Influence of Multi-hole Arrangement on Cooling Film Development

A series of computations is conducted for many multi-hole arrangements at several blowing ratios to further investigate the evolution of the film from multi-holes. The influence of multi-hole arrangement on effusion film cooling is analyzed and a preliminary relationship evaluating the film development from developing state to developed state is brought forward. Results show that the coolant jets from front rows of multi-holes merge rapidly and the strength of the kidney vortices due to mainstream-coolant jet interaction in the downstream region are mitigated under super-long-diamond arrangement where the streamwise hole-to-hole pitch is bigger than spanwise hole-to-hole pitch. The holes array arranged in super-long-diamond mode is not only in favor of obtaining developed film layer, but also improving averaged adiabatic film cooling effectiveness.     

A Tracking Filter in Spherical Coordinates Enhanced by De-noising of Converted Doppler Measurements

Tracking problem in spherical coordinates with range rate (Doppler) measurements, which would have errors correlated to the range measurement errors, is investigated in this paper. The converted Doppler measurements, constructed by the product of the Doppler measurements and range measurements, are used to replace the original Doppler measurements. A de-noising method based on an unbiased Kalman filter (KF) is proposed to reduce the converted Doppler measurement errors before updating the target states for the constant velocity (CV) model. The states from the de-noising filter are then combined with the Cartesian states from the converted measurement Kalman filter (CMKF) to produce final state estimates. The nonlinearity of the de-noising filter states are handled by expanding them around the Cartesian states from the CMKF in a Taylor series up to the second order term. In the mean time, the correlation between the two filters caused by the common range measurements is handled by a minimum mean squared error (MMSE) estimation-based method. These result in a new tracking filter, CMDN-EKF2. Monte Carlo simulations demonstrate that the proposed tracking filter can provide efficient and robust performance with a modest computational cost.     

基于案例推理的机场应急预案管理

为提高机场应急处置能力,提出一种新的基于案例推理方法的机场应急救援模型。利用XML技术来表示案例和构造预案库,给出机场应急预案库的分类方法,构建预案特征属性的层次结构。采用两两比较打分法确定航空器紧急事件预案特征属性的权重．运用最邻近算法对已有救援案例进行检索与匹配。实例证明该方法能有效提高机场应急救援效率,检索结果客观合理。     

Dynamic and figure parameters of Venus and Mars

Parameters of the best-fitting tri-axial ellipsoids representing external equipotential surfaces of Venus and Mars have been determined from satellite data. The dynamic consequence of the equatorial flattening of Venus has been discussed from the point of view of the s.c. synodic resonance rotation. The major gravitational anomalies of Venus have been interpreted, space locations and magnitudes of anomalous masses determined and their contribution to the second zonal Stokes' constant in the gravitational potential computed. The conclusions were done: The figure of the aphroditoid is strange even if there is a relatively small polar flattening; an equatorial “disc” of Venus is enormous. Recent space data do not support hypothesis that the Earth controls the spin of Venus.     

纳米压痕实验微米级深度硬度下降现象的研究(英文)

本文针对均匀材料微米级压痕深度,分析接触深度、接触面积、载荷以及加载时间几种因素对实验数据的影响,结合有限元数值模拟,说明压头几何缺陷、接触深度与接触面积的处理并不是造成微米级压痕硬度随压深增大而下降的主要原因,最可能的原因是材料的蠕变特性。进行了不同最大压深实验显示连续刚度法(CSM)将强化蠕变特性对硬度曲线的影响,证明造成该现象的重要原因是纳米压痕实验的实验方法问题。     

形貌和空间对PAEK增韧BMI树脂及其碳纤维复合材料层压板韧性和冲击损伤阻抗的影响(英文)

通过对热塑性树脂PAEK增韧BMI树脂的玻璃化转变行为,相形貌和断裂韧性,以及对采用"离位"概念增韧的T700/BMI复合材料的层间形貌及其冲击后压缩强度(CAI)的分析,研究了微结构-性能之间的关系,发现特征相分离形貌随着PAEK的含量而变化。特别探索了PAEK-BMI复相体系的相形貌与断裂韧性之间的关系,得到的断裂机理解释了复合材料层压板的分层和冲击损伤行为。有关"离位"增韧的机理、以及扩散控制的相行为等还需要继续研究。     

Plasma Morphology at Mars. Aspera-3 Observations

A total of about of 400 orbits during the first year of the ASPERA-3 operation onboard the Mars Express spacecraft were analyzed to obtain a statistical pattern of the main plasma domains in the Martian space environment. The environment is controlled by the direct interaction between the solar wind and the planetary exosphere/ionosphere which results in the formation of the magnetospheric cavity. Ionospheric plasma was traced by the characteristic “spectral lines” of photoelectrons that make it possible to detect an ionospheric component even far from the planet. Plasma of solar wind and planetary origin was distinguished by the ion mass spectrometry. Several different regions, namely, boundary layer/mantle, plasma sheet, region with ionospheric photoelectrons, ray-like structures near the wake boundary were identified. Upstream parameters like solar wind ram pressure and the direction of the interplanetary electric field were inferred as proxy from the Mars Global Surveyor magnetic field data at a reference point of the magnetic pile up region in the northern dayside hemisphere. It is shown that morphology and dynamics of the main plasma domains and their boundaries are governed by these factors as well as by local crustal magnetizations which add complexity and variability to the plasma and magnetic field environment.     

Random Weighting Estimation Method for Dynamic Navigation Positioning

This paper presents a new random weighting estimation method for dynamic navigation positioning.This method adopts the concept of random weighting estimation to estimate the covariance matrices of system state noises and observation noises for controlling the disturbances of singular observations and the kinematic model errors.It satisfies the practical requirements of the residual vector and innovation vector to sufficiently utilize observation information,thus weakening the disturbing effect of the kinematic model error and observation model error on the state parameter estimation.Theories and algorithms of random weighting estimation are established for estimating the covariance matrices of observation residual vectors and innovation vectors.This random weighting estimation method provides an effective solution for improving the positioning accuracy in dynamic navigation.Experimental results show that compared with the Kalman filtering,the extended Kalman filtering and the adaptive windowing filtering,the proposed method can adaptively determine the covariance matrices of observation error and state error,effectively resist the disturbances caused by system error and observation error,and significantly improve the positioning accuracy for dynamic navigation.     

中国通用航空区域发展水平综合测评

为了科学评价目前中国各区域通用航空发展水平,为国家政府层面、民航局层面、地方政府层面制定中国各区域通用航空发展政策提供依据,以2009年中国通用航空区域发展水平为研究对象,按照中国七大中国民用航空地方管理局（华北、华东、东北、中南、西北、西南、新疆）进行区域划分,从各区域通用航空运营规模、运营效率两大方面建立评价体系。运用层次分析法（AHP）确定评价指标体系中七个指标的权重,利用灰色关联分析法测算中国七大区域通用航空发展水平。最后根据灰色关联度值将七个区域的通用航空发展水平进行了由高到低的排序,并找出中国通用航空发展相对较好和相对落后的区域。     

Global Muon Detector Network Used for Space Weather Applications

In this work, we summarize the development and current status of the Global Muon Detector Network (GMDN). The GMDN started in 1992 with only two muon detectors. It has consisted of four detectors since the Kuwait-city muon hodoscope detector was installed in March 2006. The present network has a total of 60 directional channels with an improved coverage of the sunward <a href='/search?dc.title=Interplanetary+Magnetic+Field&amp;facet-content-type=ReferenceWorkEntry&amp;sortOrder=relevance' class='reference-link webtrekk-track' gaCategory="internal-link" gaLabel="Interplanetary Magnetic Field" gaAction="reference-keyword">Interplanetary Magnetic Fielda> (IMF) orientation, making it possible to continuously monitor cosmic ray precursors of geomagnetic storms. The data analysis methods developed also permit precise calculation of the three dimensional cosmic ray anisotropy on an hourly basis free from the atmospheric temperature effect and analysis of the cosmic ray precursors free from the diurnal anisotropy of the cosmic ray intensity.