钛合金螺旋铣孔孔径偏差研究

螺旋铣孔是航空航天领域新出现的制孔技术,其切削过程中会产生径向切削力,从而引起刀具变形并造成孔径偏差。针对该问题开展了钛合金螺旋铣孔孔径偏差试验,分析了包括进给方向在内的不同加工参数对孔径偏差的影响规律;基于螺旋铣孔运动学原理对不同进给方向下的材料去除过程和径向切削力方向进行了研究,分析了不同进给方向下的孔径偏差变化规律及形成原因,并设计切削力试验进行了验证;通过分析不同加工参数下的未变形切屑形状及径向切削力变化情况,研究了各加工参数对孔径变化趋势的影响规律。研究结果表明,当进给方向为顺时针时,刀具受背离孔心的径向切削力的作用向孔径外侧发生挠曲变形,导致所加工孔径大于理论孔径;当进给方向为逆时针时则相反。进给速度和导程的增加将加剧孔径偏差,切削速度的增加则会减弱孔径偏差。     

沟槽织构球头铣刀刀具结构强度仿真研究

为研究横向沟槽微织构的制备对刀具应力和应变的影响,采用有限元仿真方法,针对横向沟槽微织构形式,进行了刀具结构强度的仿真。同时,研究了不同横向沟槽微织构参数对球头铣刀结构强度的影响规律。     

Dark Matter Particle Explorer:The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

The Dark Matter Particle Explorer (DAMPE) mission is one of the five scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Science (CAS) approved in 2011. The main scientific objective of DAMPE is to detect electrons and photons in the range of 5GeV-10TeV with unprecedented energy resolution (1.5% at 100GeV) in order to identify possible Dark Matter (DM) signatures. It will also measure the flux of nuclei up to above 500TeV with excellent energy resolution (40% at 800GeV), which will bring new insights to the origin and propagation high energy cosmic rays. With its excellent photon detection capability, the DAMPE mission is well placed for new discoveries in high energy-ray astronomy as well.      

运载火箭组装与测试远程协同信息平台技术

为适应未来高频度发射任务需求,在借鉴国内外远程协同及信息应用技术基础上,以中国运载火箭组装、测试及发射任务为背景,通过对功能需求和技术难点分析,设计了运载火箭组装与测试远程协同应用系统,对关键技术进行了分析和论述,为运载火箭远程测试、协同决策发射提供有效技术解决途径。     

Approach to Interference Riveting Process Control of Aircraft Automatic Drilling and Riveting

Interference fit riveting is an effective way to improve the fatigue life of aircraft.The accurate control of riveting interference of aircraft automatic drilling and riveting equipment is achieved by process parameters including upsetting force and upset head height.It is valuable for aircraft manufacturing engineering.An approach to interference riveting process control based on the analysis of interference riveting stress field is proposed.According to assembly structure,the upsetting force is calculated by the material property and interference fit level,and the upset head height is deduced by the upsetting force.The experimental result shows that the interference fit level can be controlled accurately by the upsetting force and upset head height,and then,the quality of aircraft automatic riveting can be improved.The proposed approach is verified by the good match between the predicted result and the experimental result.     

CFRP曲面铣削力及加工缺陷研究

碳纤维增强复合材料(Carbon fiber reinforced polymer,CFRP)曲面结构不断变化的工件倾角使得在加工过程中易产生分层、毛刺等缺陷。为研究工件倾角对CFRP曲面结构可加工性的影响规律,采用金刚石涂层铣刀对不同倾角下CFRP叠层平板结构进行顺铣加工试验,对不同坐标系下的铣削力和加工侧面、表面缺陷进行了研究。研究结果表明,随工件倾角的增大,水平方向上每齿所切材料平均厚度与截面积均减小,等效轴向切深逐渐增大,但是每齿去除材料体积保持不变。机床坐标系下的铣削力几乎不随工件倾角的变化而变化。而在工件坐标系下,铣削力沿工件厚度方向逐渐增大,沿工件长度方向逐渐减小。同时随着工件倾角的增大,侧面表层分层缺陷不断加重,纤维束发生弯曲,裂纹沿纤维方向逐渐扩展至表层内部,加工表面遭受破坏铺层数量也同样增加。     

Theoretical and Experimental Analysis on Influence of Revolution Radius in Orbital Drilling

Revolution radius is one of the significant parameters in orbital drilling,which has great influence on many factors,such as the cutting area of front and side cutting edge,undeformed chip geometry,delamination and burr at hole exit side,hole surface roughness,cutting tool force and deflection,chip removal and heat transmission.First,the influence of revolution radius on the factors is discussed theoretically in detail.Analysis results show that big revolution radius can reduce axial cutting force,restrain exit delamination and burr,and improve chip removal and heat transmission.Then,single factor test and orthogonal test are utilized in the two processing methods as machining unidiameter holes with several cutting tools and machining different diameter holes with one tool.Finally,the influence of revolution radius on cutting force and hole machining precision is studied.These results provide a profound foundation for future optimization of cutting control parameters.     

A simplified approach to uncertainty quantification for orbits in impulsive deflection scenarios

For the majority of near-Earth Asteroid (NEA) impact scenarios, optimal deflection strategies use a massive impactor or a nuclear explosive, either of which produce an impulsive change to the orbit of the object. However, uncertainties regarding the object composition and the efficiency of the deflection event lead to a non-negligible uncertainty in the deflection delta-velocity. Propagating this uncertainty through the resulting orbit will create a positional uncertainty envelope at the original impact epoch. We calculate a simplified analytic evolution for impulsively deflected NEAs and perform a full propagation of uncertainties that is nonlinear in the deflection delta-velocity vector. This provides an understanding of both the optimal deflection velocities needed for a given scenario, as well as the resulting positional uncertainty and corresponding residual impact probability. Confidence of a successful deflection attempt as a function of launch opportunities is also discussed for a specific case.     

Equatorial Ionospheric Anomaly (EIA) and comparison with IRI model during descending phase of solar activity (2005–2009)

The ionospheric variability at equatorial and low latitude region is known to be extreme as compared to mid latitude region. In this study the ionospheric total electron content (TEC), is derived by analyzing dual frequency Global Positioning System (GPS) data recorded at two stations separated by 325 km near the Indian equatorial anomaly region, Varanasi (Geog latitude 25°, 16^/ N, longitude 82°, 59^/ E, Geomagnetic latitude 16°, 08^/ N) and Kanpur (Geog latitude 26°, 18^/ N, longitude 80°, 12^/ E, Geomagnetic latitude 17°, 18^/ N). Specifically, we studied monthly, seasonal and annual variations as well as solar and geomagnetic effects on the equatorial ionospheric anomaly (EIA) during the descending phase of solar activity from 2005 to 2009. It is found that the maximum TEC (EIA) near equatorial anomaly crest yield their maximum values during the equinox months and their minimum values during the summer. Using monthly averaged peak magnitude of TEC, a clear semi-annual variation is seen with two maxima occurring in both spring and autumn. Results also showed the presence of winter anomaly or seasonal anomaly in the EIA crest throughout the period 2005–2009 only except during the deep solar minimum year 2007–2008. The correlation analysis indicate that the variation of EIA crest is more affected by solar activity compared to geomagnetic activity with maximum dependence on the solar EUV flux, which is attributed to direct link of EUV flux on the formation of ionosphere and main agent of the ionization. The statistical mean occurrence of EIA crest in TEC during the year from 2005 to 2009 is found to around 12:54 LT hour and at 21.12° N geographic latitude. The crest of EIA shifts towards lower latitudes and the rate of shift of the crest latitude during this period is found to be 0.87° N/per year. The comparison between IRI models with observation during this period has been made and comparison is poor with increasing solar activity with maximum difference during the year 2005.     

航天器测控资源调度模型及算法

航天器测控资源调度问题研究的目的是通过一定的调度方法科学地分配有限的地面测控资源和最大化地完成航天器测控任务。在参考面向任务执行计划的航天器测控资源调度模型研究的基础上,文章提出了面向可见窗口的航天器测控调度模型,并给出了问题的确定性分支定界求解算法及其计算复杂度分析。最后,通过仿真计算验证了算法的有效性和实用性。