First estimations of the aerosol optical thickness using Langley Method at Southern Brazil (29.4°S, 53.8°W)

The first estimations of the aerosol optical thickness (AOT) using Langley Method at Southern Space Observatory (SSO) at Southern Brazil (29.4°S, 53.8°W) are presented. In addition to ozone and sulphur dioxide columns, AOT can be obtained using Brewer Spectrophotometer at specific wavelengths: 306.3, 310.1, 313.5, 316.8 and 320.1 nm. The AOT was obtained for the period from November/2002 to May/2003. Very low AOT averages were obtained, whose values were about 0.21 ± 0.03 at 306.3 nm, 0.21 ± 0.02 at 310.1 nm, 0.19 ± 0.02 at 313.5 nm, 0.20 ± 0.02 at 316.8 nm and 0.20 ± 0.02 at 320.0 nm for all period analysed. Different behaviour of AOT were obtained at two daily specific periods of aerosol accumulation, one in the afternoons from November/2002 to February/2003, caused mainly by a mild biomass burning season’s in the region and other in the mornings from March to May/2003, due the high relative humidity presented in the region studied.     

Tidal associated temperature disturbances observed at the middle atmosphere (30–65 km) by a Rayleigh lidar at 23°S

A lidar has been operated in São José dos Campos, Brazil (23.2°S, 45.8°W) since 1972, mainly dedicated to the study of mesospheric sodium at the 589 nm resonant line. The molecular Rayleigh scattering can also be used provided we limit the height to ∼75 km where the sodium scattering begins. Nevertheless, the weak signal obtained only permits the determination of density and temperature profiles by accumulating a large number of shots giving only nocturnal average profiles. Temporal variations in density and temperature on the scale of hours can however, be obtained by performing a superposed epoch analysis for a given time interval and covering a period of several days. In this way we obtained hourly mean profiles grouped by months, seasons and overall, with data acquired from 1993 to 2004. The difference between the hourly temperatures and the nocturnal means shows for some months, with enough data coverage, downward propagating structures that apparently have tidal origin. The seasonal averages show a recurrent feature with high temperatures before and low temperatures after midnight above 50 km. Some similarity is found with the GSWM model, but the observed temperature amplitudes are twice of that for the model.     

半球轴承批量检测夹具的设计及应用

三坐标测量机是快速自动测量设备,其装夹工件环节产生的准备时间对测量效率的影响远比手动量仪大.因此在批量轮番生产方式下采取有效措施,缩短测量准备时间,对提高产品检测效率具有重要意义.针对动压马达半球轴承成批轮番生产检测的任务特点,在分析检测流程、零件结构以及测量机工作特点的基础上,设计了由孔系基础板及专用定位、支承、紧固件组成的半球轴承批量检测夹具,实现了工件离线快速装夹、缩短了测量准备时间.通过实际应用证明了此方法的有效性.     

Seasonal variations of GPS derived TEC at three different latitudes of the southern hemisphere during geomagnetic storms

Data from the archive of the International GNSS Services (IGS) were used to study the seasonal variations of Total Electron Content (TEC) over three stations located at different latitudes in the southern hemisphere during the geomagnetic storms of 11 January, 6 April, 8 June, and 13 October 2000, representing storms that occurred in summer, autumn equinox, winter and spring equinox, respectively. The percentage TEC deviation with respect to reference values differs substantially from season to season. A strong seasonal anomaly and clear equinoctial asymmetry in TEC response to the storms were observed. Weak and short-lived positive TEC deviations as well as strong and long-lasting negative trends were observed in summer storm during the main and recovery phases respectively over the high and low latitudes whereas in winter storm, the highest positive TEC deviations was recorded during the main phase over the entire latitudes. TEC enhancement dominated all the stations during the autumn (March) equinox storm while TEC depletion was majorly observed during the spring (September) equinox. All these variations find their explanations in the thermospheric composition change and circulation. Future work with direct or modeled measurement of atomic Oxygen to molecular Nitrogen ratio (O/N₂), large number of storms and other possible factors such as variations in storm’s intensity and local time dependence of the storm onset is expected to validate the observations in this study.     

闭合等角转位法的测量精确度

闭合等角转位法广泛地应用于传感器旋转式圆度测量仪、工作台旋转式圆度测量仪或精密轴系的径向、轴向及其综合误差的测量。对闭合等角转位法的测量精确度做了详细的理论分析和实验验证,并提出了正确确定其采样点数的方法。     

谐振陀螺及半球壳谐振子陀螺仪

阐述了一种无需高速转子和轴承支承的陀螺仪——谐振陀螺的发展过程。文中特别对近年来在战略武器研制中广受注意的新型半球壳谐振子陀螺仪(HRG)作了评价性的论述,并作为展开后续研究的开端。     

微半球陀螺敏感结构热成型规律研究

针对近年来受到广泛关注的微半球热成型工艺,研究了表面张力、黏性力、惯性力、重力及压差对成型的影响,得出了黏性力在成型过程中起主导作用,表面张力、惯性力及重力对成型的影响可以忽略,压差的变化不影响成型的形状,只影响成型的速度的结论,并通过仿真及实验验证了该结论。     

C/SiC复合材料热辐射性能研究

利用稳态量热计法和傅里叶红外光谱仪分别测定了C/SiC复合材料在90℃时的半球向总发射率和室温法向光谱反射率.研究了纤维预制体编织方式、涂层厚度及表面形貌对C/SiC复合材料热辐射性能的影响.结果表明,3D C/SiC复合材料的热辐射性能优于2D C/SiC.2D C/SiC的总发射率为0.78,3D C/SiC达到0.82;SiC涂层厚度对C/SiC复合材料的热辐射性能影响很大,随着SiC涂层厚度的增加,C/SiC总发射率先降低后上升,最高值可达0.85;表面抛光后C/SiC复合材料热辐射性能有所下降,2D和3D C/SiC总发射率分别为0.74和0.75.     

面向Micro-PNT系统的微陀螺敏感结构参数化有限元仿真研究

针对Micro-PNT系统中多环和微半球陀螺敏感结构在设计阶段三维实体仿真分析存在的模型复杂、网格特征较难匹配结构特征、模型复用性较低等问题,提出一种基于低维单元简化建模,并通过实常数和截面定义等方式对特征结构进行全参数化表征的分析方法。通过对比,在相当的分析精度下,参数化分析中所需的节点数量仅为三维实体仿真的2%和43%,仿真效率提高显著,可加快陀螺设计收敛进程,支撑Micro-PNT技术发展。     

半球动压马达转子端面垂直度检测装置

在半球动压马达转子端面垂直度的工序中,检测一直是影响生产效率的重要瓶颈问题,因没有理想的检测手段,目前只能依赖三坐标仪进行检测.因检测频繁、测点多、耗时长,极大地影响了生产效率.介绍了一种基于光学检测原理研制的端面垂直度检测装置,工程实际应用结果表明,它具有检测精度高、操作简便、时间短的特点,极大地提高了检测效率,在提高生产效率方面具有重大的实际意义.