Coronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare

The 22 min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ond?ejov radiospectrograph in frequency range 1200–4500 MHz has been analyzed. We have found that the characteristic periods of about 60 s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200–4500 MHz. The behavior of individual wave trains at lower frequencies is different from that at higher frequencies. These individual wave trains have some common as well as different properties. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters in their wavelet power and global spectra are studied and discussed.     

The acceleration of Anomalous Cosmic Rays by stochastic acceleration in the heliosheath

Stochastic acceleration in the heliosheath appears to be a likely mechanism by which Anomalous Cosmic Rays (ACRs) are accelerated. However, most stochastic acceleration mechanisms are not appropriate. The energy density in the ACRs and in the interstellar pickup ions out of which the ACRs are accelerated greatly exceeds the energy density in the turbulence in the heliosheath. Thus, a traditional stochastic acceleration mechanism in which particles are accelerated by damping the turbulence will not work. A stochastic acceleration mechanism has been developed in which the total energy of the pickup ions and the ACRs is conserved. Energy is redistributed from the core pickup ions into a suprathermal tail to create the ACRs. A model for the acceleration of the ACRs in the heliosheath, based on this stochastic acceleration mechanism, is presented. The model provides reasonable fits to the spectra of suprathermal particles and ACRs observed by Voyager.     

SVIRCO contribution to the world-wide network of cosmic ray detectors

Since 1954 a research team (called SVIRCO) has been performing measurements of cosmic rays in Rome at La Sapienza University till 1997 and then at Roma Tre University. The experimental work carried out over more than 50 years is summarized in this paper. It describes: the early history of SVIRCO, the evolution from SVIRCO station to SVIRCO observatory, land and sea cosmic-ray surveys and the mini-network of neutron monitors, operating inside the world-wide network of cosmic ray detectors.     

The radiation environment in the ISS-USLab measured by ALTEA: Spectra and relative nuclear abundances in the polar,equatorial and SAA regions

We present here the energy spectra relative to different geomagnetic regions as measured by the ALTEA (Anomalous Long Term Effects on Astronauts) detector in the International Space Station – USLab from August 2006 to July 2007.     

改进的多处理器混合关键性系统可调度性分析

针对混合关键性系统的多重认证需求,研究多核处理器平台中全局调度算法fixed-priority and Earliest Deadline First by Virtual Deadline（fpEDF-VD）的可调度性分析问题。fpEDF-VD结合处理器利用率和虚拟截止期两个方面来计算任务优先级,系统可调度性取决于是否存在可行的虚拟截止期调整参数。考虑到现有可调度分析方法仅测试有限数量的调整参数候选值,不能有效地判定系统可调度性,故提出了一种改进的判定方法。该方法基于传统（非混合关键）任务调度算法fpEDF的可调度利用率约束条件,利用函数图像分析研究不同关键性级别的系统可调度性需求,并在此基础上给出有效虚拟截止期调整参数的确切范围。通过实例分析及与现有判定方法的比较,验证了该方法的正确性和高效性。与理论分析一致,基于随机生成任务集的仿真实验结果表明改进后的方法具有更优越的可调度性能,能显著地提高任务集的可调度接受率。      

基于优先级赤字轮询调度的WAIC网络延迟分析

航空电子机内无线通信（WAIC）在降低飞机重量和节省成本等方面的优势让其在航空电子系统的应用上具有可观的前景。为了研究基于802.11的WAIC网络的传输延迟并保证其可靠性,提出了一种优先级赤字轮询调度（PDRR）的介质访问控制（MAC）协议。首先,通过确定性网络演算方法为MAC层协议的活动建立了到达曲线和服务曲线模型。其次,充分考虑无线通信物理层的特点和所结合信道反转方法,给出了WAIC网络流量调度最坏情况下的端到端延迟的评价方法,可以发现信道反转后稳定的信道容量提供了较为保守的延迟界限。最后,通过案例分析对比了高优先级的WAIC节点与普通优先级节点的延迟界限以及信道反转的影响。结果表明:高优先级节点比普通优先级节点具有更好的实时性,并且可以通过增加平均信噪比来改善传输的延迟界限。      

Spacecraft survivability in the natural debris environment near the stable Earth-Moon Lagrange points

The theoretical analysis of the motion of natural space debris near the stable Earth-Moon Lagrange Points, $L_4$ and $L_5$, is presented with a focus on the potential debris risks to spacecraft operating near these points. Specifically, the research formulates a debris propagation model using four-body dynamics, then applies candidate probabilistic survivability models to a notional spacecraft operating at the $L_4$ and $L_5$ Lagrange points to quantify the collision risks to the spacecraft from natural debris particles. Of the survivability models implemented, the natural debris collision risks to spacecraft survivability are found to be incredibly low, but mitigation strategies to reduce the risk further are identified in this study. Overall, research into stable Lagrange point natural debris propagation improves understanding of the collision risks posed by the naturally occurring Kordylewski clouds and enhances operational planning for Lagrange point space missions.     

三维编织复合材料力学性能的实验研究

本文考察了三维编织方法的发展历史及应用背景,针对不同的编织方法,研究了所产生的编织复合材料基本“单胞”结构,以及不同编织参数对复合材料构件基本力学性能的影响,着重比较研究了二步法及四步法所形成构件与层合板构件的结果。采用反射光弹技术考察了编织复合材料的孔边应力集中现象,得到了有益的结果。本文针对三维立体织物的特点,研究使用了RTM成型工艺,得到了较好的编织试验件。     

利用三维激光测速方法研究悬停状态下的桨尖涡

利用三维多谱勒激光测速仪，对悬停状态下模型旋翼桨叶附近的流场进行了实验测量。研究了悬停状态下桨盘附近的流场特征、旋翼桨尖涡的形成和发展，以及桨尖涡对后续桨叶的影响     

基于含间隙吸振器的半主动振动控制

提出一种基于刚度分段线性动力吸振器的半主动振动控制策略，通过调节弹性元件的间隙实现吸振器工作频率连续跟踪外激励频率的变化。文中根据基波平衡导出了使主系统近似完全消振所需的弹性元件间隙控制律。数值仿真表明：这种半主动控制策略对于单自由度主系统和多自由度主系统均有很好的消振效果和相当宽的工作频带