高速列车进入带缓冲结构隧道的压力变化研究(Ⅰ)

给出了列车穿越带有缓冲结构的隧道压力变化的三维粘性流场数值模拟过程,控制方程为三维粘性、可压缩、非定常流的N-S方程,空间离散采用了中心有限体积法格式,时间采用预处理二阶精度多步后差分格式进行离散,对列车与隧道之间的相对运动采用移动网格技术处理。对不同的缓冲结构缓解隧道内瞬变压力及压力梯度的作用进行了研究。研究结果表明,缓冲结构的设置能够有效地降低隧道内的压力和压力梯度的最大值,其原因在于缓冲结构延长了压缩波压力上升的时间,降低列车突入隧道时所形成的最大压力梯度;另一方面由于压缩波在缓冲结构和列车、隧道之间多次的反射,也降低了压力峰值。     

高速磁浮列车会车压力波数值计算研究

根据可压缩粘性流体的N-S方程和k-ε双方程湍流模型,运用移动网格技术,采用有限容积法对磁浮列车以500 km/h速度运行时的会车压力波进行了数值计算研究,计算结果与现车试验结果相差10%以内,表明了本文计算模型和方法的正确性;文中还研究了交会过程中列车周围的流场分布,结果表明:当列车交会时,两车之间的流场相互叠加,而两车之外的流场分布在整个交会过程中变化不大。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

高速列车进入带缓冲结构隧道的压力变化研究（I）

给出了列车穿越带有缓冲结构的隧道压力变化的三维粘性流场数值模拟过程，控制方程为三维粘性、可压缩、非定常流的N．S方程，空间离散采用了中心有限体积法格式，时间采用预处理二阶精度多步后差分格式进行离散，对列车与隧道之间的相对运动采用移动网格技术处理。对不同的缓冲结构缓解隧道内瞬变压力及压力梯度的作用进行了研究。研究结果表明，缓冲结构的设置能够有效地降低隧道内的压力和压力梯度的最大值，其原因在于缓冲结构延长了压缩波压力上升的时间，降低列车突入隧道时所形成的最大压力梯度；另一方面由于压缩波在缓冲结构和列车、隧道之间多次的反射，也降低了压力峰值。     

超燃冲压发动机隔离段流场数值模拟

隔离段是双模态超燃冲压发动机实现双模态和模态转换的一个重要部件,同时,它把进气道和燃烧室隔离开,以防止燃烧室工作对进气道干扰,引起进气道不启动。由于隔离段内气体流动的复杂性及其广泛的工程应用前景,隔离段内的流动特性引起了人们的广泛关注。本文使用隐式TVD格式,采用雷诺应力湍流模型,近壁面采用非平衡壁面函数方法处理,控制方程的离散采用二阶迎风格式,对隔离段内的流场进行了数值模拟,并分析了出口反压、来流马赫数对隔离段内流场的影响。     

高速铁路隧道初始压缩波一维流动模型的数值分析方法

基于隧道内空气流通截面是时间和距离的二元函数条件与一维流动理论,提出了高速列车驶入设有缓冲结构隧道端口时产生初始压缩波的数值分析方法。一维流动理论采用考虑摩擦、传热以及空气质交换等因素的一维可压缩非定常不等熵流动模型。数值分析方法采用广义黎曼变量特征线法。与国外有关未设缓冲结构、开孔型与未开孔型缓冲结构的隧道端口三种情况的现车试验结果进行了比较,表明本文所建方法正确、合理,能够模拟计算多种类型缓冲结构条件下的压缩波波动规律。     

利用均匀抽吸地板进行高速列车模型地板边界层影响的试验研究

在KD－03低速风洞中研制了一种边界层可人为控制的均匀抽吸地板。研究了在各种来流速度下均匀抽吸地板上边界层与抽吸系数的关系。在该地板上对高速列车模型气动力与地板边界层的关系进行了实验研究。对实验的几种模型状态，边界层吸除使列车模型所受阻力、负向升力和低头力矩均有明显增加，其增量与模型底部形状有关；在有侧滑角时，边界层吸除对模型气动力的六个分量均有影响。在没有边界层控制的固定地板上进行高速列车模型风洞实验，会使实验结果固边界层的影响而产生较大偏差。利用均匀抽吸地板可有效地消除边界层的影响，从而较准确地模拟地面效应的影响，提高高速列车模型风洞实验气动载荷的实验精度。而且，它的实验结果可为没有地板边界层控制装置的风洞中同类模型实验的边界层修正提供参考依据。     

Numerical investigation on flow nonuniformity-induced hysteresis in scramjet isolator

Numerical simulation and theoretical analysis were conducted to study the hysteresis inside scramjet isolator during the reciprocating process of back pressure variation. It is revealed that only a regular reflection is theoretically possible for two leading shocks when the inflow Mach number is greater than 2.0, and no hysteresis can occur in the transition between shock reflection types. Nevertheless, wall suction, gas injection, and background waves cause non-uniformity of the incoming flow and would make hysteresis possible. Besides the classical hysteresis in the transition between shock reflection, new kinds of hysteresis were found in both the deflection angle of separated boundary layer and the location of the shock train. Moreover, the occurrence of hysteresis in the deflection angle of the separated boundary layer is accompanied with the shock reflection hysteresis. In the case with background waves or gas injection, hysteresis in the starting position of leading shock was observed too. As back pressure decreases, the leading shock does not follow the same path as that as the back pressure increases, and it is anchored at the location where the background shock or the injection interacts with the leading shock. It is inferred that, if two strong adverse pressure gradient regions move towards and interact with each other, hysteresis will take place when they start to separate.     

Nonlinear dynamic modeling of a helicopter planetary gear train for carrier plate crack fault diagnosis

Planetary gear train plays a significant role in a helicopter operation and its health is of great importance for the flight safety of the helicopter. This paper investigates the effects of a planet carrier plate crack on the dynamic characteristics of a planetary gear train, and thus finds an effec-tive method to diagnose crack fault. A dynamic model is developed to analyze the torsional vibra-tion of a planetary gear train with a cracked planet carrier plate. The model takes into consideration nonlinear factors such as the time-varying meshing stiffness, gear backlash and viscous damping. Investigation of the deformation of the cracked carrier plate under static stress is performed in order to simulate the dynamic effects of the planet carrier crack on the angular displacement of car-rier posts. Validation shows good accuracy of the developed dynamic model in predicting dynamic characteristics of a planetary gear train. Fault features extracted from predictions of the model reveal the correspondence between vibration characteristic and the conditions (length and position) of a planet carrier crack clearly.     

烧蚀后的C-SiC隔离段内流场精细测量试验

为了获得极度粗糙内壁面对激波串流动特性的影响规律,通过基于纳米粒子示踪的平面激光散射技术和高频动态压力测量技术测量了Ma2来流下烧蚀后的C-SiC隔离段中激波串流场结构,获得了激波串初始激波形态、激波后附面层发展形态以及激波串动态特性。结果表明,烧蚀后的C-SiC隔离段中激波串结构与光滑不锈钢隔离段相似。但是极度粗糙的内壁面深刻影响了近壁区流动,附面层增厚效应非常明显。前者激波串内的附面层比后者厚约50%,前者激波分叉点比后者更接近唇口约30%。极度粗糙的内壁面也提高了附面层的分形维数,加剧了拟序结构的破碎程度。烧蚀后的C-SiC隔离段中附面层的分形维数在1.548～1.649,比光滑不锈钢隔离段高6.7%～8.9%。烧蚀后的C-SiC隔离段极度粗糙内壁面对激波串振荡频率几乎没有影响。激波串前传过程中的振荡频率约20Hz。