有关误差的基本概念与表示

阐述了“测量误差”、“测量不确定度”及“测量准确度，，等计量学基本概念，明确指出了这些概念的内涵、表达方法及使用中应注意的问题，并讨论了它们的联系与区别。     

N2O/丙烷火箭发动机研制

为进行N2O/丙烷(C3H8)火箭发动机(NOP)试验,在亚拉巴马大学(UAH)新建了一座发动机试车台,装备了台架式推进剂供应系统、10001bsf(4448.22N)的推力架和数据采集系统.研究了N2O催化分解点火方案,对几种催化剂材料进行了评估.Shel1-405和钴基的ZSM-5性能良好,可使N2O充分分解,并点燃碳氢燃料,如丙烷.试验表明,纯N2O通过Shel1-405时,催化分解反应在400°F(204℃)时进行,如果加入少许碳氢燃料(例如丙烷或丙烯),此温度将下降到大约200°F(93℃).NOP发动机在L*=3m时,在混合比4.89到8.68之间进行了试验.在合适的热损失模型下,试验数据与理论计算结果相吻合.使NOP发动机稳定工作的范围基本确定为N2O流量＜0.270 1bm/sec(0.122kg/s),混合比在5～6之间.用辐射测量仪来测量发动机排气温度和羽流成分,用羽流皮托管校验推力数据.     

K—ε两方程模型的改进及其应用

本文对标准的k-ε两方程模型进行了改进。摒弃了v_t=C_μ(k~2/ε)的假定,而从雷诺应力方程和Rodi的简化假设出发,得出了计算v_t的新表达式(10)。算例表明,它对时均速度u的计算结果比标准k-ε模型更精确。     

Pro／ENGINEER在模具设计中的使用技巧

分析了Pro／ENGINEER进行模具设计的使用技巧，阐明了并行工程技术与Pro／ENGINEER软件相结合的重要性。     

浅议我国责任会计体系存在的问题及对策

20世纪80年代开始,我国的企业大胆吸收西方先进的责任会计思想,从加强内部机制入手,提高管理水平,增强市场竞争力,责任会计曾一度受到较大重视并发挥了积极的作用.但随着市场经济的进一步发展和现代企业制度的建立,我国企业在推行责任会计过程中也出现了种种问题,本文就我国企业责任会计体系存在的问题及建议谈几点看法.     

基于星体边缘和轨道投影的光学自主导航算法

针对光学导航中存在的通过星体（球体）图像部分边缘点拟合椭圆参数计算轨道参数产生中间误差的问题,提出利用边缘点映射轨道参数的直接投影模型,避免拟合椭圆参数的方法。在小孔成像模型基础上,建立了边缘点与轨道参数的直接投影数学模型,对其映射过程进行了理论推导,利用列文伯格-马夸尔特迭代算法进行求解轨道参数。用实际探测器以及镜头参数进行数值仿真验证,结果表明：该方法在相同边缘点的条件下,轨道精度可以达到5‰。与传统方法相比,这种方法避免了椭圆的拟合过程,减少了引入中间误差过程。     

Ground experiments of Chang’e-5 lunar regolith penetrating radar

The Lunar Regolith Penetrating Radar (LRPR) is an Ultra-Wideband (UWB) array-based Ground penetrating radar (GPR) onboard the lander of Chang’e-5 (CE-5) mission. The primary scientific objectives of the LRPR are to probe the thickness and structure of lunar regolith of the landing site, and support the drilling and sampling process. In order to evaluate the performance of the LRPR, a series of ground experiments are performed using the LRPR prototype mounted on a CE-5 lander model. The performance of the LRPR is evaluated by comparing the experimental data with the simulated data. Data processing and imaging method are verified, and the interferences from the lander and other aspects are analyzed. The results of the ground experiments and simulation demonstrate that the LRPR is able to meet the design requirement of 2-m detection depth. They also indicate that the upper and lower interfaces of the stratified structure in the lunar regolith can be well distinguished by the LRPR when the dielectric constant difference is greater than 0.3, and the imaging effect of the location under the dense antennas is better than that of other positions. However, the identification capability of the LRPR to the independent blocky objects is relatively poor mainly due to the clutters caused by the lander, the sparsity of the antenna elements compared to the size of the basalt block, the limited aperture of the antenna array, and the tail of the transmitted waveform.     

Simulation and analysis of chemical release in the ionosphere

Ionospheric inhomogeneous plasma produced by single point chemical release has simple space-time structure, and cannot impact radio wave frequencies higher than Very High Frequency (VHF) band. In order to produce more complicated ionospheric plasma perturbation structure and trigger instabilities phenomena, multiple-point chemical release scheme is presented in this paper. The effects of chemical release on low latitude ionospheric plasma are estimated by linear instability growth rate theory that high growth rate represents high irregularities, ionospheric scintillation occurrence probability and high scintillation intension in scintillation duration. The amplitude scintillations and the phase scintillations of 150?MHz, 400?MHz, and 1000?MHz are calculated based on the theory of multiple phase screen (MPS), when they propagate through the disturbed area.