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.     

基于粗集的调度Agent知识库建模研究

首先通过相识集、招标集、投标集和中标者的概念，描述了车间调度系统中的调度Agent与资源Agent间任务分配的招投标关系；运用粗集理论，基于任务的属性和资源Agent完全任务的成本、质量、负荷和时间等属性构造决策表；在分析了决策表的特征基础上，生成调度规则集，即调度知识库；最后给出车间调度Agent的调度过程算法。     

应用聚类分析对关联规则进行分组

关联规则是要从大量的数据中找到数据之间的规律，但有时所产生的规律十分繁多，从而形成新的知识管理问题。针对该问题本文提出了一个新的算法，该算法利用系统聚类分析方法对规则进行分组，从而可更好地帮助用户解所发现的规律，该方法的距离（RatioD）是基于关联规则本身，因此，可对规则进行高效地分组。实验结果表明，该算法是有效的。     

用于导弹系统性能统计分析的统计线性化伴随法

本文在研究ＳＬＡＭ方法基础上，进行了理论推导和计算方法方面的改进，并将此方法应用于导弹系统性能的统计分析，计算机仿真结果表明该方法与采用ＣＡＤＥＴ方法的结果完全一致。     

太阳同步卫星轨道参数的容许偏差分析

飞行任务对卫星轨道提出指标要求，这些指标决定了卫星轨道参数的容许偏差范围。结合太阳同步(准)回归轨道卫星的轨道特性，针对覆盖重叠率、太阳同步等指标，使用解析方法讨论了大气阻力摄动影响下轨道参数的容许偏差，通过分析可以初步确定轨道控制策略及能量需求，最终为轨道保持方法的设计提供参考和依据。     

无穷观问题的研究(Ⅲ)——‘每一''与‘所有''

本组系列论文（I）－（Ⅴ）从数学和认识论的角度系统地研究了无穷观问题的历史发展和现状，确立了无穷观背景世界的三分法原则，指出了两种穷观相互排斥的局限性，形成了统一两种无穷于同一框架中的基本观点，并建立了一个统一实无限与潜无限于同一框架中的公理集合论系统APAS。     

低纬地磁Z分量的半年变化

利用武汉、广州、泉州和琼中等4个低纬地磁站连续多年的地磁资料，计算了各月5个磁静日Z分量日均值与中午1100---1300时段平均值之差(Dz)，对每年12个Dz采用多元回归分析方法，得到各年的半年变化幅度和相位．结果表明：4个站的Dz每年都有半年变化现象；半年变化幅度与太阳活动有关，一般来说，太阳活动高年Dz半年变化幅度明显大于太阳活动低年；太阳活动本身的半年变化，对Dz半年变化幅度有显著的调制作用；Dz半年变化的相位在3—4月(或9—10月)，即极大值出现在分季；低纬地区地磁Z分量存在显著的半年变化，能够反映赤道电急流也有明显的半年变化，这再一次证明，赤道电急流幅度的半年变化，通过“喷泉效应”使得电离层，f0F2产生半年变化，其是产生，f0F2半年变化的一个主要因素．     

临近空间立法问题研究及对技术发展的影响

当前学界关于临近空间的争议焦点主要集中在临近空间是否应当成为法律概念,以及临近空间是否应当成为法律上的独立空间两方面。随着在临近空间的利益冲突愈演愈烈,临近空间应上升成为独立的法律概念。在当前空天划界问题悬而未决的特殊背景下,宜认定其从属于空气空间,赋予领空主权。鉴于当前临近空间国际法规则尚处于空白阶段,应积极引领和推动临近空间国际法规则的制定,倡导设立临近空间的无害通过制度,同时加快发展临近空间技术,不断增强技术实力,为后续临近空间国际法规则制定增加博弈砝码。     

密集编队中飞机发动机的疲劳损伤差异

选取典型密集编队飞行任务,利用实测飞行数据,研究了在飞行动作几乎完全相同的条件下飞机发动机疲劳损伤的差异.经过二次雨流法统计循环次数和线性累积损伤理论折合到标准循环,得出了密集编队中长、僚机因位置不同而造成的发动机疲劳损伤的差异及其统计规律,发现疲劳损伤差异分布为威布尔分布,单机差异一般为2～4倍,最大可以达到9～10倍.进一步揭示了发动机疲劳载荷/损伤的分散性和单机疲劳寿命监控的必要性.