嵌入式大气数据传感系统压力传感器设计研究

嵌入式大气数据传感(FADS)系统较之传统的大气数据系统有很大的优势,它依靠飞行器前端的压力传感器间接得到飞行大气数据.在本文中,首先简要介绍了FADS系统的压力模型;然后通过分析压力传感器几何外形设计对系统性能的影响,建立了压力传感器的动力学模型,并提出了FADS系统中的压力传感器的设计准则;最后给出了仿真结果.     

风挡防（除）雾表面瞬态热特性计算

风挡表面瞬态热特性计算是热空气射流防（除）雾系统设计的重要内容。在分析风挡防（除）雾换热机理的基础上，建立了风挡表面瞬态热特性的计算模型，用差分法对其求解。通过计算机模拟，得出计算结果，与试验结果比较，计算误差小于５％，研究的内容，具有工程实用价值。     

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.     

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。     

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。     

方形膜片压力敏感元件的频率特性

方形膜片是一种先进的敏感压力的谐振子。其于板的大找度变形理论，建立了被测压力与谐振子固有频率的数学模型，计算机、分析了谐振子的几何参数对振动特性的影响规律，得到了在给定压力得程内，对确定材料的膜片其固有频率相对零压力频率的变化率只与其边长、膜片厚的比值有关的重要结论，为设计该类谐振子提供了理论依据。     

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.     

Solar wind dependence of the Pc1 wave activity

There are a host of factors influencing the excitation of Pc1 geomagnetic pulsations, which are ULF waves in the frequency range between 0.2 and 5 Hz. We have studied carefully the dependence of the pearl-type Pc1 activity at Sodankylä, Finland (L = 5.1) on the plasma density N in front of the magnetosphere, the bulk velocity V of the solar wind, and the intensity B of the IMF. The result is as follows: high values of N and reduced values of V are favorable to appearance of Pc1, whereas the dependence of Pc1 activity on B is practically absent. We also show that the probability of Pc1 occurrence decreases with the interplanetary electric field, and increases with solar wind impact pressure and with the plasma to magnetic pressure ratio “beta”.