The Orbital Forcing of Climate Changes on Mars

Solar variability influences the climate of a planet by radiatively forcing changes over a certain timescale; orbital variations of a planet, which yield similar solar forcing modulations, can be studied within the same scientific context. It is known for Earth that obliquity changes have played a critical role in pacing glacial and interglacial eras. For Mars, such orbital changes have been far greater and have generated extreme variations in insolation. Signatures associated with the presence of water ice reservoirs at various positions across the surface of Mars during periods of different orbital configurations have been identified. For this reason, it has been proposed that Mars is currently evolving between ice ages. The advent of climate tools has given a theoretical frame to the study of orbitally-induced climate changes on Mars. These models have provided an explanation to many puzzling observations, which when put together have permitted reconstruction of almost the entire history of Mars in the last 10 million years. This paper proposes to give an overview of the scientific work dedicated to this topic.     

A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.     

J—8ACT验证机平尾助力系统抖振分析

本文对J-8ACT验证机纵向数字电传操纵系统所使用的平尾助力系统的抖振原因和抑制措施进行了线性和非线性分析。证明了引起助力系统抖振的主要原因,除由流量特性决定的过大的流量系数外,对于内反馈式的助力系统来说,不可避免的安装支承间隙是一个重要因素。机械输入式液压伺服裝置的一些重要特性是由滑阀摩擦引起的。这种受机械反馈影响的特殊摩擦力,具有增加液压作动器的增益和滞后作用。由于这个特点,它能抑制/消除助力系统抖振。     

产品全生命周期快速研制技术

总结了产品生命周期各个阶段的快速研制技术,提出了产品全生命周期快速研制多维体系结构和“靶心”实现模型。     

颤振板的极限环振动

本文研究了在匀速气流中悬臂板的极限环振动。采用冯·卡门大挠度板理论和准定常空气动力,应用瑞雷-里兹法导出悬臂颤振板的非线性振动的计算方程。并提出一组模态函数展开式用于拉格朗日方程,从而确定随时间历程的极限环振动和颤振边界。计算表明,模态展开式具有收敛性,板的长宽比对极限环振幅有显著影响。     

直接反转完全可逆式组合叶栅的实验研究

针对矿井、隧道等行业对风机反风性能的要求,提出了一种动叶直接反转完全可逆式组合叶栅设计的新方案。该方案具有结构简单、正反向性能完全相同、便于采用现有成熟叶型等特点。通过平面叶栅试验确定了重叠度、栅距比等组合叶栅最佳组合参数,此外,试验结果表明在相同雷诺数下,组合叶栅的正反向最大升力系数C_(L max)和失速攻角α_(L max)较现有双对称叶型均有大幅度提高,显示出较好的应用前景。     

Mission-oriented cooperative 3D path planning for modular solar-powered aircraft with energy optimization

Modular Solar-Powered Aircraft(M-SPA) is a kind of High-Altitude Long-Endurance(HALE) aircraft which exploits the mission advantage of swarm UAV and the HALE advantage of large aspect-ratio SPA. M-SPA’s separated mode and combined mode give it the potential to maximize the mission efficiency with limited solar energy. In this paper, firstly, oriented by the mission of maximizing the cruise area, the overall design of the M-SPA is modeled, including the energy model, the aerodynamic model and the...     

进口导叶形式对核心机驱动风扇级的影响

以某变循环发动机(VCE)所用核心机驱动风扇级(CDFS)为研究模型,数值模拟了CDFS在真实边界环境下的流动特性,分析了单/双涵道工作模式下,不同形式的可调进口导叶(IGV)对CDFS流动特性及性能的影响机理。结果表明:不同工作模式时,CDFS靠导叶角度的开闭实现大范围的流量调节。单涵道(SB)工作模式时,不同形式的可调进口导叶(VIGV)对CDFS性能的影响差异很小;双涵道(DB)工作模式时采用常规可调导叶(CIGV)会在其吸力面产生较大的流场分离,且流通能力和流量调节范围大大降低。可变弯度导叶通过可转动部分的开闭实现CDFS对流量调节的需求;通过固定部分保证CDFS导叶进口气流攻角基本不变,同时在固定部分和可转动部分连接处所形成的收缩通道的加速效应显著抑制了导叶吸力面的流动分离。可变弯度导叶是适用于CDFS在不同工作模式下性能参数及流量调节需求的可调导叶的形式。     

串联式TBCC发动机风车冲压模态性能模拟

建立了基于部件低转速特性匹配的串联式涡轮基组合循环（TBCC）发动机风车冲压模态性能计算模型,提出了压气机低转速大流量特性扩展方法,由换算扭矩代替等熵效率表示旋转部件特性,解决了低转速部件效率不连续相关问题。分析了冲压外涵面积变化和涡轮功率提取对风车冲压模态性能及部件匹配的影响规律,并基于推力、流量连续准则设计了涡轮模态至冲压模态转换过程（含风车冲压模态）的参数调节规律。计算结果表明:在风车冲压模态下,冲压外涵面积变化对风扇工作状态有显著影响,对压气机影响较小;涡轮可提取功率随着风车转速的减小先增加后降低,比冲随提取功率的增加基本呈线性降低趋势,功率提取位置（高、低压涡轮）对部件匹配有显著影响。      

一种阵列天线逐通道相关在线标校法

由于发送端和接收端时钟的不一致性,导致低信噪比下阵列天线卫星移动通信的逐通道相关标校有很大的难度。在考虑易实现性和简易性基础上,提出了一种可以解决低信噪比下通道校正的多周期长时累积方法。该校准信号为由地面标校站产生的BPSK调制扩频信号,可以减少卫星设计的复杂度,且在不中断用户数据传输的基础上实现在线标校。该方法通过对接收信号打标、速率匹配等措施来解决收发时钟不一致导致的码偏和频偏问题。研究结果可以为阵列天线卫星通信技术提供支持。