基于OH-PLIF技术的环形燃烧室预混火焰结构实验

针对微型燃气轮机环形燃烧室中的燃烧特性,利用平面激光诱导荧光(PLIF)技术,对环形燃烧室内甲烷/空气预混湍流多束火焰燃烧开展实验研究,得到OH自由基物质的量浓度分布,并研究雷诺数和当量比对火焰结构特征参数的影响。结果表明:OH自由基浓度分布呈现环形结构,并有火焰托举和分叉现象,OH-PLIF瞬时和平均图像揭示了火焰具有湍流和层流预混结构共同特征。火焰结构特征参数的定量分析表明,雷诺数升高,拉伸火焰预混锥形结构,促进射流之间相互作用；康达效应使内焰向内壁面弯曲,火焰张角增大；适当调节预混火焰的当量比,有利于火焰结构的稳定。      

多孔介质微燃烧器内的火焰驻定机理研究

为解释毫米尺度多孔介质燃烧器中火焰可在一个当量比范围内驻定的物理现象,搭建了二维非稳态数学物理模型,利用数值计算方法定性研究了氢气/空气预混气在部分填充不锈钢网的微通道内的火焰传播特性。通过分析浸没火焰及表面火焰的温度分布特点并量化燃烧室内的预热和散热发现：火焰驻定在多孔介质内的不同位置时对应的传热特性存在差异,是控制火焰传播速度在一定当量比范围内保持恒定的关键因素,而预热及散热的相对大小可作为衡量传热对火焰宏观影响的重要参数。对火焰的的总预热与总散热之比R越临近多孔介质入口边界变化越剧烈,导致浸没火焰易驻定在多孔介质的中上游区域；多孔介质对火焰的预热虽在多孔介质出口边界外减小,但与多孔介质散热之比Rp呈上升趋势,使得低流速工况下易形成表面火焰。同时,R随当量比的变化规律导致多孔介质下游火焰的稳定性相对较弱。     

限制域、预混气初始温度对多孔介质表面火焰熄火特性的影响

为了对基于多孔介质表面火焰的微型燃烧室技术进行优化设计,以甲烷/空气预混气为研究对象,针对不同的限制域、预混气初始温度,开展了多孔介质表面火焰熄火特性实验研究.实验结果表明:在石英玻璃限制域下,多孔介质表面火焰可以维持在0.188~0.436m/s的低预混气速度下,速度升高容易发生推举和吹熄;而限制域的长度未产生影响作用;随着预混气初始温度从293K升高至550K,多孔介质表面火焰的熄火速度极限得以提高.当量比为1.0时,预混气熄火速度从293K的1.176m/s增加至550K的2.678m/s,并存在不同斜率的上升过程,而初始温度对熄火本质没有影响.     

预混旋流多喷嘴火焰激光可视化实验研究

为了研究预混旋流多喷嘴火焰结构及当量比对多喷嘴火焰结构的影响,针对当量比0.51～0.8的甲烷/空气预混旋流多喷嘴火焰开展了平面激光诱导荧光测量研究。通过实验,获得了不同当量比下预混旋流多喷嘴火焰时均火焰形态和瞬态火焰结构分布特点。实验结果表明,相邻火焰相互冲刷,在相互作用区内强化了燃烧化学反应。相邻火焰之间的相互作用随着当量比的减小逐渐减弱,当量比小于0.53时,中心火焰熄灭,相邻火焰相互作用消失。多喷嘴外侧火焰推举高度小于中心火焰,稳定范围比中心火焰宽。当量比大于0.6时火焰推举高度随当量比的变化不明显,当量比小于0.6后火焰推举高度随着当量比的减小显著增加。随着当量比的降低,湍流脉动对火焰的褶皱扭曲作用逐渐增强,湍流火焰传播速度与层流火焰传播速度之比逐渐增大。     

富油/焠熄/贫油(RQL)燃烧室燃烧和排放特性的实验研究

针对燃气轮机低排放燃烧室的研究,设计了以甲烷为燃料采用预混燃烧的富油/焠熄/贫油(RQL)模型燃烧室。通过对RQL模型燃烧室内轴向温度和组分浓度分布,燃烧室出口温度分布及排放进行实验研究,分析了焠熄与主流空气流量之比,富油区当量比对燃烧性能和排放特性的影响规律。结果表明:典型RQL燃烧方式下富油区火焰颜色较暗,贫油区火焰为淡蓝色,燃烧室内轴线方向温度呈M型分布,NO_x主要在焠熄区生成。CO,UHC和O_2浓度在经历焠熄区时发生突变;出口NO_x和CO排放都较低。保持头部当量比不变,随着焠熄与主流空气流量比的增加,燃烧室出口平均温度下降,NO_x排放下降,CO排放上升。保持焠熄与主流空气流量比不变,富油区当量比小于1.4时,不能再实现RQL燃烧模式。     

多孔介质结构参数对表面火焰熄火特性的影响

为优化基于多孔介质头部的微型燃烧室,以甲烷/空气预混气为燃料,针对多孔介质结构参数(当量孔径、孔隙率)在不同预混气初始温度下,对表面火焰熄火特性进行实验研究.研究表明:当量孔径为120μm的多孔介质表面火焰两侧同时发生脱火,当量孔径为80μm时先发生一侧脱火.随孔隙率或当量孔径的减小,熄火速度提升.当量孔径为80μm,孔隙率为0.55,0.50,0.45的多孔介质在当量比为1.0,预混气初始温度为300K时的熄火速度分别为1.11,1.22,1.31m/s.孔隙率为0.50,孔径为120,80μm的多孔介质在当量比为1.0,预混气温度为300K时的熄火速度分别为0.73,1.22m/s.预混气初始温度的升高对当量孔径为120μm或孔隙率为0.45的多孔介质影响更加明显,预混气初始温度从300K升至500K时,熄火速度分别增加了120%,76%.     

贫燃料湍流预混燃烧火焰稳定性的数值研究

对突扩燃烧室内甲烷-空气预混燃烧进行了数值模拟,时均控制方程组的封闭采用RNG 湍流输运模型和premixed combustion模型.通过模拟研究了不同当量比及进口速度对甲烷-空气预混燃烧效果的影响.CFD数值模拟结果给出了燃烧室内湍流预混反应流的速度场及温度场分布.模拟结果表明当量比为0.6、进口速度为30 m/s时燃烧室内产生稳定预混火焰.该结果对于航空燃气轮机低NOx排放燃烧技术的研究提供了一定的参考条件.     

不同当量比下氢气体积分数对甲烷-氢混合气预混火焰燃烧不稳定性的影响

在可调振幅的正弦波声场作用下,以甲烷-氢混合气预混钝体火焰为实验对象,通过火焰传递函数表征整个燃烧系统的燃烧不稳定性特征,借助CH基自发荧光图像描述火焰锋面运动及演化过程,研究了在声激励下不同当量比（0.8、1.0、1.2）下氢气体积分数的变化（0、10%、20%）对火焰燃烧不稳定的影响。结果表明: 对于当量比为0.8和1.0的预混火焰,氢气的加入使得火焰传递函数幅值增大,热释放波动变大,整体火焰的不稳定性增强;对于当量比为1.2的富燃预混火焰,随着氢气体积分数的增加,火焰传递函数幅值先减小后增加,火焰稳定性较强。      

适用于微小型温差发电器的变通道燃烧室设计研究

本文为微小型半导体温差发电机提供合适的热源,对燃烧器进行了结构设计和数值仿真。通过分析微燃烧器内碳氢燃料稳定燃烧的关键条件和因素,对微燃烧器结构进行了设计计算,并对微燃烧器内甲烷/空气混合物的燃烧情况进行了数值模拟研究,探讨改进后模型当量比、质量流量等因素对甲烷/空气混合物在微燃烧器内燃烧的影响。仿真结果表明:(1)不同的甲烷流量对甲烷燃烧影响程度不同,甲烷流量偏高或偏低的情况下,燃烧室内预混气体都无法正常燃烧;(2)合适的甲烷当量比是实现甲烷稳定高效燃烧的关键性因素;(3)文中设计的变通道结构的燃烧室与恒通道结构的燃烧室相比,室内平均温度更高,且温度分布更均匀,燃烧室平均温度为355K—510 K,在一定条件下新模型既能实现燃烧的安全性,同时对于温差发电元件的受热面而言,热量也得到了均匀分布,使其拥有了更好的工作环境。     

三级旋流燃烧室流动和点火过程中火焰传播特性

为了研究三级旋流燃烧室的流动以及预燃级煤油非预混燃烧特性,设计了三级旋流燃烧室结构方案与光学非接触测量方案,研究了总压损失与当量比对三级旋流燃烧室流动特性及火焰结构的作用和油气参数对点火过程中火焰特征结构与特征时间的影响规律。研究结果表明：在高速气流碰壁区存在内、外剪切层,剪切层的无量纲高度随总压损失变化较小,剪切强度随总压损失增大而增大;火焰结构随着当量比变化存在“V”型火焰、过渡火焰以及包络火焰三种形态,过渡当量比约在0.6左右;热态回流区扩张段扩张角度随总压损失的增大而增大,随着当量比先减小后增大;点火过程中存在大尺度火焰的熄灭与复燃,复燃火焰从回流涡附近以三维螺旋方式回传;点火过程中,随总压损失的增大,火核生成时间增大,火焰传播时间减小,熄火复燃时间减小;随当量比增大,火核生成时间增加,火焰传播时间先增大后减小,熄火复燃时间减小。     

从科技论文的特点看科技论文的选题

本文论述了科技文的特点及选师原则。在特点方面主要就科技论文的科学性,创造性,理论性进行了阐述,在选题方面科技论文选题的客观需要与主条件进行阐述,旨在揭示科技论文的特点与课题选择之间的关系,从而了解其特点,并据此选题,写出符合要求的科技论文。     

某任务计算机调试设备配套软件的设计与实现

简介了任务计算机调试设备配套软件在任务计算机仿真环境中的重要作用 ,对该软件设计方法和流程进行了详细的说明 ,主要介绍了VC ++6 .0环境下串行通信和显示控制软件的设计技术 ,并讨论了如何提高应用程序性能的途径。     

Effect of a transverse plasma jet on a shock wave induced by a ramp

We conducted experiments in a wind tunnel with Mach number 2 to explore the evolution of a transverse plasma jet and its modification effect on a shock wave induced by a ramp with an angle of 24°. The transverse plasma jet was created by arc discharge in a small cylindrical cavity with a 2 mm diameter orifice. Three group tests with different actuator arrangements in the spanwise or streamwise direction upstream from the ramp were respectively studied to compare their disturbances to the shock wave. As shown by a time-resolved schlieren system, an unsteady motion of the shock wave by actuation was found: the shock wave was significantly modified by the plasma jet with an upstream motion and a reduced angle. Compared to spanwise actuation, a more intensive impact was obtained with two or three streamwise actuators working together. From shock wave structures, the control effect of the plasma jet on the shock motion based on a thermal effect, a potential cause of shock modification, was discussed. Furthermore, we performed a numerical simulation by using the Improved Delayed Detached Eddy Simulation(IDDES) method to simulate the evolution of the transverse plasma jet plume produced by two streamwise actuators. The results show that flow structures are similar to those identified in schlieren images. Two streamwise vortices were recognized, which indicates that the higher jet plume is the result of the overlap of two streamwise jets.     

Impact of a cavitation bubble on a wall

Impulse action of a cavitation bubble on a rigid wall is studied depending on the distance between them. We determine the distances at which the periphery pressure maximums on a wall are preserved as well as the distances at which these maximums exceed the water hammer pressure.     

Flow about a jet source with a deflector

We suggest a method to solve one of the model problems of aerohydrodynamics, namely, a problem of a flow about a point source, from which a fluid with density and total pressure, different from the corresponding values in the incoming flow enters. The calculations are carried out for various values of the determining parameter; and the data are compared with the known results. We revealed the advantages of the suggested method in comparison with the known ones.     

Analysis of a redshifted plasma flow over a sunspot

The ultraviolet spectrum of a redshifted plasma flow appearing over a sunspot observed during the first flight of the High Resolution Telescope Spectrograph (HRTS I) is analysed, and interpreted as a radiatively cooling plasma. For most of the lines emitted from this plasma, the assumption of ionization equilibrium during the cooling is good. However for He II (and other ions with a single electron outside of closed shells), this is not the case. Integrating differential equations for the various ionization fractions of helium and the temperature allows an approximate determination of the abundance of helium relative to other elements whose lines appear in the spectrum of the plasma flow.     

The intersection of a Loxodrome with a great circle

The intersections of a loxodrome (rhumb line) and a great circle are of interest for some navigational problems, but a closed-form solution cannot be formulated. An algorithm is given for computing approximations to any desired degree of accuracy using Newton's method. By using the equatorial angle φ as an independent variable all solutions can be found rapidly using the modest computational capabilities of a personal computer     

Oscillations of a viscous liquid in a cylindrical container

The natural damped frequencies of a viscous liquid in a circular cylindrical container are obtained for slipping and anchored contact line at the container wall r = a. In addition the response to translational forced excitation has been determined. The results may also be applied to viscous liquid in a micro-gravity environment, as long as the contact angle of the liquid surface to the cylindrical container wall is in the vicinity of π/2, indicating, that the free liquid surface equilibrium position remains a plane surface. It could be found that there exists in contrast to frictionless liquid a small filling range, in which the liquid performs only an aperiodic motion. The adherence condition at the side wall was replaced by the somewhat weaker condition of an anchored contact line.     

Relativistic Energy-Momentum of a Body with a Finite Volume

The problem of energy-momentum in a body with a finite volume has been causing confusion in the theory of relativity, especially in relativistic thermodynamics. Its correct understanding has been given since the early years of relativity, however, erroneous misunderstandings are still found in papers and textbooks to this date. The present paper introduces a simple paradox to demonstrate the problem, and gives a brief review on a way to handle the energy-momentum correctly.     

Towards a new paradigm: from a quasi-steady description to a dynamical description of the magnetosphere

A great deal of the research done on the dynamical process of the solar wind- magnetosphere interaction is based on large-scale, quasi-steady theoretical models, such as the classical reconnection model. However, it can be argued that the theoretical and observational foundations of these commonly believed paradigms are not always strong, and support for these models is sometimes weak, controversial or inconsistent. This paper discusses the need for a transition from an oversimplified quasi-steady paradigm towards a more realistic one including the dynamics of MHD waves and wave packets. The effects of localized wave packets may be most important in active plasma regions, where ideal MHD breaks down and localized, time-dependent processes become dominant. New insights into the theories of field-aligned current generation, auroral particle acceleration and the concept of reconnection may be found by including MHD wave propagation and wave packet dynamics.