单涡/贫油驻涡燃烧室的出口温度分布试验

采用试验方法对单涡贫油驻涡燃烧室的出口温度分布的影响因素进行了研究,通过分析试验数据得到如下结论:①凹腔气量对出口温度分布影响较大.随着凹腔气量的增加,出口温度分布系数(OTDF)先增加后减小,与掺混射流的穿透深度有关.②燃油掺混温度对出口温度分布的影响也较大.当燃油掺混温度较小时,出口温度分布系数较低.随着燃油掺混温度增加,出口温度分布系数随之先增加后减小.③燃油供油量对出口温度分布也有重要影响.当燃油量增加时,出口温度分布系数随之先增加后减小.      

基于驻涡燃烧室的贫油熄火经验关系式初探

 驻涡燃烧室（TVC）与传统旋流燃烧室相比采用不同稳焰方式。在前期试验研究的基础上对其贫油熄火(LBO)性能进行归纳总结,参考并与Lefebvre基于化学反应的贫油熄火经验关系式相比较,提出适用于采用煤油为燃料、蒸发管方式供油的驻涡燃烧室的贫油熄火经验关系式。针对驻涡燃烧室提出的贫油熄火经验关系式包含了蒸发管雾化性能、主流气流量和凹腔卷吸气流量等因素,对比经验关系式的预测结果与试验结果,最大误差在15%以内。     

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.     

某重型燃气轮机放气活门及排气管路的改进设计

针对某重型燃气轮机放气系统放气活门在结构设计上存在的问题,经过分析和论证,提出了改进方案,通过计算验证了该方案可以实施。     

空间重粒子击中卤虫卵的定位技术及其生物效应

为了能够估价空间重粒子对单个生物细胞的放射生物学效应,我们设计、制成了卤虫卵-核乳胶夹层式生物包.经搭载我国“8885”卫星飞行数天后回收.用图象分析仪研究了空间重离子在核乳胶上留下的径迹及其分布;并实验观察了卤虫卵的前期发育情况.看到:随星飞行过的卤虫卵与地面对照组相比,其发育能力明显降低,表现为孵化率低且发育时间推迟.实验表明:生物样品板-核乳胶影象定位技术能清楚而比较准确地给出卤虫卵(或其他生物细胞)受重离子作用的信息,是重离子生物效应及其作用机理研究的可行实验手段及分析方法之一.     

Atmospheric Ion-induced Aerosol Nucleation

Ion-induced nucleation has been suggested to be a potentially important mechanism for atmospheric aerosol formation. Ions are formed in the background atmosphere by galactic cosmic rays. A possible connection between galactic cosmic rays and cloudiness has been However, the predictions of current atmospheric nucleation models are highly uncertain because the models are usually based on the liquid drop model that estimates cluster thermodynamics based on bulk properties (e.g., liquid drop density and surface tension). Sulfuric acid (H₂SO₄) and water are assumed to be the most important nucleating agents in the free troposphere. Measurements of the molecular thermodynamics for the growth and evaporation of cluster ions containing H₂SO₄ and H₂O were performed using a temperature-controlled laminar flow reactor coupled to a linear quadrupole mass spectrometer as well as a temperature-controlled ion trap mass spectrometer. The measurements were complemented by quantum chemical calculations of the cluster ion structures. The analysis yielded a complete set of H₂SO₄ and H₂O binding thermodynamics extending from molecular cluster ions to the bulk, based on experimental thermodynamics for the small clusters. The data were incorporated into a kinetic aerosol model to yield quantitative predictions of the rate of ion-induced nucleation for atmospheric conditions. The model predicts that the negative ion-H₂SO₄-H₂O nucleation mechanism is an efficient source of new particles in the middle and upper troposphere.     

凹腔驻涡模型燃烧室内涡的演化发展

使用大涡模拟对凹腔内双驻涡冷态流场进行了分析研究.结果发现, 在主流、前后壁面射流的情况下, 凹腔在某些特定几何条件下会产生准周期生成和破碎的驻涡, 同时研究了凹腔内准周期驻涡的生成发展的过程, 得到了影响凹腔内涡演化的新结果.      

旋转冲压发动机驻涡燃烧技术研究现状分析

旋转冲压发动机是一种全新概念发动机,采用激波增压和驻涡燃烧技术。其显著的高效、低污染特性引起越来越多人关注。本文首先扼要介绍了旋转冲压发动机总体结构,然后介绍了驻涡燃烧技术的概念和研究现状,最后描述了旋转冲压发动机中驻涡燃烧室的结构特点。     

蒸汽引射稠油输送新技术

管线输送是稠油输运的一种主要手段。由于我国一些油田原油粘度高,常温下流动性差,管输需采用特殊工艺。根据粘度随温度沿指数下降的规律,与其它工艺比较,加热输送工艺有更大的潜力。该文提出了一种蒸汽引射直接加热稠油输送的新技术。为研究其有效性,进行了性能分析,并在辽河油田Ф80mm,300m输油管线上进行了现场实验,测量了三种工况下该方法对稠油的温度、压降和含水率的影响。实验结果表明该文提出的方法是可行的。     

Ion thruster accelerator grid erosion mechanism under extreme conditions of cylindrical erosion and chamfer erosion

In this paper, the abnormal experimental phenomenon on barrel erosion under extreme working conditions in the ultra-long life experiment(>10000 h) of ion thruster ion optics is studied by the Immersed-Finite-Element Particle-In-Cell Monte-Carlo-Collision(IFE-PIC-MCC) method and the grid erosion evaluation model. The transport process of beam ions and Charge Exchange(CEX) ions in the grid system, and the characteristics and mechanisms of the aperture barrel erosion under extreme erosion condit...