复合材料界面裂纹尖端应变能释放率及模态混合度计算

为了准确预测复合材料层合板分层扩展及疲劳损伤,应用改进的虚裂纹闭合技术计算复合材料分层尖端处应变能释放率及模态混合度.首先介绍了改进的虚裂纹闭合技术,然后将其应用到重合网格法中,求得了分层尖端处总应变能释放率,并提取了各模态下的应变能释放率分量.最后利用某界面裂纹模型验证了该方法计算应变能释放率、模态混合度及提取应变能释放率分量的有效性.     

裂纹间距及铺层角度对复合材料分层的影响

分层问题是复合材料层合板最常见问题,据统计约60%的层合板失效都与分层相关.通过基于虚裂纹闭合技术(VCCT)的重合网格法(S-FEM),分析了不同铺层角度及裂纹间距对应变能释放率的影响.由分析结果可看出,应变能释放率随铺层角度增加而减小;在裂纹尖端距离相对较小时,距离对能量释放率的影响要远大于锗层角度变化的影响.     

用于未来月球探测的ILOM 技术现状

使用面包板模型和仿真方法,在实验室内研究月球指向就位测量望远镜(ILOM)的基本特征,如望远镜星像中心点位置精度、温度效应、倾斜以及地面震动的影响。使用这个技术预期在月球表面观测月球自转时可以达到1ms的精度。将在地面上开展测试验证观测以全面评价达到优于0.1″观测精度目标所需条件和特征。     

复合材料加筋层合板结构分层扩展分析

采用基于模式混合度的分层扩展准则,研究了复合材料加筋层合板结构分层扩展力学行为,分析了铺层方式对复合材料层合板结构界面力学性能的影响。首先,由计算所得分层前缘处的应变能释放率分量计算求得模式混合度;然后,将其代入材料断裂韧性函数及分层扩展量计算公式,进而预测复合材料加筋层合板结构的分层起始及其扩展行为。并通过对规则对称正交铺层、反对称铺层与用于V-22飞行器结构中的铺层方式下的层合板分层扩展行为进行比较,验证了该方法的有效性。     

Overview of Differential VLBI Observations of Lunar Orbiters in SELENE (Kaguya) for Precise Orbit Determination and Lunar Gravity Field Study

The Japanese lunar explorer SELENE (Kaguya), which was launched on September 14th, 2007, was the target of VLBI observations over the period November 2007 to June 2009. These observations were made in order to improve the lunar gravity field model, in particular the lower degree coefficients and the model near the limb. Differential VLBI Radio sources, called VRAD instruments, were on-board the subsatellites, Rstar (Okina) and Vstar (Ouna), and the radio signals were observed by the Japanese VERA (VLBI Exploration of Radio Astrometry) network, and an international VLBI network. Multi-frequency and same-beam VLBI techniques were utilized and were essential aspects of the successful observing program. Multi-frequency VLBI was employed in order to improve the accuracy of the orbit determination obtained from the phase delay from the narrow-band satellite signals, while the same-beam VLBI method was used to resolve the cycle ambiguity which is inherent in the multi-frequency VLBI method. The observations were made at three S-band frequencies (2212, 2218 and 2287 MHz), and one X-band frequency (8456 MHz). We have succeeded in correlating the recorded signals from Okina/Ouna, and we obtained phase delays with an accuracy of several pico-seconds at S-band.