甲烷-空气贫燃料预混燃烧的数值模拟

针对燃气轮机燃烧室火焰筒中的甲烷-空气贫燃料预混燃烧问题,给出了基于八步化学反应动力学机理的数学模型。以某型航空发动机燃烧室火焰筒为例,对甲烷-空气贫燃料的预混燃烧进行数值模拟。研究结果表明,基于八步化学反应动力学机理的数值模拟方法,可以比较准确地反映燃烧产物的形成过程,在分析航空发动机燃烧室火焰筒内的贫燃料预混燃烧问题时具有较强的实用性。     

ICR循环燃气轮机的仿真研究

采用MATLAB和VC混合编程的方法,建立了不同循环燃气轮机的热力性能仿真模型,并利用该模型对比研究了压比、燃气初温、间冷度、回热度等参数对ICR(间冷-回热)循环比功和效率的影响.研究表明:在给定条件下,合理匹配压比、燃气初温、间冷度和回热度等参数,可使ICR循环的比功和效率均达到最大;与单循环相比,ICR循环的比功...     

周向总压畸变条件下多级轴流压气机失速首发级预测分析

基于多级轴流压气机的逐级特性,发展了1种预测周向总压畸变条件下多级轴流压气机失速首发级的方法。该方法结合平行压气机模型和级叠加计算方法,以进气畸变条件下多级轴流压气机某级的有效相对气流角达到稳定状态时该级的最大相对气流角为条件,进行多级轴流压气机失速首发级的预测分析。通过对J85—13发动机8级轴流压气机总压畸变试验数据进行模拟计算,预测出该轴流压气机畸变条件下的失速首发级。     

进气条件对压气机中介机匣流场影响的试验研究

以某压气机中介机匣为试验研究对象,通过改变来流径向分布与马赫数,建立了评估中介机匣气动性能的进口约束条件。在同步测量轴向流路离散压力参数的基础上,分析了中介机匣内部流场对进气条件的稳态响应。研究结果表明:进气条件对中介机匣流动损失影响较大,与均匀进气相比,进气畸变会增大弯曲流道内部径向压力梯度,影响流道曲率与流向压力梯度对附面层的控制效果;支板尾流对通道主流的干扰导致下游平直流道上部区域流场恶化,而进气畸变会加剧支板尾迹的影响;随着进口马赫数的增大,中介机匣总压损失系数与总压畸变强度呈现出不同的增长趋势,其出口流场径向分布对马赫数变化的气动敏感性较高。     

CubeSail: A low cost CubeSat based solar sail demonstration mission

CubeSail is a nano-solar sail mission based on the 3U CubeSat standard, which is currently being designed and built at the Surrey Space Centre, University of Surrey. CubeSail will have a total mass of around 3 kg and will deploy a 5 × 5 m sail in low Earth orbit. The primary aim of the mission is to demonstrate the concept of solar sailing and end-of-life de-orbiting using the sail membrane as a drag-sail. The spacecraft will have a compact 3-axis stabilised attitude control system, which uses three magnetic torquers aligned with the spacecraft principle axis as well as a novel two-dimensional translation stage separating the spacecraft bus from the sail. CubeSail’s deployment mechanism consists of four novel booms and four-quadrant sail membranes. The proposed booms are made from tape-spring blades and will deploy the sail membrane from a 2U CubeSat standard structure. This paper presents a systems level overview of the CubeSat mission, focusing on the mission orbit and de-orbiting, in addition to the deployment, attitude control and the satellite bus.     

水反应金属燃料在水蒸气环境下的稳态燃烧特性

为探索高金属含量水冲压发动机的稳态燃烧机理,开展了镁基高金属含量水反应金属燃料在水蒸气氛围下的稳态燃烧试验研究,燃料中金属镁含量高于70%.采用直径0.5 mm的K型热电偶测量燃料燃烧波曲线,并拍摄了火焰图片.结果显示,工作压强2.0 MPa时,燃料稳态燃烧的燃面温度约为900.1℃,气相平衡火焰温度约为1 214.9...     

固液火箭冲压发动机燃烧室流场数值仿真

固液火箭冲压发动机通过固液两种燃料匹配工作,相比传统的固体火箭冲压发动机和液体燃料冲压发动机具有较为明显的优势.基于离散相模型和单步反应模型,采用Fluent 对设计点飞行参数下,不同结构和不同工况条件下的燃烧室两相反应流场进行了数值仿真.结果表明,燃气发生器喷管参数和进气道进气角度主要影响空气与燃气流的撞击以及头部区...     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).     

大型双曲冷却塔表面脉动风压随机特性——风压极值探讨

针对风压信号呈现的非高斯特性和传统极限估计方法的局限,首次提出基于保证率和相关性的极值估计方法——全概率迭代法进行冷却塔表面脉动风荷载极值分析,并和传统的峰值因子法及改进的Sadek-Simiu法计算结果进行对比验证。结果表明：全概率迭代法避开了对随机过程的高斯分布假定,相比传统的极值估计方法其结果更加真实可靠;表达风压极值中脉动分量的峰值因子数值沿着环向和子午向变化显著,如取为同一数值则偏于危险或过于保守;采用全概率迭代法得到的表面风压系数极值分布曲线与规范取值相比,迎风面和负压峰值区域极值偏小,背风区域极值偏大,且最小值对应角度相差约10°。     

DORIS processing at the European Space Operations Centre

This paper gives an overview of the DORIS related activities at the Navigation Support Office of the European Space Operations Centre. The DORIS activities were started in 2002 because of the launch of the Envisat satellite where ESOC is responsible for the validation of the Envisat Precise Orbits and a brief overview of the key Envisat activities at ESOC is given. Typical orbit comparison RMS values between the CNES POE (GDR-C) and the ESOC POD solution is 6.5, 18.8 and 23.1 mm in radial-, along- and cross-track direction. In the framework of the generation of the ITRF2008 ESOC participated in the reprocessing of all three space geodetic techniques; DORIS, SLR, and GPS. Here the main results of our DORIS reprocessing, in the framework of the International DORIS Service (IDS), are given. The WRMS of the weekly ESOC solution (esawd03) for the 2004–2009 period compared to the IDS-1 combined solution is of the order of 12 mm. Based on the long time series of homogeneously processed data a closer look is taken at the estimated solar radiation pressure parameters of the different satellites used in this DORIS analysis. The main aim being the stabilization of the Z-component of the geocentre estimates. We conclude that the ESOC participation to the IDS ITRF2008 contribution has been beneficial for both ESOC and the IDS. ESOC has profited significantly from the very open and direct communications and comparisons that took place within the IDS during the reprocessing campaign.