Venus Interior Structure and Dynamics

No two rocky bodies offer a better laboratory for exploring the conditions controlling interior dynamics than Venus and Earth. Their similarities in size, density, distance from the sun, and young surfaces would suggest comparable interior dynamics. Although the two planets exhibit some of the same processes, Venus lacks Earth’s dominant process for losing heat and cycling volatiles between the interior and the surface and atmosphere: plate tectonics. One commonality is the size and number of mantle plume features which are inferred to be active today and arise at the core mantle boundary. Such mantle plumes require heat loss from the core, yet Venus lacks a measurable interior dynamo. There is evidence for plume-induced subduction on Venus, but no apparent mosaic of moving plates. Absent plate tectonics, one essential question for interior dynamics is how did Venus obtain its young resurfacing age? Via catastrophic or equilibrium processes? Related questions are how does it lose heat via past periods of plate tectonics, has it always had a stagnant lid, or might it have an entirely different mode of heat loss? Although there has been no mission dedicated to surface and interior processes since the Magellan mission in 1990, near infrared surface emissivity data that provides information on the iron content of the surface mineralogy was obtained fortuitously from Venus Express. These data imply both the presence of continental-like crust, and thus formation in the presence of water, and recent volcanism at mantle hotspots. In addition, the study of interior dynamics for both Earth and exoplanets has led to new insights on the conditions required to initiate subduction and develop plate tectonics, including the possible role of high temperature lithosphere, and a renewed drive to reveal why Venus and Earth differ. Here we review current data that constrains the interior dynamics of Venus, new insights into its interior dynamics, and the data needed to resolve key questions.     

面向高超声速飞行器双重不确定性的自适应状态估计

将高超声速飞行器双重不确定性因素建模为未知干扰输入项，针对状态演化方程和量测方程含有不同未知干扰输入的高超声速飞行器控制系统状态估计问题开展研究，提出一种基于自适应方差极小化的递推状态估计器(Adaptive variance minimization based Recursive Estimator, AVMRE)。首先建立了状态估计递推滤波器模型，实现滤波误差中的量测未知干扰解耦，之后引入自适应调整因子刻画状态未知干扰并推导了最小上界估计误差协方差矩阵，最后，基于最小方差估计准则设计了滤波器中的量测增益反馈矩阵。以外部突风和传感器故障为例，受内外部双重不确定性因素影响下的高超声速飞行器仿真实验验证了本文算法的有效性，与相关算法的仿真对比反映了本文算法的优越性。     

Superluminous Supernovae

Superluminous supernovae are a new class of supernovae that were recognized about a decade ago. Both observational and theoretical progress has been significant in the last decade. In this review, we first briefly summarize the observational properties of superluminous supernovae. We then introduce the three major suggested luminosity sources to explain the huge luminosities of superluminous supernovae, i.e., the nuclear decay of ⁵⁶Ni, the interaction between supernova ejecta and dense circumstellar media, and the spin down of magnetars. We compare these models and discuss their strengths and weaknesses.     

基于编辑距离相似度的文本校验技术研究与应用

树形结构的文本配置在分布式的测控数据处理软件中使用广泛,它的正确性对数据处理而言至关重要。为了实现树形结构的文本配置自动检查和纠错,通过引入LD(Levenshtein Distance)编辑距离算法,把字符串的编辑操作推广到多叉树之间。在此基础上定义了多叉树之间的编辑距离,建立了衡量多叉树之间相似度的方法,设计了基于模糊匹配的文本配置自动校对流程,解决了精确匹配时由字符的多义性导致的查全率失真和误判的问题。根据实验结果,查全率和查准率分别达到了87.5%和100%,有效提高了基于树形结构的文本配置自动校验时的可靠性。     

高动态下惯性加速度辅助三阶锁相环性能分析

针对高阶跟踪环路稳定性比低阶环路差,大带宽带来测量误差大的问题。研究在高动态环境下,惯导加速度信息辅助卫星接收机三阶载波锁相环跟踪算法,以及不同环路参数下跟踪环路的性能。对载体高动态场景、加速度信息延迟进行建模,并对算法进行了数学仿真。仿真分析结果表明,在加速度信息辅助下,即使压缩载波跟踪环路等效噪声带宽到3Hz,在高达1200g/s的加速度动态下,环路跟踪同样稳定可靠。     

Combustion efficiency test method in scramjet engine

A scramjet engine combustion efficiency measure system was designed.The combustion efficiency was measured by chromatography method,and the results of chromatography method were compared with those of temperature method.The results indicate that the combustion efficiency measured by chromatography method was 80.7%,lower than the combustion efficiency of 84.5%measured by temperature method;the combustion efficiency could be measured more precisely by chromatogram method than by temperature method.The combustion efficiency measure system based on chromatogram method can work well,and thus can be used to measure the combustion efficiency of scramjet engine.     

旋转爆轰发动机工作过程的数值模拟

为了深入研究旋转爆轰发动机工作过程,采用高精度高分辨率迎风通量分裂格式(AUSMPW+)、氢氧7组分8反应化学动力学模型,求解三维带化学反应的Euler方程。对旋转爆轰发动机工作过程进行了数值模拟,分析了采用预爆轰管点火过程的流场特征以及整个发动机推力、推力偏心距、侧向力随时间的变化规律。计算结果表明:切向预爆轰管紧贴喷注入口时,点火过程仅产生一道单向爆轰波,能成功点燃旋转爆轰发动机;在本文给定的计算条件下,旋转爆轰发动机平均推力约180N,旋转爆轰波传播频率约为14285Hz;旋转发动机正常工作过程中,推力偏心矩、侧向力随时间周期性变化。     

Nonlinear relative position control of precise formation flying using polynomial eigenstructure assignment

A nonlinear relative position control algorithm is designed for spacecraft precise formation flying. Taking into account the effect of J₂ gravitational perturbations and atmospheric drag, the relative motion dynamic equation of the formation flying is developed in a quasi-linear parameter-varying (QLPV) form without approximation. Base on this QLPV model, polynomial eigenstructure assignment (PEA) is applied to design the controller. The resulting PEA controller is a function of system state and parameters, and produces a closed-loop system with invariant performance over a wide range of conditions. Numerical simulation results show that the performance can fulfill precise formation flying requirements.     

基于输出反馈的编队卫星姿态同步和跟踪控制

研究了卫星编队无角速度测量信息且采用局部信息交互时的姿态协同控制问题.以四元数为姿态描述手段,采用超前滤波方法重构星体绝对和相对角速度信息,设计了基于输出反馈的分散姿态同步和跟踪控制器.利用Barbalat引理和代数图论等对闭环系统的全局渐近稳定性进行了理论分析和证明.以六星编队为背景的数值仿真进一步验证了算法的有效性.     

一种光学遥感成像系统优化设计新方法研究

针对空间光学高分辨率遥感器,既要实现轻小型化,又要获得高品质遥感图像的要求,文章提出一种空间光学遥感成像系统优化设计新方法;综合考虑成像链路各环节因素,采用全面的指标设计和合理的优化设计流程来改进空间光学遥感成像系统的总体指标和成像品质,并显著降低遥感器的研制难度.通过比较全链路优化设计方法和传统设计方法的仿真结果及其...