扇面波导中馈电探针输入电阻数值计算

推导出扇面波导中激励探针的等效输入电阻表达式，探针是伸入波导中的同轴线的内导体，在Ｘ波段，计算了输入电阻值随着探针伸入波导中不同长度的变化。     

扇面波导斜缝特性的矩量法分析

根据缝隙口面切向场的连续条件,采用解析数值法--矩量法,对扇面波导宽壁上窄的斜缝进行了计算,解得了磁流系数及其分布,并得到散射场、等效散射参量及等效阻抗等重要参数.假定波导中仅有TE-11主模传输,在X波段计算了散射参量和归一化等效串联阻抗,给出计算结果,为缝隙天线和缝隙阵列设计提供了依据.     

圆突矩形波导缝隙线阵设计

把常用的矩形波导一个宽面改成圆弧形构成的波导称为圆突矩形波导.这种波导与扇面波导相比:电性能相当;波导管结构更加简单,容易加工,便于安装.文中给出圆突矩形波导中主模场,圆曲面上纵向槽归一化谐振电导近似公式.设计了C和X波段波导曲面纵向谐振缝隙线阵,缝隙电压相位为同相分布,输入端匹配.实际测量了天线输入端电压驻波比和H面方向图,理论与实验相吻合.     

共形波导场近似解及缝隙天线

把矩形波导一个宽面外突成均匀曲面构成的新波导统称为共形波导.利用金属波导边界条件、变分法、边界元素法构造这种新波导中主模场的一种近似解表达式,包括曲面横截线为对称、非对称圆弧,抛物线弧,双曲线弧,椭圆弧等.然后根据等效原理,推导非对称圆弧 矩形波导曲面上窄的纵向半波长缝隙的等效谐振电导的近似计算公式,给出计算曲线.这种解虽然是近似的,但却能解决这类共形波导缝隙天线的工程设计.     

矩形波导中H00模与缝隙参数

本文讨论矩形波导中H_(00)模对波导壁上缝隙耦合与辐射特性等效参数的影响问题。根据几个具体典型实例,通过理论计算的等效参数与已有的实验数据进行对比,认为研究具有纵向缝隙或倾斜缝隙的波导元件和天线的等效参数时,一般情况下应包括H_(00)模的作用。     

扇面波导中TM模

根据波动方程和边界条件，利用分离变量法导出扇面波导中ＴＭ模场分量通用表达式，计算了具有不同的张角和内外单径比的扉面波导中ＴＭ模的截止波数，并列出数表，给出截止波长的精确和近似的表达式。     

波导宽边H—T接头缝隙耦合特性的分析

本文讨论由缝隙耦合的矩形波导宽边H-T分支接头的电气特性。计入了波导壁的实际厚度,在主波导和副波导尺寸是任意的情况下,对任意位置和长度的窄缝电气特性进行了理论推导,导出它的散射场及其等效参数。给出数值计算和实验结果,并作了比较。     

伽略金法分析矩形波导缝隙天线耦合特性

本文用矩量法对波导宽边上的、有厚度的、任意位置的两个纵向缝隙的耦合特性做了分析。文章首先根据Maxwell方程、等效原理、连续性条件建立了两个缝隙上、下口面切向电场为待求函数的四个联立耦合积分方程,然后用伽略金法将积分方程化为矩阵方程。在对矩阵中的内积进行了适于计算机计算的合理的处理后,借助于计算机求出了积分方程的解及一系列特性参数。理论计算和实验结果比较一致,对某些特殊情况的缝隙(如单隙缝、半波长双缝隙)的理论计算也和前人已发表过的计算和实验结果相吻合。文章最后根据计算和实验结果,讨论了缝隙的耦合对缝隙的口径场分布,导纳特性,谐振电导和谐振长度等特性参数的影响。     

波导缝隙阵列RCS

介绍了Ｘ波段波导缝隙谐振阵列天线ＲＣＳ的实验研究实例，初步证明这种谐振式阵列天线的结构与模式散射大致相等，同时验证了得ＲＣＳ的测试结果获得天线增益之方法的实用性。     

波导窄边纵向缝隙耦合特性的研究

本文介绍两矩形波导窄边之间的及H面T形接头的长缝隙的耦合特性。考虑到波导壁厚度的影响,导出求解缝隙的口面场、散射场和等效参数的表达式。给出了计算实例并与实验值进行了比较。所获结果适合于主、副波导尺寸相同和不同的情况,缝隙尺寸、波导壁厚度可以是任意的。     

Learning in an immersive digital theater

The Houston Museum of Natural Science, in collaboration with Rice University has an outreach program taking portable digital theaters to schools and community sites for over five years and has conducted research on student learning in this immersive environment. By using an external independent evaluator, the effectiveness of NASA-funded Education and Public Outreach (EPO) projects can be assessed. This paper documents interactive techniques and learning strategies in full-dome digital theaters. The presentation is divided into Evaluation Strategies and Results and Interactivity Strategies and Results. All learners from grades 3–12 showed statistically significant short-term increase in knowledge of basic Earth science concepts after a single 22-min show. Improvements were more significant on items that were taught using more than one modality of instruction: hearing, seeing, discussion, and immersion. Thus immersive theater can be an effective as well as engaging teaching method for Earth and Space science concepts, particularly those that are intrinsically three-dimensional and thus most effectively taught in an immersive environment. The portable system allows taking the educational experience to rural and tribal sites where the underserved students could not afford the time or expense to travel to museums.     

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

Scaling analysis and model estimation of solar corona index

A monthly average solar green coronal index time series for the period from January 1939 to December 2008 collected from NOAA (The National Oceanic and Atmospheric Administration) has been analysed in this paper in perspective of scaling analysis and modelling. Smoothed and de-noising have been done using suitable mother wavelet as a pre-requisite. The Finite Variance Scaling Method (FVSM), Higuchi method, rescaled range (R/S) and a generalized method have been applied to calculate the scaling exponents and fractal dimensions of the time series. Autocorrelation function (ACF) is used to find autoregressive (AR) process and Partial autocorrelation function (PACF) has been used to get the order of AR model. Finally a best fit model has been proposed using Yule-Walker Method with supporting results of goodness of fit and wavelet spectrum. The results reveal an anti-persistent, Short Range Dependent (SRD), self-similar property with signatures of non-causality, non-stationarity and nonlinearity in the data series. The model shows the best fit to the data under observation.     

Development of a gas chromatography compatible Sample Processing System (SPS) for the in-situ analysis of refractory organic matter in martian soil: preliminary results

In the frame of the 2009 Mars Science Laboratory (MSL) mission a new sample preparation system (SPS) compatible with gas chromatography–mass spectrometry (GC–MS) has been developed for the in situ analysis of complex organic molecules in the Martian soil. The goal is to detect, if they exist, some of the key compounds that play an important role in life on Earth including carboxylic acids, amino acids and nucleobases.     

基于LuGre模型的电液加载系统摩擦补偿

为了提高电液加载系统控制精度,针对摩擦问题提出了基于LuGre摩擦模型的前馈补偿方法.建立了用于摩擦仿真分析和补偿器设计的电液加载系统数学模型;通过实验获取并分析了相关的摩擦数据;基于实验数据进行LuGre模型参数辨识,把LuGre模型和辨识结果引入电液加载系统数学模型,并进行仿真结果与实际摩擦数据的对照,证明了LuGre摩擦模型的准确性.设计前馈补偿器,进行了实验对比,实验结果表明前馈补偿器可将摩擦产生的控制误差有效地降至未补偿时的30%左右.      

CoRoT and Kepler results: Solar-like oscillators

The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars.     

Radioactivity of the Moon and planets

In this report the main results of the study of radioactivity of the solar sistem bodies are considered. The radioactivity of the Moon and planets was measured by means of vehicles in situ. The radioactivity of the lunar samples, brought to the Earth was studied with laboratory equipment.     

Return to Europa: Overview of the Jupiter Europa orbiter mission

Missions to explore Europa have been imagined ever since the Voyager mission first suggested that Europa was geologically very young. Subsequently, the Galileo spacecraft supplied fascinating new insights into this satellite of Jupiter. Now, an international team is proposing a return to the Jupiter system and Europa with the Europa Jupiter System Mission (EJSM). Currently, NASA and ESA are designing two orbiters that would explore the Jovian system and then each would settle into orbit around one of Jupiter’s icy satellites, Europa and Ganymede. In addition, the Japanese Aerospace eXploration Agency (JAXA) is considering a Jupiter magnetospheric orbiter and the Russian Space Agency is investigating a Europa lander.     

基于最小值原理的冗余度机器人动力学控制

为了解冗余度机器人全局法优化中数值求解的困难,本文讨论了动力学方程的建立,无约束和有约束最优控制问题之间的内在联系,重点分析了求解最优控制问题的数值方法,文中提出了双向异步积分迭代的求解正则方程组的直接迭代法,较好解决了状态方程和协态方程稳定相逆给求解两点这值问题带来的困难。     

基于GPS载波相位的微卫星姿态算法研究

GPS姿态系统是利用GPS载波相位测量来确定载体的航向和姿态角。本文对微卫星的GPS姿态系统进行了研究。重点解决短基线的GPS状态算法，讨论了姿态价格函数的了小化方法。测试结果表明，所提的算法对小于1m的基线是有效的。