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91.
仿生减阻翼型的气动性能 总被引:1,自引:1,他引:0
利用一种基于滑移边界理论的仿生肋条结构的模化方法,对仿生减阻翼型的气动性能开展了数值模拟研究。结果显示:肋条结构同时布置在翼型压力面和吸力面湍流区域时,仿生减阻翼型的阻力可降低1.73%~3.07%,升阻比可提高2.10%~4.08%,其中黏性阻力的减小是总阻力下降的主要原因。对流场分析表明,仿生减阻翼型的速度曲线出现一定抬升,使得湍流边界层中的黏性子层增厚,进而导致了仿生减阻翼型气动性能的提升。 相似文献
92.
分布式动力系统尾缘射流与边界层抽吸的数值分析 总被引:2,自引:2,他引:0
为研究带有边界层抽吸的分布式动力系统尾缘射流对机身气动性能及推进效率的影响,将机身简化为二维翼型,并加入尾缘射流及边界层抽吸的作用,利用数值模拟的手段来研究来流攻角、射流偏转角、边界层抽吸对推进效率及气动性能的影响,为分布式动力系统的设计与应用提供初步的建议.结果表明在中、小来流攻角(2°及0.6°)的情况下尾缘射流及边界层抽吸能够提高升阻比,推进效率可超过80%;而在大来流攻角(4°)情况下射流偏转角增大使翼型的阻力大幅上升,对气动性能和推进效率产生极为不利的影响. 相似文献
93.
基于放大因子与Spalart-Allmaras湍流模型的转捩预测 总被引:1,自引:0,他引:1
为了验证放大因子输运方程与Spalart-Allmaras(S-A)湍流模型耦合对转捩现象的模拟精度,选取Schubauer and Klebanoff(S-K)平板、S809低速翼型、30p30n多段翼型以及复杂的三维HiLiftPW-1构型进行自由转捩计算,并将计算结果与实验进行比较分析,其中针对S809算例,还与Langtry-Menter(L-M)转捩模型进行了比较.算例结果表明:放大因子输运方程与S-A湍流模型的耦合能够较好的捕捉转捩位置以及转捩发展过程,对分离泡诱导的转捩的模拟相比L-M转捩模型更精确,转捩位置的捕捉精度提升了10%;对比实验,多段翼转捩位置的捕捉误差最大为6.5%;针对三维高升力增升构型,以实验作为参考,全湍流计算与考虑边界层转捩的对比显示考虑边界层转捩能够更加精确的模拟气动力系数,升力和表面摩擦阻力系数的模拟精度精度提升1%. 相似文献
94.
95.
飞行器在高空高速飞行时黏性效应显著,摩阻预示精度对飞行器的关键气动性能意义重大。目前,摩阻预示主要依赖数值计算,但高马赫数层流摩擦阻力计算与试验测量结果仍存在差距。以具有高速飞行器典型部件特征的球锥、三角翼为对象,结合风洞试验摩阻测量结果,使用国家数值风洞(NNW)数值计算软件和自研CFD程序研究了数值计算中影响摩阻计算精度的格式数值耗散及壁面温度边界条件等重要因素。研究结果表明:数值耗散越小,表面摩阻的计算精度越高;在速度较低的边界层近壁区内关闭熵修正,将有助于提高表面摩阻的预示精度。此外,在高马赫数流动问题的数值模拟中,壁面温度条件对表面摩阻计算同样具有重要影响。最后,基于分析结果和工程需要提出了对高精度摩阻数值预示的研究需求。 相似文献
96.
超声速条件下燃料和空气之间的高效混合是超然冲压发动机技术上的主要挑战。基于大涡模拟和流动稳定性分析,针对超声速尾迹-剪切流动开展了混合增强方法研究。尾迹的存在改变了混合层流动的速度剖面,对流动稳定性产生了重要影响,使混合层由三维最不稳定变为二维最不稳定,最不稳定扰动波频率和增长率增大。基于流动稳定性结果引入扰动的混合增强方式依然有效,根据稳定性结果设计了波纹隔板。数值结果表明:二维波纹壁引入的扰动未能增长,不具备混合强化效果,而三维波纹壁引入的扰动能够快速增长,具有混合强化效果,且波纹壁参数越接近最不稳定扰动波参数,混合强化效果越明显。 相似文献
97.
Numerical investigation of the impact of asymmetric fuel injection on shock train characteristics 总被引:1,自引:0,他引:1
Numerical simulations are carried out to investigate the impact of asymmetric fuel injection on shock train characteristics using the commercial-code FLUENT. The asymmetry of fuel injection is examined by changing the fuel flow rates of the upper and lower wall fuel injectors. The numerical approach solves the two-dimensional Reynolds-averaged Navier–Stokes (RANS) equations, supplemented with a k-ω model of turbulence. As a result, different ways of fuel injections will always lead to shock train transitions, with the variations of shock train structure, strength and leading edge position. For symmetric fuel injection, the flowfield of the isolator is quite asymmetric with the boundary layer of the upper wall side developing much stronger than that of the lower wall, which is due to the heterogeneity of the incoming flow. Regarding to asymmetric fuel injection with more of lower wall side, though the pressures in the combustor are nearly the same, the first shock of the shock train converts between ‘Distinct symmetric X type shock’ and ‘Obscure and weaker asymmetric shock’ and the shock train leading edge moves upstream with the increase of the asymmetry level. With regard to asymmetric fuel injection with more of upper wall side, ‘incomplete asymmetric X type shock’ occurs and the shock train structures keep nearly the same with low level of fuel injection asymmetry. Unexpected results like unstart will happen when increasing the level of fuel injection asymmetry. And the isolator will come back to normal state by decreasing the differential of upper and lower wall sides fuel injections. 相似文献
98.
N. Mridula Tarun Kumar PantC. Vineeth K. Kishore Kumar 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The general features of occurrence of an additional layer on the bottom side of F region, referred to as F0.5 layer in the pre noon period, over the magnetic equatorial location of Trivandrum (8.5° N; 77° E; dip lat of 0.5° N) in India during the period from 2004 to 2007 are presented using ionosonde observations. The F0.5 layer has a June (northern summer) solsticial maximum probability of occurrence with secondary maxima during December (northern winter) solstice. The seasonal as well as the day-to-day variability in the occurrence of F0.5 layer as mentioned in this paper seems to be a result of the variations in the amplitude and phases of the tides and gravity waves, and inventory of the metallic ions of meteoric origin. This study brings out an important manifestation of morning time F layer base region dynamics. 相似文献
99.
N. Zolotukhina N. Polekh E. Romanova A. Polyakova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We report work utilizing 15-min resolution ionospheric data obtained with DPS-4 digisonde in 2003–2011 to study the seasonal variations in amplitudes and phases of the most powerful spectral components of the F2 layer critical frequency (foF2) and peak height (hmF2) fluctuations over Irkutsk (52.5°N, 104.0°E). We show that fluctuations of both parameters contain quasi-harmonic components with periods of Tn = 24/n h (n = 1–7). The number of distinct spectral peaks varies from 3 in summer to 7 in winter. Amplitude and phase characteristics of the diurnal (n = 1) and semidiurnal (n = 2) components is studied using the data sets extracted from the original data sets with band-pass filter. It has been found that the amplitudes of diurnal/semidiurnal foF2 and diurnal hmF2 components are maximum in winter and minimum in summer. Amplitudes of the diurnal components vary gradually; those of the foF2 semidiurnal one, abruptly, thus forming a narrow winter maximum in November–January. The phase (local time of maximum) of the diurnal foF2 component increases gradually by 4–6 h from winter to summer. The phase of the semidiurnal foF2 component is nearly stable in winter/summer and sharply decreases (increases) by 2–3 h near the spring (autumn) equinox. The phase of the diurnal component of hmF2 (local time of minimum) varies slightly between 1130 and 1300 LT; that of the semidiurnal one decreases (increases) by 4–6 h from January to March (from September to November). The results obtained show that the main features of seasonal variations in the diurnal and semidiurnal components of the mid-latitude F2 layer parameters recur consistently during the solar activity growth and decline phases. 相似文献
100.
M. Pietrella M. PezzopaneC. Bianchi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Hourly systematic measurements of the highest frequency reflected by the sporadic-E layer (foEs) recorded from January 1976 to June 2009 at the ionospheric stations of Rome (Italy, 41.8°N, 12.5°E) and Gibilmanna (Italy, 37.9°N, 14.0°E) were considered to carry out a comparative study between the sporadic E layer (Es) over Rome and Gibilmanna. Different statistical analysis were performed taking into account foEs observations near the periods of minimum and maximum solar activity. The results reveal that: (1) independently from the solar activity, Es develops concurrently over extended regions in space, instead of being a spatially limited layer which is transported horizontally by neutral winds over a larger area; especially during summer months, when an Es layer is present at Rome, there is a high probability that an Es layer is also present over Gibilmanna, and vice versa; (2) Es layer lifetimes of 1–5 h were found; in particular, Es layers with lifetimes of 5 h both over Gibilmanna and Rome are observed with highest percentages of occurrence in summer ranging between 80% and 90%, independently from the solar activity; (3) latitudinal effects on Es layer occurrence emerge mostly for low solar activity during winter, equinoctial, and summer months, when Es layers are detected more frequently over Gibilmanna rather than Rome; (4) when the presence of an Es layer over Rome and Gibilmanna is not simultaneous, Es layer appearance both over Rome and Gibilmanna confirms to be a locally confined event, because drifting phenomena from Rome to Gibilmanna or vice versa have not been emphasized. 相似文献