焊接工艺方法对6061-T6铝合金焊接接头疲劳性能的影响

通过对6061铝合金MIG焊接头和TIG焊接头在对应的加载应力条件下疲劳寿命的测定,对比分析了两种工艺方法对铝合金焊接接头疲劳性能的影响。结果表明,在加载应力低于焊接接头静载力学性能的90%时,焊接接头的疲劳寿命均能满足需求背景的需要(100000次不破坏)。同样载荷条件下,MIG焊接头的疲劳性能优于TIG焊接头,尤其是在高应力条件下,MIG焊接头的优势更为明显。焊接接头显微组织分析表明,MIG焊接头比TIG焊接头具有更为细小的晶粒和焊接热影响区,有效地提高了接头的滑移形变抗力,抑制了循环滑移带的形成和开裂,从而提高接头的疲劳性能。疲劳断口分析显示,试件的表面缺陷(疏松、气孔、夹杂等)及机械损伤是疲劳裂纹主要的策源地。     

作动器输出机构刚度优化设计与仿真分析

作动器输出机构的变形可以看作是输出轴体扭转变形与摇臂变截面悬臂梁变形的综合。从材料力学的角度出发,详细推导了作动器输出机构机械刚度的理论计算方法,并以此理论为依据对作动器输出机构的结构进行优化设计。通过仿真对比确定优化设计的正确性,为工程应用提供了有力的理论支撑。     

深空探测器大口径天线指向在轨标定方案

基于深空探测器配备的大口径天线的指向精度要求,给出了一种深空探测器大口径天线在轨指向的标定方案,以解决深空探测器安装的大口径天线的在轨指向评价问题。通过对飞行器特点和约束条件的分析,结合"嫦娥4号"中继星天线的具体情况,采用星地协同工作的方法,给出了天线指向在轨标定的方案,并明确了标定的实施流程,最后对标定过程中的误差情况进行了分析。本方案可推广应用于其他深空探测器大口径天线指向标定方案的设计。     

太空环境下电子束原位制造技术

美国国家航空航天局（NASA）载人探索计划的提出给载人登月和载人火星等带来了机会和风险,NASA的工程师和科学家正在开展在月球或火星表面利用当地提炼的材料进行原位制造工艺技术的研究。首先,介绍了太空原位制造和修复（ISFR）技术的概念和特点,结合该技术的发展背景,介绍了电子束原位制造技术的概念、特点以及在太空环境下应用的优势和潜力。然后,根据所用原材料和成形工艺原理的不同,电子束原位制造技术又分为电子束熔融（EBM）和电子束自由成形制造（EBF³）技术两个分支,分别介绍了这两个分支技术的概念、原理、特点以及采用该技术研制出的零件的性能,结合硬件设备的情况介绍了在太空环境下应用的适用性,同时也详细介绍了NASA利用兰利研究中心的C-9抛物线飞行试验系统进行电子束原位制造微重力试验的研究成果、试验数据和未来的发展趋势。最后,结合中国未来空间事业发展的需要,提出了关于发展太空环境下电子束原位制造技术的设想与建议。     

民用航空发动机TA19电子束焊疲劳试验

针对民用航空发动机钛合金整体叶盘常用材料TA19开展其母材试件与电子束焊焊接试件在20,300,450℃的疲劳试验,通过焊接试件的焊缝材料断口与母材断口形貌的比较探讨了焊缝材料的疲劳破坏机理,并在104~106循环的疲劳寿命区间内采用Basquin模型分别建立了焊缝材料和母材的应力-疲劳寿命(S-N)曲线,结果显示母材试件与焊接试件的试验疲劳寿命大部分都落在了对应模型计算疲劳寿命的2倍线之内,表明试验得到的S-N曲线是合理的.焊接试件与母材试件的S-N曲线的对比分析表明,20℃时焊接试件的疲劳性能比母材试件略高,而在300℃和450℃时焊接试件与母材试件的疲劳性能差异随应力水平发生变化.但总地说来,在所关注疲劳寿命区间内,母材试件与焊接试件的计算疲劳寿命差异也在2倍线以内,初步表明两者的疲劳性能相当.      

梁纵向与横向耦合非线性振动分析

纵向振动和横向振动耦合是捆绑火箭等结构中的典型振动现象.以Rayleigh梁为研究对象,通过Hamilton变分原理推导了考虑应变二次项的纵向振动与横向振动耦合控制方程,并用有限元方法对该非线性系统的行为进行了模拟.针对线性系统固有振动频率和非线性纵横耦合动态响应情况,把所得结果与NASTRAN结果进行了比较,二者结果吻合,证明了本方法的正确性.在此基础上,借助振动控制方程和模拟结果,讨论了非线性系统频率与模态的时变特性,非线性动态响应频率成分特性,横向振动和纵向振动相互影响以及共振现象等.研究结果为本方法的实际应用提供了理论基础.      

Assessment of precision in ionospheric electron density profiles retrieved by GPS radio occultations

The Constellation Observing System for Meteorology Ionosphere and Climate (COSMIC) is a six satellite radio occultation mission that was launched in April 2006. The close proximity of these satellites during some months after launch provides a unique opportunity to evaluate the precision of Global Positioning System (GPS) radio occultation (RO) retrievals of ionospheric electron density from nearly collocated and simultaneous observations. RO data from 30 consecutive days during July and August 2006 are divided into ten groups in terms of daytime or nighttime and latitude. In all cases, the best precision values (about 1%) are found at the F peak height and they slightly degrade upwards. For all daytime groups, it is seen that electron density profiles above about 120 km height exhibit a substantial improvement in precision. Nighttime groups are rather diverse: in particular, the precision becomes better than 10% above different levels between 120 and 200 km height. Our overall results show that up to 100–200 km (depending on each group), the uncertainty associated with the precision is in the order of the measured electron density values. Even worse, the retrieved values tend sometimes to be negative. Although we cannot rely directly on electron density values at these altitudes, the shape of the profiles could be indicative of some ionospheric features (e.g. waves and sporadic E layers). Above 200 km, the profiles of precision are qualitatively quite independent from daytime or latitude. From all the nearly collocated pairs studied, only 49 exhibited a difference between line of sight angles of both RO at the F peak height larger than 10°. After analyzing them we find no clear indications of a significant representativeness error in electron density profiles due to the spherical assumption above 120 km height. Differences in precision between setting and rising GPS RO may be attributed to the modification of the processing algorithms applied to rising cases during the initial period of the COSMIC mission.     

Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm

The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere.     

150kV/30kW逆变式电子束焊接高压电源设计

针对150kV/30kW电子束焊接高压电源高电压、大功率输出的要求,低压电路采用IGBT (Insulated Gate Bipolar Transistor)逆变隔离直流电源与逆变全桥串联的主电路拓扑,高压电路由3组升压变压器与10倍压整流电路的串联结构并联组成;设计了高压采样电路、束流采样电路,以及双闭环控制电路.基于上述技术,实现了150kV/30kW高电压大功率输出.实验结果表明高压加速电源的输出线性度和束流输出线性度较好,同时高压稳定度和束流稳定度均在0.5%左右,能够满足电子束焊接的要求.     

铰链对含铰结构非线性动力学特性影响分析

针对可展结构中铰链带来的展开后非线性动力学问题,建立了含铰结构的动力学模型。基于铰链侧向和径向的几何约束关系,分析了不同约束条件下的铰链非线性特性。基于谐波平衡法（HBM）,对含铰结构的非线性变量进行一次谐波展开,得到铰链非线性力的谐波展开表达式,将含铰可展结构的非线性动力学方程转化为代数方程。分析了铰链在不同非线性特性下各参数对结构动态特性的影响,得到结构固有频率随铰链间隙、刚度和激振力的变化规律。考虑铰链的非线性特性,通过固有频率脊线求解,得到结构固有频率极值随铰链数量、位置和刚度的变化曲面,并对其进行非线性拟合,得到铰链参数对结构固有频率的影响函数,其计算方法和结果在多维复杂结构中具有一定的扩展性,为可展结构的设计和研究提供参考。利用龙格库塔法对非线性结构进行数值仿真,得到结构的固有频率变化曲线,仿真结果表明了利用HBM进行含铰结构动力学分析的正确性。