昆虫翅悬停飞行中的三维空间旋涡结构

昆虫(果蝇)悬停飞行中,翅膀按照特定的拍动方式往复运动,产生非定常高升力维持身体的平衡.研究昆虫高升力机理,需要探索拍动翼运动引发的三维空间非定常流场的特性,尤其是三维空间非定常涡的发展变化过程.本文将氢气泡流动显示技术应用于动态模型实验,定性的观察拍动翼前缘涡(LEV)的发展破裂过程.并利用数字体视粒子图像测速,DSPIV(Digital Steroscopic Particle Image Velocimetry)技术,测得了拍动翼运动瞬时相位和相位平均的三维空间流场信息(速度向量场、截面涡量场、空间涡量场,以及三维空间流线),揭示了拍动翼展向流动的存在,并结合定性和定量方法多角度说明了前缘涡沿展向发展到破裂的流动结构,并说明了侧缘涡与前缘涡的相互影响.测量结果表明:在雷诺数960的情况下,拍动翼运动至相位时,翼面上前缘涡在距翼根约60%展长的位置发生破裂;翼根至破裂点之间,展向流动稳定,指向翼梢;破裂点以后,展向流改变方向,指向翼根.     

航空二冲程汽油发动机均值模型的研究与仿真

发动机平均值模型由于其模型简单、计算时间短、使用方便,且能满足控制设计的要求被广泛应用。目前均值模型主要在四冲程汽油机和大型二冲程柴油机上广泛应用,小型航空二冲程汽油发动机平均值模型国内外应用很少。本文采用机理建模和试验建模相结合的方法建立了发动机均值模型,为研究二冲程汽油发动机提供了一种思路。二冲程汽油机平均值模型主要分为三个动态子模块：燃油蒸发与油膜动态子模块、进气道与曲轴箱扫气子模块和动力输出子模块,建模中考虑了簧片阀的建模,同时考虑了扫气过程中的短路损失。分别建立了动力输出和转速模型、空燃比模型,并进行了Matlab/simulink仿真,仿真结果和实验数据吻合,证明了该均值模型的正确性。     

The Electric Antennas for the STEREO/WAVES Experiment

The STEREO/WAVES experiment is designed to measure the electric component of radio emission from interplanetary radio bursts and in situ plasma waves and fluctuations in the solar wind. Interplanetary radio bursts are generated from electron beams at interplanetary shocks and solar flares and are observed from near the Sun to 1 AU, corresponding to frequencies of approximately 16 MHz to 10 kHz. In situ plasma waves occur in a range of wavelengths larger than the Debye length in the solar wind plasma λ _D ≈10 m and appear Doppler-shifted into the frequency regime down to a fraction of a Hertz. These phenomena are measured by STEREO/WAVES with a set of three orthogonal electric monopole antennas. This paper describes the electrical and mechanical design of the antenna system and discusses efforts to model the antenna pattern and response and methods for in-flight calibration.     

The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories

The Plasma and Suprathermal Ion Composition (PLASTIC) investigation provides the in situ solar wind and low energy heliospheric ion measurements for the NASA Solar Terrestrial Relations Observatory Mission, which consists of two spacecraft (STEREO-A, STEREO-B). PLASTIC-A and PLASTIC-B are identical. Each PLASTIC is a time-of-flight/energy mass spectrometer designed to determine the elemental composition, ionic charge states, and bulk flow parameters of major solar wind ions in the mass range from hydrogen to iron. PLASTIC has nearly complete angular coverage in the ecliptic plane and an energy range from ～0.3 to 80 keV/e, from which the distribution functions of suprathermal ions, including those ions created in pick-up and local shock acceleration processes, are also provided.     

The THEMIS Array of Ground-based Observatories for the Study of Auroral Substorms

The NASA Time History of Events and Macroscale Interactions during Substorms (THEMIS) project is intended to investigate magnetospheric substorm phenomena, which are the manifestations of a basic instability of the magnetosphere and a dominant mechanism of plasma transport and explosive energy release. The major controversy in substorm science is the uncertainty as to whether the instability is initiated near the Earth, or in the more distant >20 Re magnetic tail. THEMIS will discriminate between the two possibilities by using five in-situ satellites and ground-based all-sky imagers and magnetometers, and inferring the propagation direction by timing the observation of the substorm initiation at multiple locations in the magnetosphere. An array of stations, consisting of 20 all-sky imagers (ASIs) and 30-plus magnetometers, has been developed and deployed in the North American continent, from Alaska to Labrador, for the broad coverage of the nightside magnetosphere. Each ground-based observatory (GBO) contains a white light imager that takes auroral images at a 3-second repetition rate (“cadence”) and a magnetometer that records the 3 axis variation of the magnetic field at 2 Hz frequency. The stations return compressed images, “thumbnails,” to two central databases: one located at UC Berkeley and the other at the University of Calgary, Canada. The full images are recorded at each station on hard drives, and these devices are physically returned to the two data centers for data copying. All data are made available for public use by scientists in “browse products,” accessible by using internet browsers or in the form of downloadable CDF data files (the “browse products” are described in detail in a later section). Twenty all-sky imager stations are installed and running at the time of this publication. An example of a substorm was observed on the 23rd of December 2006, and from the THEMIS GBO data, we found that the substorm onset brightening of the equatorward arc was a gradual process (>27 seconds), with minimal morphology changes until the arc breaks up. The breakup was timed to the nearest frame (<3 s) and located to the nearest latitude degree at about ±3^oE in longitude. The data also showed that a similar breakup occurred in Alaska ～10 minutes later, highlighting the need for an array to distinguish prime onset.     

New Horizons: Anticipated Scientific Investigations at the Pluto System

The New Horizons spacecraft will achieve a wide range of measurement objectives at the Pluto system, including color and panchromatic maps, 1.25–2.50 micron spectral images for studying surface compositions, and measurements of Pluto’s atmosphere (temperatures, composition, hazes, and the escape rate). Additional measurement objectives include topography, surface temperatures, and the solar wind interaction. The fulfillment of these measurement objectives will broaden our understanding of the Pluto system, such as the origin of the Pluto system, the processes operating on the surface, the volatile transport cycle, and the energetics and chemistry of the atmosphere. The mission, payload, and strawman observing sequences have been designed to achieve the NASA-specified measurement objectives and maximize the science return. The planned observations at the Pluto system will extend our knowledge of other objects formed by giant impact (such as the Earth–moon), other objects formed in the outer solar system (such as comets and other icy dwarf planets), other bodies with surfaces in vapor-pressure equilibrium (such as Triton and Mars), and other bodies with N₂:CH₄ atmospheres (such as Titan, Triton, and the early Earth).     

德国机床工业的创新和趋势

机床是一个复杂的机电一体化系统.机床的创新离不开新结构、新材料、新的功能部件、新刀具和新的外围设备.加工工艺的发展以及加工过程的仿真和监控也日益受到重视.     

最新高性能中速走丝电火花数控线切割机床

<正>秉承苏州三光精心制造的传统,苏州三光科技股份有限公司的产品始终将产品性能、可靠性放在首位。随着高品质产品所带来的市场高认可度,苏州三光的产品走进了越来越多的工厂和车间。同时,市场对高性     

基于需用速度增益曲面的大气层外超远程拦截导引方法

考虑拦截器使用耗尽关机固体推进系统的情况,提出需用速度增益曲面概念,设计了基于该概念的大气层外超远程拦截导引方法。根据Lambert导引,给定拦截时间就有唯一的指令推力方向与之对应,导引过程分为两个阶段:零控拦截到达阶段,选择最优拦截时间,需用速度增益曲面迅速与助推时间-拦截时间平面相切;零控拦截保持阶段,拦截时间不断减小,保持需用速度增益曲面在助推时间-拦截时间平面上滑动,消耗多余的推进剂。利用拟零控拦截概念使两个导引阶段平缓过渡,避免了导引方法切换时推力方向的跳变。导引律计及了J2项摄动对滑行段弹道的影响,导引精度对推进系统参数偏差的鲁棒性强。仿真结果表明本文制导方法用于大气层外超远程目标拦截,脱靶量仅为km量级,推进系统参数偏差对导引精度的影响很小。     

多段翼混合边界层改变对流场的影响研究

前缘缝翼尾流与主翼边界层混合的改变对主翼气动力具有重要影响.利用数值模拟手段,通过在前缘缝翼尾缘添加一定动量系数的喷流,改变前缘缝翼尾缘的尾流,进而改变尾流与主翼边界层的混合状况.求解二维多段翼模型30P30N在各个不同喷流条件下的二维非定常流场,结果表明:提高前缘缝翼尾缘喷流的动量系数,将使前缘缝翼尾流和主翼边界层混合开始点后移,提高主翼上表面负压峰值和主翼升力;混合开始点对主翼的负压峰值及升力均有一定的影响;增大来流攻角会抑制前缘缝翼尾流和主翼边界层的混合.