Variations in the thermosphere and ionosphere response to the 17–20 April 2002 geomagnetic storms

The responses of the thermospheric density and ionospheric foF2 to the intense magnetic storms event on 17–20 April were analyzed by using data from CHAMP/STAR and ionosonde stations respectively, and NRLMSISE-00 and IRI-2007 models were used to simulate. The models can capture the tendency of changes, especially under quiet or moderate geomagnetic conditions, but are less accurate under geomagnetic storms. The thermospheric density is sensitive to the EUV emission and geomagnetic activity, and double-peak structure appeared in the dayside. On 19 April dayside, TADs traveled toward the equator with phase speeds of the order of 300–750 m/s, interfered near the equator to produce a total density perturbation of 25%, and then passed through each other and into the opposite hemisphere. For ionospheric foF2, there are non-symmetric hemispheres’ features during the intense geomagnetic activities. In details, middle latitudes in the north and high latitudes in both hemispheres are negative ionospheric storms, and the maximum amplitudes of δfoF2$\delta \mathit{foF}2$ is about 60%, but the amplitudes decrease from the higher to lower latitudes in the Southern Hemisphere. Meanwhile, the equatorial station shows positive phase, and the maximum value is about 100%. Finally, the mechanisms for these features will be discussed in this study.     

S弯进气道旋流缩涡实验研究

本文提出的旋流缩涡法采用了一种结构简单的缩涡器, 是一个金属薄片弯成的框架。这个缩涡器框架被安置在进气道喉道前, 通过4个薄片固定在模型上。实验研究表明:该法可缩小由S弯进气道进口分离所造成的单涡旋流作用范围, 并提高出口截面平均总压系数。      

航天器实验模型的热网络分析

采用航天器热控系统设计中常用的热分析计算方法——节点网络法,对一航天器实验模型进行了温度计算,并将计算结果与实验数据进行了比较。采用修正后的网络系数,大部分仪器温度计算值与实验值差值的绝对值在３℃以内,少数在３℃～５℃之间,极个别超过５℃。     

复杂地形下基于三视约束的景象匹配方法

 景象匹配通过将飞行器实拍图像与机载的基准图像比较而进行导航。当飞行高度较低时,由地面大起伏引起的实时图几何变形会严重影响匹配性能,造成匹配精度下降甚至出现误匹配,这一问题严重制约了现有景象匹配系统的应用范围,比如无法应用于建筑林立的城镇地区和梯田、丘陵地带。本文首先推导了小视场内无几何变形的高空竖直透视投影模型;在此基础上,依据三视约束关系,把相邻两幅下视实时图像的特征赋给该透视模型所成的像,得到消除几何变形的特征模板,再和基准图进行匹配。因此,所提方法不仅能处理由飞行器姿态引起的实时图几何变形问题,而且适用于城镇等地面存在较大起伏的地形。理论分析和仿真实验表明,该算法取得了较好的结果,具有良好的环境适应能力,实用性较强。     

S弯进气道中静压场研究

本文给出了 S弯进气道出口截面上的静压场测量结果。研究表明 ,在不同的进气攻角下 ,S弯进气道出口截面上的静压是不均匀的。攻角愈大 ,静压场畸变愈严重。在进行旋流场研究中 ,如果攻角较大 ,需认真考虑以往壁面 4点线性加权平均压力场处理所带来的误差影响     

合成气组分及雷诺数对火焰结构影响的实验研究

利用非接触的激光PLIF技术测量了在湍流贫燃预混燃烧中的OH自由基分布。以典型煤制合成气真实组分为基础进行工况设计,分为H2含量变化、CO/（CO＋CH4）相对比例变化、雷诺数变化和中低热值对比4部分进行实验。通过OH-PLIF信号分析,探讨了H2含量、CO/（CO＋CH4）相对比例和雷诺数对燃烧的影响。实验结果表明,雷诺数、H2含量和CO/（CO＋CH4）相对比例的变化对合成气燃烧过程都有显著的影响。其中雷诺数的增大和H2含量的增加都加强了OH-PLIF信号强度,即有利于火焰中OH自由基的生成。而CO/（CO＋CH4）相对比例的上升,因同时减少了CH4含量,导致OH自由基浓度下降。H2含量的升高和CO/（CO＋CH4）相对比例的上升（转折点前）对于火焰行程都有缩短的作用,强化了燃烧。转折点之后CO/（CO＋CH4）相对比例的继续上升不利于燃烧。后文对裂解气火焰瞬时图像和火焰面密度的分析印证了上述规律。     

HTPB推进剂凝胶分解特性与老化性能的相关性

研究了贮存老化过程中 HTPB推进剂凝胶的氧化反应热效应与推进剂力学性能之间的相关性。实验表明 ,HTPB推进剂贮存老化过程中 ,凝胶的氧化反应热效应与推进剂最大强度下的延伸率 ,二者之间存在很好的线性相关性 ,为进一步快速预估 HTPB推进剂的贮存寿命 ,提供了一种样品用量少、快速简便的新方法     

基于二进小波阈值决策的血管内超声图像噪声抑制

针对血管内超声图像中血液散射引起的斑点噪声,提出了一种基于小波多尺度分析的非线性去噪算法,在二进小波变换域分别采用软阈值滤波法和硬阈值滤波法对不同尺度的小波系数进行非线性处理,并根据二进小波分解结构提出了一种局部阈值估计方法.实验结果表明,该方法在抑制血流斑点噪声的同时也较好地保留了图像边缘,有助于识别管壁和周围组织.     

基于异向介质的高增益圆极化微带天线的设计

文章提出一种基于人工异向介质(metamaterials)覆层的高增益圆极化微带天线。采用商业软件AnsoftHFSS对该天线的电特性进行了仿真。仿真结果表明,人工异向介质覆层将普通的圆极化微带天线增益从7.8dB增加到了11.4dB,同时保持了良好的圆极化特性,并且该天线具有结构简单、易于加工等特点。     

Interplanetary magnetic field control of plasma distribution in the polar ionosphere

We used the TEC (Total electron content) data of 5 min resolution obtained from the Madrigal database during solar-maximum winter (Nov. 6, 2000–Feb. 4, 2001) to study statistically the polar ionospheric plasma distribution response to different intensity and orientation of IMF By/Bz components. The sunlit high-density plasma extension from dayside to nightside is favored in negative IMF By and Bz conditions. With the magnitude of the negative Bz increasing, the time range corresponding to the distinct high-density extension feature expands, and the plasma density along the extension path enhances, which can be attributed to the interaction between dayside solar-produced ionization whose poleward limit is decided by terminator and convection extent mainly modulated by IMF Bz component. As for IMF By component influence on the sunlit plasma extension, the combination effect of convection and corotation electric fields is necessary to be considered.