27-day variation in solar-terrestrial parameters: Global characteristics and an origin based approach of the signals

The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ～27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ～27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation.     

横航向驾驶员诱发振荡研究及地面模拟验证

本文建立了包括非线性环节在内的横航向驾驶员—操纵系统—飞机本体组合系统的数学模型,采用闭环控制原理,对JJ-7飞机横航向驾驶员诱发振荡PIO问题进行了研究,并详细地讨论了驾驶员参数及其各种操纵动作、操纵系统和飞机本体气动参数对横航向PIO的影响,探讨了横航向PIO产生的机理。文中以JJ-7飞机为例,采用时域法在整个飞行包线各点进行了检查,并用固基飞行模拟器进行模拟验证。其结果与理论计算结果相一致。     

复合材料结构健康主动监测中激励信号的优化

利用L am b波频散方程及其数值求解得到的频散曲线,对L am b波模式及激励信号中心频率范围进行预测。建立了试验测试系统,利用集成在复合材料层合板上的PZT压电陶瓷片作为驱动器和传感器,激励并接收结构中激发的L am b波信号。对具有不同函数形式、中心频率和波峰数的信号激励,结构中传播的L am b波模式进行试验研究,为激励信号的选择与优化提供依据。利用H ilbert-Huang变换及H ilbert谱提取传感器信号特征,提出了L am b波信号在结构中传播时的能量衰减率和损伤敏感度两个考察指标,并据此对激励信号进行优化。实验结果表明,优化后的激励信号在结构中能激发出单一模式的L am b波(S0模式),有效地抑制了多模式现象的出现。同时,激发出的L am b波具有最低的能量衰减和最高的损伤灵敏度,响应信号特征明显,便于损伤识别。     

防止Ⅱ型驾驶员诱发振荡技术的研究

许多严重的飞行事故都与由速率限制引起的Ⅱ型PIO有关。针对如何预防PIO，首先介绍了自适应杆增益和软件限制环节的设计原理。然后以某带速率限制的电传飞机为例，运用同一理论，分析采用自适应杆增益和软件限制环节来改善速率限制的不利影响。仿真结果表明，自适应杆增益环节和软件限制环节都能抑制住PIO的发生，但两者组合加入抑制效果更好，飞行品质也能达到满意的程度。     

用胞映射法分析双线性结构刚度的机翼颤振

将映射轨迹追踪技术引入基于空间Poincar啨截面的胞映射方法中 ,并定义初值分析空间 ,以适应分析高维动力系统运动类型初值域的需要。改进后胞空间中胞的数目大大减少 ,计算时间缩短 ,运动特征的确认更为准确。应用该方法研究扭转方向具有双线性结构刚度因素的机翼颤振问题 ,结果显示 ,初始条件对系统动力学行为有着很大的影响。当两段刚度之比小于某临界值时 ,随着机翼颤振速度增大 ,不同的初始条件会导致平衡点、极限环振动、复杂的周期运动、混沌和发散运动等不同的运动形式     

气动谐振管加热振荡流动过程数值研究

为了了解气动谐振管加热现象的振荡流动过程，利用显式TVD－MacCormark格式数值求解二维轴对称雷诺平均N－S方程，获得了一个谐振循环中完整的喷嘴－谐振管系统的振荡流动湍流流场，结果表明，欠膨胀声速冲击喷流固有的流场不均匀性和不稳定性是谐振管加热现象产生的内在原因，激波耗散是谐振管主要的加热机理。     

迟滞非线性二元机翼颤振特性分析

 采用多项式迟滞非线性模型建立二元机翼气动弹性运动方程，并用数值积分法进行求解。通过系统响应振幅随来流速度变化的分叉图和频谱分析发现，俯仰方向由于含有非线性因素，振动中的高阶分量随速度提高不断增加，并引起高次分叉。重点研究“机翼/空气”质量比以及“沉浮/俯仰”两个自由度的自然振动频率比对非线性颤振速度边界的影响，并提出可以通过提高自然振动频率比来减小迟滞非线性因素的不利影响。     

移相全桥变换器寄生振荡的抑制方法研究

移相全桥变换器是中大功率直流/直流变换场合的一种理想拓扑,但在其输出整流桥上会产生寄生振荡,二极管上存在很高的尖峰电压。这将带来电路损耗并影响整流桥的使用寿命,因此应该想办法抑制。文中分析了寄生振荡产生的原因,介绍了几种可行的抑制方法,并进行了比较研究和实验验证。     

一类递归序列的稳定性和振动性

研究了递归序列x_(n 1)α-β_(n-1)/1-g(x_n),n=0,1,的持久性、振动性、稳定性和全局吸引性。其中α、β为正实数,g(x)是非负连续函数。     

A Possible Transfer Mechanism for the 11-Year Solar Cycle to the Lower Stratosphere

Observational evidence of the 11-year solar cycle (SC) modulation of stratosphere temperatures and winds from the ERA-40 dataset is reviewed, with emphasis on the Northern winter hemisphere. A frequency modulation of sudden warming events is noted, with warmings occurring earlier in solar minimum periods than in solar maximum periods. The observed interaction between the influence of the SC and the quasi biennial oscillation (QBO) on the frequency of sudden warmings is noted as a possible clue for understanding their mechanism of influence. A possible transfer route for the 11-year solar cycle from the equatorial stratopause region to the lowest part of the stratosphere is proposed, via an influence on sudden warming events and the associated induced meridional circulation. SC and QBO composites of zonal wind anomalies show anomalous wind distributions in the subtropical upper stratosphere in early winter. Mechanistic model experiments are reviewed that demonstrate a sensitivity of sudden warmings to small wind anomalies in this region. Various diagnostics from these experiments are shown, including EP fluxes and their divergence and also the synoptic evolution of the polar vortex, in order to understand the mechanism of the influence. Some recent GCM experiments to investigate the SC/QBO interaction are also described. They simulate reasonably well the observed SC/QBO interaction of sudden warming events and appear to support the hypothesis that tropical/subtropical upper stratospheric wind anomalies are an important influence on the timing of sudden warmings.