信号,经谐波小波的频段分析后,能够得到通常难以由理论分析与实验结果获得的非整数倍周期分叉的非线性特征频谱。计算了裂纹转子的分形维数,发现裂纹转子的振动信号比理论结果要复杂、可以用多重分形作为判断实际转子是否有裂纹的一个特征。提出了用谐波小波变换后的奇异谱来识别裂纹转子非整数倍周期分叉的非线性特征频谱的方法,并对实际转子信号进行分析,得到了明显的非整数倍周期分叉的奇异谱。      

利用经验正交函数分解的大气密度模式校准方法

热层大气密度产生的阻力是作用在低轨航天器上最大的非引力摄动,现有大气密度模式存在15%~20%的偏差,难以满足空间任务应用需要。采用NRLMSISE-00模式作为密度参考标准,通过修正Jacchia-Roberts经验大气模式温度参数校准密度,建立温度修正量与密度的参数方程。针对部分区域修正量迭代计算发散问题,采用改进高斯牛顿迭代法求解方程。选择经验正交函数（EOF）分解方法分析修正量的时空特征,并与传统球谐（SH）分析的结果进行比较。结果表明,前4阶EOF基函数与前9项球谐基函数分别可提取温度修正量超过85%与80%的变化特征,EOF分解方法对温度修正量的表示效率高于球谐分析方法。第1阶EOF基函数反映了温度参数的整体偏差,第2~4阶EOF基函数对应的时间系数表明温度修正量的变化具有天周期性,且球谐分析得到的时间系数同样具有天周期性的特点。利用前4阶EOF基函数和前9项球谐基函数重构的温度修正量校准Jacchia-Roberts模式,校准后的模式密度偏差分别下降了9.06%与5.37%,表明EOF分解方法与传统球谐分析方法相比,能够更有效地修正温度参数,改进模式精度。     

电容均压三相四开关变换器预测功率控制

三相四开关变换器直流侧分离电容电压不平衡,将降低其并网电能质量,缩短电解电容寿命。针对该问题,提出了一种直流侧分离电容电压均衡的模型预测功率控制策略。基于αβ两相静止坐标系分析电压矢量,建立功率预测模型。由于直流侧电容中点电压偏差值含有交流分量和直流分量,使用低通滤波器提取直流分量后计算功率补偿值,并计入给定功率,进行模型预测功率控制,实现直流侧分离电容电压均衡。该控制策略无需锁相环和PWM调制,易于实现。通过仿真和试验对其动、静态特性进行分析,验证了所提出控制策略的有效性和可行性。     

Structural and collisional data for Mg III and Al IV

We present in this work energy levels, oscillator strengths, radiative decay rates and fine structure collision strengths for the Mg III and Al IV ions. The 11 configurations: (1s²) 2s²2p⁶, 2s²2p⁵3l, 2s2p⁶3l, 2s²2p⁵4l   (l?n-1$l?n-1$, where n is the principal quantum number), yielding the lowest 75 levels are used. The collisional data for these two ions are missing in the literature, especially the database CHIANTI, this is the principal motivation behind the present work. Calculations have been performed using the AUTOSTRUCTURE code. AUTOSTRUCTURE treats the scattering problem in the distorted wave approach. Fine structure collision strengths are calculated for a range of electron energies from 10 Ry to 240 Ry. The atomic structure data are compared to available experimental and theoretical results.