乘波飞行器广义参数概念设计

在传统布局外形设计参数的基础上，提出用广义参数对乘波飞行器概念外形进行前体／进气道-后体／喷管一体化设计。对所设计的三种外形方案，计算了设计点和非设计点的气动性能，并对影响性能的因素进行了讨论。计算结果表明，采用广义参数设计乘波飞行器概念外形是可行的。     

钻尖数控刃磨中的尾隙角研究

通过对尾隙角的分析研究,提出了作用尾隙角的概念,给出了作用尾隙角的计算方法,研究了刃磨参数对作用尾隙角的影响.给出了作用尾隙角在数控刃磨求取刃磨参数中的应用方法.研究表明,尾隙角是关系到钻头钻削性能的重要参数,数控刃磨中的几个刃磨参数对它的影响程度由大至小的次序为θ、C_y、σ、ω、C_x.     

磨粒特征参数的筛选及权分析

基于概率分布特性及集合论 ,提出区分度概念并建立一种用于对金属磨粒的特征参数进行分析筛选的方法。该方法根据特征参数的数据结构特征 ,筛选出具有较强分类特性的特征参数 ,而将分类特性差的或是派生的特征参数能准确地分离出来。本文同时采用集合域分析方法 ,对特征参数进行了权分析 ,从而大大提高了特征参数的分类特性。文中对金属磨粒分类中常用的几种几何特征参数 (圆度、长 /短轴比、线性度、凹度及综合参数 )进行了计算分析 ,结果显示圆度的区分度最大 ,其他依次为长 /短轴比、综合参数、凹度和线性度。而这一结果与作者根据实际经验来对磨粒进行分类所采用的分类决策的秩序是相一致的 ,从而说明该方法的有效性及实用性     

参数化装配方法研究(英文)

参数化零件的装配是一个很复杂的问题。本文论述了以辅助线法生成的参数化零件为基础,交互输入定位关系、装配关系,通过平移、旋转等编辑操作功能,拼成装配图,实现了装配图与零件图的同步参数化驱动。文中对装配图的数据结构、装配过程实现的图形消隐等关键技术作了详细描述,并应用于实际工程,取得了良好效果.     

特材零件除油工艺参数的优化研究

特材零件除油作为表面处理重要而又关键的环节,直接影响表面膜层的形 成和性能。本文重点论述了除油工艺的重要性和特材零件油污的来源,并有针对性的对 汽油浸泡、表面活性剂超声清洗、阴极电解除油等除油方法进行试验研究,优化各工序 工艺参数。除油效果采用水润法进行检验,检验结果表明：试验确定的除油工艺方法合 理,效果明显,去除了特材基体表面油污,露出了活泼的特材基体,为特材表面获得优 良的表面处理膜层打下了基础。     

雷达参数对SAR图像中Kelvin尾迹的影响

舰船尾迹的SAR成像受到船艇自身、海洋环境和SAR系统等多种因素的影响,其中起主要作用的是雷达参数的影响。文章重点对影响舰船Kelvin尾迹SAR成像的SAR系统参数进行了详细讨论和分析,其中包括极化方式、视向角、频率以及入射角对Kelvin尾迹的影响因素。给出了各种参数对尾迹成像的影响规律,通过此规律有助于下一步得出舰船尾迹的最佳观测条件。     

基于Gauss平均引数的RNAV进近程序航迹引导参数计算

为准确计算基于WGS-84坐标的RNAV进近程序航路点坐标和航迹引导参数,提供精密RNAV导航数据,降低RNAV进近系统误差,提出了实测跑道入口WGS-84坐标,然后沿跑道中线外推各航路点WGS-84坐标的计算方法。采用Gauss平均引数法对各航段的航线角及航段距离进行了反算,以验证外推航路点坐标的计算精度。通过西南地区某机场＂T＂型RNAV进近程序的设计及飞行验证,该方法可推广到其他机场的RNAV进近程序设计。     

Evaluation of global modeling of M(3000)F2 and hmF2 based on alternative empirical orthogonal function expansions

Global modeling of M(3000)F2 and hmF2 based on three alternative EOF (empirical orthogonal function) expansion methods is described briefly. Data used for the model construction is the monthly median hourly values of M(3000)F2 from the ionosonde/digisonde stations distributed around the world for the period of 1975–1985 and the hmF2 data of the same period converted from the measured M(3000)F2 based on the strong anti-correlation existing between them. Independent data of a low (1965) and a high (1970) solar activity year are used to validate the three alternative models based on different EOF expansion methods. Comparisons between the modeled results and observed data for both the low (1965) and high (1970) solar activity years showed good agreement for both M(3000)F2 and hmF2 parameters. Statistical analysis on the differences between model values and observed data showed that all the three alternative models (Model A, B and C) based on the different EOF expansion methods have better agreement with the observed data than the models currently used in IRI. All three alternative EOF based models have almost the same accuracy. Discussion on the preference of the three alternative EOF based models is given.     

Validation of B2bot in the NeQuick model during high solar activity at Hainan station

NeQuick ionospheric electron density model, which has been developed to version 2, produces the full electron density profile in the ionosphere. Each part of the profile is modeled using Epstein layer formalism. Simple empirical relations are used to compute the thicknesses of each layer. In order to validate the B2_bot parameter in the NeQuick model during high solar activity, we use the data at Hainan, China (109.1°E, 19.5°N; Geomagnetic coordinates: 178.95°E, 8.1°N), measured with DPS-4, and study the diurnal and seasonal variations of B2_bot, ΔB2 (B2_best − B2_NeQuick 2) and the seasonal median values of B2_best/B2_NeQuick 2 at that region. The results show that, (1) The differences between B2_best and B2_NeQuick 2 have diurnal and seasonal variations. (2) The diurnal variations of B2_NeQuick 2 are smaller than those of B2_best. (3) Generally, except for early morning the experimental values are properly reproduced. (4) Generally, during morning the NeQuick model has an underestimation. The magnitude of underestimation varies with LT and season.     

An intercomparison of meteor radar measurements at the South Pole using two different processing systems

A new meteor radar system was installed at the Amundsen–Scott station South Pole in 2001 to further the understanding of the dynamics of the Antarctic region. The antenna array consists of four yagis pointed along the 0°, 90°, 180°, and 270° meridians and five folded crossed dipoles arranged in a cross configuration and operating as an interferometer to provide position measurements for the detected radio meteors. The four yagis are time division multiplexed and used for both transmitting and receiving while the five folded crossed dipoles are only used for reception. The current arrangement of data acquisition (DAQ) systems at the South Pole allows the collection of meteors in a configuration similar to the previous meteor radar system that operated at the South Pole in the mid 1990s while also using an interferometer to accurately determine the meteor positions in the sky, which enables the determination of the vertical structure of the observed waves. This has been accomplished through the use of two DAQ and post-processing systems: COBRA (Colorado Obninsk radar) connected to the yagis and MEDAC (meteor echo detection and collection) connected to the folded crossed dipoles. With two separate DAQ systems operating in parallel we have the ability to directly compare the results and understand the inherent variability in the derived scientific results based on different system architectures and processing assumptions. The impact of operating a system without an interferometer on the amplitudes and phases of the observed wave components is considered. We find that the lack of altitude resolution of the COBRA DAQ system leads to an underestimation of the amplitude of the s = 1 component of the semidiurnal tide of ∼20% during the summer months.