仿生减阻翼型的气动性能

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。      

高空环境下喷嘴参数对航空活塞发动机燃烧与性能的影响

以一台四缸四冲程压燃式航空煤油活塞发动机为研究机型,运用工程系统高级建模和仿真平台软件(AMESim)仿真软件建立了发动机的整机模型,并使用台架实验的采集数据对该仿真模型进行了验证。在高空环境中,仿真分析了飞行器起飞工况、最大巡航工况下发动机喷油器的不同喷孔数、孔径对发动机燃烧过程、性能和NOx排放特性的影响。计算结果表明:稳态工况下,随着喷孔数的增加,最高燃烧压力和温度增加,瞬时放热率增长速度快且峰值上升;同时,缸内预混燃烧得到强化,燃烧始点提前,滞燃期和燃烧持续期缩短,燃烧重心前移,循环热效率增高,但同时会提高NOx的生成量;在飞行器瞬态变海拔的起飞工况下,多喷孔数、小孔径的喷油嘴有利于航空活塞发动机在高空环境下恢复发动机功率,提升飞行器的动力性和续航性能。      

Influence of leading edge with real manufacturing error on aerodynamic performance of high subsonic compressor cascades

To investigate the influence of real leading-edge manufacturing error on aerodynamic performance of high subsonic compressor blades, a family of leading-edge manufacturing error data were obtained from measured compressor cascades. Considering the limited samples, the leading-edge angle and leading-edge radius distribution forms were evaluated by Shapiro-Wilk test and quantile–quantile plot. Their statistical characteristics provided can be introduced to later related researches. The parameterization design method B-spline and Bezier are adopted to create geometry models with manufacturing error based on leading-edge angle and leading-edge radius. The influence of real manufacturing error is quantified and analyzed by self-developed non-intrusive polynomial chaos and Sobol’ indices. The mechanism of leading-edge manufacturing error on aerodynamic performance is discussed. The results show that the total pressure loss coefficient is sensitive to the leading-edge manufacturing error compared with the static pressure ratio, especially at high incidence. Specifically, manufacturing error of the leading edge will influence the local flow acceleration and subsequently cause fluctuation of the downstream flow. The aerodynamic performance is sensitive to the manufacturing error of leading-edge radius at the design and negative incidences, while it is sensitive to the manufacturing error of leading-edge angle under the operation conditions with high incidences.     

轴向间距对压气机通道堵塞及总性能的影响

为了研究转静子叶片排之间的轴向间距对压气机内部流动堵塞及气动性能的影响,选取某单级轴流压气机为研究对象,采用多通道非定常数值计算方法对其5种不同轴向间距下的内部流场进行了全三维数值模拟。结果表明:在每一种轴向间距下,当压气机节流至某一工况之后,压气机通道内的流动堵塞区主要集中在转子叶顶间隙区域和动叶吸力面尾缘附近以及静叶吸力面轮毂角区内;在同一流量下,随着轴向间距的减小,转子叶根吸力面尾缘处的流动堵塞区有所扩大,但转子叶顶间隙区域及静叶吸力面轮毂角区内的流动堵塞区体积却不断减小,压气机通道内回流区的总体积也随之减小,其结果是压气机的静压升能力和流动稳定性增强且效率增大。通过进一步研究发现:在同一流量下,当轴向间距减小时,转子叶顶间隙区域内的主流轴向动量增大且泄漏流的轴向动量减小,其结果是转子叶顶间隙区域内流动堵塞区的体积减小。     

ROPP反演软件算法及其精度分析

介绍了ROPP反演软件中无线电掩星反演的算法与精度分析. 采用COSMIC卫星2008年1 月1日全天的附加相位数据, 反演得到折射率、温度、压强与湿度等参数, 并与CDAAC 相应结果进行对比. 实验结果表明, 在30km高度以下, 折射率、压强和湿度的相对 误差在2%以内, 温度误差不超过2K.      

多视场星敏感器结构参数标定方法

提出一种基于星间角距不变原理的多视场(FOV)星敏感器结构参数标定方法.这种方法以欧拉角表征多视场星敏感器各个子视场之间的旋转关系,利用识别得到的各个视场星点的坐标信息和赤经赤纬信息,计算出多对星光矢量来建立标定模型和目标函数,然后使用L-M算法优化目标函数并解算出各个子视场之间的结构参数.此方法不需要外部姿态测量仪器辅助,可用于在轨和地面标定.在全天球随机抽取多个姿态生成多视场的仿真星图用于标定,并采用星内角统计偏差作为结构参数标定精度的评价指标.这种方法能够准确求解多视场星敏感器的结构参数.星内角统计偏差的平均值在星点位置噪声标准差为0.1像素的仿真试验中为1.3",在外场观星的实际试验中为6.4".      

Flow field characteristics,mixing and emissions performance of a lab-scale rich-quench-lean trapped-vortex combustor utilizing a quench orifice plate combined with a bluff-body

In this study, the low emission combustion technology of Rich-Quench-Lean (RQL) has been applied in Trapped-Vortex Combustor (TVC), and the combinative RQL-TVC shows a promising low emissions performance. By utilizing a quench orifice plate combined with a bluff-body, a lab-scale RQL-TVC was designed. The flow fields of RQL-TVC were measured by 2-D PIV and predicted by 3-D numerical simulation. Flow structures, radial profiles of normalized mean axial velocity, turbulence intensity and mixing level of the quench zone were analyzed. Results reveal that the dual-vortex and the single-vortex flow patterns both exist in cavities and quench zone of RQL-TVC, and the turbulence intensity is strong in the quench zone with some reverse flows. The spiral vortex was discussed by 3-D streamlines and the detail flow structures of the quench zone were analyzed based on the numerical results. The mixing level of the quench zone was determined, and results show that the quench device enhances the mixing level compared with TVC. Combustion efficiency and emissions performance were investigated experimentally, and results demonstrate that RQL-TVC has relatively higher combustion efficiency and lower emission index of CO, UHC and NO_x than the same size lab-scale TVC in present work.     

The effective temperatures of O-type stars from UV spectroscopy

We present an analysis of high resolution spectra in the far-UV – UV range (∼905–2000 Å) with non-LTE, spherical, hydrodynamical, line-blanketed models, of three O-type Galactic stars, and derive their photospheric and wind parameters. These data extend previously analyzed samples and fill a gap in spectral type coverage. The combined sample confirms a revised (downward) T_eff scale with respect to canonical calibrations, as found in our previous works from UV and optical spectra, and in recent works by other authors.     

激波引燃冲压发动机一体化流场数值模拟

激波引燃冲压发动机是一种采用爆轰形式组织燃烧的吸气式高超声速飞行器动力系统。采用AUSMPW+迎风格式、氢氧7组分8步基于反应模型,在非结构网格离散域上求解二维多组分化学非平衡流Euler方程。采用发展的数值方法求解了激波引燃冲压发动机内外一体化流场,研究了台阶长度、斜劈尖角度对发动机流场结构和发动机性能参数的影响规律。计算结果表明,所发展的数值方法能用于激波引燃冲压发动机的一体化流场和性能预示计算;台阶长度和斜劈尖角度影响发动机流场结构和预混气体能量释放程度。推力和燃料比冲均随台阶长度的增大而增大,随斜劈尖角度的增大而减少。     

Quasars and their emission lines as cosmological probes

Quasars are the most luminous sources in the Universe. They are currently observed out to redshift z≈7$z\approx 7$ when the Universe was less than one tenth of its present age. Since their discovery 50 years ago astronomers have dreamed of using them as standard candles. Unfortunately quasars cover a very large range (8 dex) of luminosity making them far from standard. We briefly review several methods that can potentially exploit quasars properties and allow us to obtain useful constraints on principal cosmological parameters. Using our 4D Eigenvector 1 formalism we have found a way to effectively isolate quasars radiating near the Eddington limit. If the Eddington ratio is known, under several assumptions it is possible to derive distance independent luminosities. We discuss the main statistical and systematic errors involved, and whether these “standard Eddington candles” can be actually used to constrain cosmological models.