弧齿锥齿轮齿面优化修正及计算机仿真

由于加工误差和热处理变形等因素的影响 ,实际弧齿锥齿轮齿面啮合质量通常与“轮齿接触分析”(TCA)所得的理论结果有所差异。本文提出了基于最小二乘法的加工参数识别方法和齿面优化修正方法 ,经计算机仿真验证 ,修正后的齿面与原设计的齿面 ,具有非常近似的 TCA结果。     

弧齿锥齿轮的齿距误差对传动性能的影响研究

采用齿轮啮合仿真和承载啮合仿真技术 ,对重合度达到 2 .0的航空弧齿锥齿轮的齿距误差的影响进行了研究。首先定义了航空弧齿锥齿轮相对齿距误差 ,选取了量级 ,研究了这一误差对齿轮实际重合度、传动误差、齿面载荷分布和齿间载荷分配的影响。进一步又分析了在一定齿距误差下载荷变化的影响以及固定载荷下误差变化的影响 ,为高重合度航空弧齿锥齿轮的应用提供了依据     

高重合度弧齿锥齿轮的强度分析

本文采用有限元应力影响矩阵法研究了高重合度弧齿锥齿轮在多种误差和载荷条件下的弯曲应力状态 ,证明了经过优化设计的高重合度弧齿锥齿轮不仅有良好的动态性能 ,而且在一定误差范围内在强度方面具有优越性     

亚声S型进气道模型吹风试验特性的研究

采用半经验的方法，对某S型进气道的模型试验数据进行了回归，建立了弹用涡喷（扇）发动机常用S型高亚声速进气道总压恢复系数与习行马赫数Ma，流量系数ψ，攻角α和侧滑角β的相关函数关系。该关经验公式可用于发动机稳态和启动加速过程一元数值仿真模型，从而提高一元发动机性能数值仿真计算的准确性。     

基于共轭方程法的跨音速机翼气动力优化设计

 设计状态的机翼气动力特性是设计人员最为关心的指标, 应用控制理论设计方法进行了有升力约束情形下跨音速机翼阻力优化设计研究, 根据给定的目标函数推导了相应的共轭方程和边界条件, 研究了共轭方程的数值求解方法, 以及计算目标函数对设计变量的敏感性导数时所涉及的度量矩阵变分求解问题, 研究了流场计算、共轭方程数值求解、敏感性导数求解和拟牛顿优化算法这几个主要方面的有效结合问题, 发展出了一种跨音速机翼气动力优化设计方法, 进行了跨音速机翼气动力优化设计研究验证, 优化后机翼气动力特性有一定程度的改善, 阻力系数能减少20%左右, 而升力系数有所增大, 说明所发展的设计方法是成功的, 该设计方法在跨音速及复杂外形气动设计方面比以往设计方法具有更好的适用性和优越性。     

Prospects of Global Navigation Satellite System (GNSS) reflectometry for geodynamic studies

Innovative processing of satellite radar altimetry over solid Earth has been successfully applied for observing geodynamic process of glacial isostatic adjustment over the former Laurentide Ice Sheet in the present-day Hudson Bay land region. In this contribution, a simulation is conducted to study the prospects of the applications of space-/airborne and land-based Global Navigation Satellite System (GNSS) reflectometry to synoptically observe global-scale geodynamic processes with a vertical accuracy of ∼2 mm/yr.     

Effects of X2-class solar flare events on ionospheric GPS-TEC and radio waves over Brazilian sector

In this investigation, we present and discuss the effects of 6 X2-class solar flare events in the ionospheric F region over Brazilian sector that occurred during 2013 to 2015. For this investigation, we present the vertical total electron content (VTEC) observations from nearly 120 Global Positioning System (GPS) receivers all over the Brazilian sector for each event. Also, ionospheric sounding observations obtained in São José dos Campos (23.2°S, 45.9°W, dip latitude 17.6°S; hereafter referred to as SJC), under the southern crest of the equatorial ionospheric anomaly (EIA), Brazil, are presented. The observations show that the greatest TEC impact occurs with the EUV fluxes increases lasting for more than one hour and when the solar active region is located close to the solar disc center. We present a detailed study of the efficiency of the EUV flux with wavelengths ranging from 0.1 to 190?nm for the F region ionization. The largest increase of ΔTEC occurs below the magnetic equator line, covering mainly the central, northeast, southeast and south regions, which includes the equatorial ionospheric anomaly (EIA) region. The ionograms show partial or total fade out in the echoes traces observed causing blackouts of radio signals of up to 60?min, which can have serious consequences to technological systems of public and private agencies around Brazilian sector. This study can help to better understand the effects of solar flares in the ionospheric F region.