CFM56-7B发动机推力等级改装的技术方法

介绍了CFM56-7B发动机推力等级、发动机推力更改的设计原理、系统构型差异以及推力更变设置的具体操作方法.     

Variability of the ionosphere over Irkutsk at low solar activity

Statistical and spectral analyses are performed to investigate variations of two ionosphere F2 layer key parameters, the critical frequency (foF2) and the peak height (hmF2), that were measured over Irkutsk (52.5°N, 104.0°E) from December 2006 to January 2008 under solar minimum. The analyses showed that both parameters contain quasi-harmonic oscillations with periods of T_n = 24/n hours (n = 1–7), among which the diurnal (n = 1) and semidiurnal (n = 2) ones are the strongest. Seasonal variations are explored of mean and median values, spectrum, amplitude, and phase of the diurnal and semidiurnal components of foF2 and hmF2.     

散乱点云自适应滤波算法

提出一种散乱点云自适应滤波算法,该算法采用改进的R*-树组织散乱点云的拓扑近邻关系,基于该结构快速准确获取局部型面参考数据,自适应调节二维高斯分布的数字特征计算滤波权值,计算局部型面参考数据对原始型面数据的影响因子,以此作为权值计算各点滤波后的坐标,采用加权平均方法实现散乱点云的自适应滤波.实验证明该算法可有效提高点云的滤波效率,在保留原始型面特征的基础上,减小点云的随机误差,提高光顺性.     

石墨烯/Fe3O4复合材料的制备及电磁波吸收性能

为扩展石墨烯的应用领域,对磁性功能化石墨烯的电磁波吸收性能进行研究.在氧化石墨与Fe3 O4粒子的悬浮液中添加还原剂水合肼,微波辐照反应制备石墨烯/Fe3 O4复合物.采用X射线衍射、透射电镜等手段对材料的结构和Fe3 O4的分布状态进行了测试表征.采用矢量网络分析仪测定了材料在0.1～18.0 GHz频率范围内的复介...     

Ka频段低轨遥感卫星可变编码调制应用效能研究

分辨率的不断提高对低轨遥感卫星的星地数据传输能力提升提出了迫切需求,导致X频段星地数传通道压力急剧增加,而Ka频段可用带宽是X频段的4倍,理论上可大幅提升传输能力。当前低轨遥感卫星的星地数据传输通常采用固定编码调制（CCM）和可变编码调制（VCM）,均未利用地面站仰角增大时大气衰减减小所带来的信道条件改善,对链路资源造成浪费。针对此问题,对指定地面站和链路可用度,综合考虑自由空间损耗和大气衰减随接收仰角增加而同时减小的特性,提出基于DVB S2标准的Ka频段星上VCM系统实现方案,给出传输效能评估标准,并对降雨特性不同的喀什站、北京站、三亚站CCM,VCM的Ka频段传输效能进行了对比仿真分析,以寻找出适合不同站点的星地数传方案。仿真结果表明：干旱少雨的喀什站更适合采用CCM,且链路可用度高达99.82%;雨量中等的北京站可根据用户使用需求灵活选择CCM或VCM;而降雨丰富的三亚站更适合采用VCM,不仅可将传输效能提升8.37%,还可将链路可用度提升11.23%。     

25t级氢氧膨胀循环发动机推力室氧腔流动仿真

为提高25 t级氢氧膨胀循环发动机推力室氧喷嘴出口流量均匀性,采用CFD方法对氧腔内流场进行了三维稳态数值仿真研究,分析了造成出口流量分布不均的原因,并据此设计了4种改进结构的氧腔,对每种结构进行了细节优化。通过数值仿真得到了不同方案氧腔内的流场分布以及喷嘴出口流量分布,对比分析了均流板和液氧入口结构对出口流量均匀性的...     

粉末烧结法制备Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料

采用粉末烧结法制备了Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料,研究了烧结温度对烧结体的显微结构、相组成、磁致伸缩、抗压强度等性能的影响.研究结果表明,600 ℃烧结时,烧结体中仍主要存在Al与GMM合金相,烧结获得较理想的相分布状态.随着烧结温度的增加,复合体中非GMM相越来越多,原始相减少.当1200 ℃烧结时,烧结体中主要存在杂相,已几乎没有GMM相.随着烧结温度的增加,复合材料的λs和抗压强度明显下降,烧结温度为600 ℃时,烧结体的λs和抗压强度最大,分别为405×10-6和61.71MPa.其不足是,复合材料仍呈现明显的脆性特征.     

Orbital steady motions of a system of two bodies with an elastic connection

Steady motions of a pair of mass points connected by a rigid rod were studied by Abrarova and Karapetyan [1], the motions of a pair of mass points connected by an elastic spring were considered by Burov and Stepanov [2]. The present article is devoted to the existence, stability and bifurcation of the steady motions for a system composed of two bodies connected by an elastic torsional spring. Each of these bodies is a massless bar with mass points at the ends. One supposes that these bars are elastically connected and the system moves in the plane of the orbit of its mass centre. The trivial steady motions are studied (the principal axes of inertia of the system are directed as the radius-vector of the centre of inertia and as the tangent to the orbit). The non-trivial steady motions (the principal axes of inertia of the system are not directed as the radius vector or as the tangent to the orbit and the bars are not orthogonal each other) are also studied. We expose the complete study of the stability and of the bifurcation diagrams.     

2A14铝合金返修焊技术

根据2A14铝合金的冶金特点，针对对接接头和锁底焊缝的不同要求，提出了相应的采用缺陷槽的补焊工艺。分析了焊接位置、补焊层数及两面补焊、预热和缓冷、补焊的收／起弧及长度、电源选择、环境控制、补焊顺序和方向，以及装配等因素的影响。由不同运载贮箱补焊的结果可知，该工艺措施有效，补焊质量较好，提高了补焊的一次合格率。     

A comparison of ionosonde measured foF2 and IRI-2016 predictions over China

A comparison of the ionospheric F-region critical frequency (foF2) between ionosonde measurements and IRI-2016 predictions is studied over China during the period from January 2008 to October 2016. Four stations are selected, and the latitude coverage starts at 49.4°N and ends at 23.2°N with a sequential latitude interval of about 10°, the corresponding geomagnetic latitudes are from 39.5°N to 13.2°N. The results show that the variability of the observed foF2 versus latitudes, seasons, local time and levels of solar activity could be well reproduced by IRI-2016. However, the daily lowest value of foF2 from the IRI-2016 prediction occurs earlier than that from the ionosonde. Around the sunrise, the IRI-2016 prediction shows a very sharp rise and grows much faster than the observed foF2 in every month. The foF2 difference between the two options (URSI and CCIR) in IRI-2016 increases as the F10.7 index decreases. During 2008–2009, the annual average deviations of URSI and CCIR range from ?5% to ?10% and from 5% to ?5%, respectively. Generally, the CCIR performs better than URSI during postsunset under low solar activity or in Equatorial Ionization Anomaly (EIA) region over China, while it shows no large difference in performance with URSI in other locations or for other time.