One-up on L1: Can X-rays provide longer advanced warning of solar wind flux enhancements than upstream monitors?

Observations of strong solar wind proton flux correlations with ROSAT X-ray rates along with high spectral resolution Chandra observations of X-rays from the dark Moon show that soft X-ray emission mirrors the behavior of the solar wind. In this paper, based on an analysis of an X-ray event observed by XMM-Newton resulting from charge exchange of high charge state solar wind ions and contemporaneous neutral solar wind data, we argue that X-ray observations may be able to provide reliable advance warning, perhaps by as much as half a day, of dramatic increases in solar wind flux at Earth. Like neutral atom imaging, this provides the capability to monitor the solar wind remotely rather than in situ.     

Propagation of interplanetary shocks into the Earth’s magnetosphere

This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper.     

利用F区电离层特性参量获取等效中性风的方法及讨论

讨论利用电离层特性参量获取F层峰值高度附近中性风信息的三类方法.这些方法主要有:传统的和改进的伺服理论方法、借助电离层模式和数据同化思想的方法和刘立波等提出的方法.并以美国Millstone Hill非相干散射雷达浓度剖面和离子速度数据,以及澳大利亚Beveridge(37°S,144°E)FPI风场和测高仪数据为个例,初步考察利用电离层特性数据导出的等效中性风与观测值的一致性.     

视频测量方法在风洞模型姿态角测量中的应用

在现代的风洞模型试验测量中,角度测量误差所引起的阻力系数误差大约占总阻力系数误差的1/4,准确地测量模型的实际角度是提高数据准确度的一个重要因素。应用视频测量原理,通过图像处理的方法动态实时采集计算模型的实际角度值,模型角度的测量精密度可达0.01°,测量准确度可达0.015°。测量速率每秒25次。     

粉尘运动风洞模拟试验的相似律

本文提出了粉粒状堆料风吹起尘规律研究的相似律和在装卸作业中风吹扬尘规律研究的相似律,所获得的一些相似律,经大小两个风洞试验验证是较为满意的,并以此为指导,对煤堆起尘和煤炭装卸中起尘作了大量风洞模型试验,其结果表明也是合理的。     

直接数字频率合成器(DDS)及其性能分析

介绍了直接数字频率合成器DDS(Direct Digital Synthesizer)的组成、工作原理及性能;运用信号系统理论和方法详细分析了DDS的相位噪声、杂散噪声、数字化截断误差对输出波形的影响以及DAC非线性对频谱纯度的影响等;还给出了相应的分析计算公式和响应曲线;得出的结论对提高DDS输出信号的质量有一定意义.     

飞机座舱风档复合玻璃结构优化设计

提出了和析的含透明导电膜的多层复合玻璃优化结构。这种复合玻璃在电磁波频率８－１８ＧＨｚ范围内有很高的电磁波功率反射率。在可见光波长０．４０－０．７６μｍ范围内有高的透光率，该复合玻璃可以用于飞机座舱风档结构，也可以用于大容器微波防护系统。     

微放电效应部件设计研究

分析了影响微放电效应阈值电平的几种因素。对微放电效应部件设计的一般步骤和方法进行了论述 ,给出了具体的设计实例 ,并对微放电效应部件设计中需要注意的问题进行了说明     

太阳风中的动力论Alfven激波

本文指出因动力论Alfven波的存在非线性作用，从而能引起波连续陡化;这种情况下考虑频散效应，理论上应该形成中间激波.针对这一物理思想，在二元流体模型下，引进离子声反常阻尼，数值解出中间激波的结构.     

我国深空探测任务电源系统发展需求

针对我国后续月球极区探测、小天体探测、火星探测、木星系探测深空探测重点任务,在梳理分析每个探测任务约束的基础上,提出电源系统的具体需求;对上述4个方向的深空探测任务的电源系统需求进行归纳总结,提出我国后续深空探测任务的电源系统主要发展建议,具体包括宽温度和光强适应性、抗辐照的太阳电池阵,轻小型智能化的电源控制装置,高功率密度的电源系统MPPT拓扑;最后对同位素温差发电技术进行了发展展望,为后续深空探测电源系统研究和设计提供参考。