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排序方式: 共有135条查询结果,搜索用时 15 毫秒
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针对激光标刻刀具编码时出现的标刻效率低、标刻质量不稳定、危害工人身体等问题,提出了一种自适应标刻技术.设计了特定结构的输送机和V型块,配合光电开关的检测功能实现自适应传送刀具;设计了使不同刀具在抓取后轴线处在同一位置的机械手爪,以保证不同刀具端面都能快速定位到激光头标刻区域;利用机械手的快速移动,采用了光电开关辅助对焦来提升对焦的速度和精度.在这3项关键技术支持下,完成了整个方案的设计.样机的测试结果表明,相比传统标刻方式,自适应标刻技术能将标刻效率提升4倍以上,保证标刻编码质量稳定可靠,实现无人化标刻. 相似文献
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薄壁管轴压胀形关键工艺参数及成形极限 总被引:4,自引:0,他引:4
利用粘性介质传压,对薄壁管轴压胀形进行了研究;基于塑性理论和分散性失稳理论,推导了轴对称胀形内压力分布规律,得出了内压加载区间和轴向加载关系;建立了基于载荷控制的加载函数,提出了送料控制方法,优化了加载模式;基于集中性失稳理论,计算了胀形压力极限,建立了均匀变形极限和极限应力比的概念,形成了零件可成形性的基本判据;分析了管材成形过程中应力变化特点,揭示了管材胀形区由拉-压应力状态迅速发展到双向受拉的机理.通过实验并利用有限元方法对薄壁管轴压胀形过程进行了模拟计算和研究,验证了理论分析结果. 相似文献
4.
采用热等静压技术及旋转电极粉,采用预合金粉粉末冶金工艺开展了粉末耐热钛合金TC11(Ti-6.5AJ-3.5Mo-1.5Zr-0.3Si)制备技术研究,研制出了全致密粉末TC11合金,通过热处理工艺研究优化粉末TC11材料的组织和性能.利用光学显微镜,对其组织进行了分析,用SEM观察了旋转电极粉末形貌,对室温及高温(550℃)拉伸性能及弹性模量等进行了测试分析.粉末TC11合金的组织和性能与同批次TC11锻棒材料进行了对比研究.利用特殊模具成形,开展了粉末TC11构件近净成形技术的研究,实现了整体大尺寸、带网格加强筋的薄壁粉末TC11合金航天飞行器舱体件近净成形,且未检测出内部缺陷.研究结果表明,粉末TC11合金具有与锻造材料相当的拉伸性能,而弹性模量更优,其金相组织均匀细致,形成了网篮组织,并有围绕其分布的等轴α.粉末TC11合金及合适的近净成形技术可在高性价比、高可靠性的轻质耐热航天飞行器构件制备中得到应用. 相似文献
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为了提高石墨材料的抗氧化性,在石墨表面制备SiC/Si-MoSi2抗氧化涂层.首先采用液硅渗透在石墨材料表面制备SiC内涂层,然后采用料浆刷涂法制备Si-MoSi2外层.详细研究了SiC内层厚度对所制备的SiC/Si-MoSi2涂层抗氧化性能的影响.结果表明,SiC内层厚度对涂层的氧化防护能力有很大影响;在本实验条件下,当SiC内层厚度为240μm左右时,所制备的涂层在1 400℃的高温下对碳基体具有长时间的氧化防护性能.并从微观结构上分析和解释SiC内层厚度对所制备涂层的抗氧化性能的影响. 相似文献
6.
This paper describes a novel approach to monitoring the condition of small permanent-magnet synchronous motors (PMSM) operating under thermal stress. The approach begins with the estimation of temperature-dependent motor parameters from measurements of line voltages and currents. The parameters are then used to derive estimates of motor temperatures. Next, the electrically estimated temperatures are combined with a surface measurement of motor temperature and a dynamic thermal model of the motor to yield an observer that is a Kalman filter. The temperatures estimated by the observer are used for failure prevention. Finally, by modifying the observer, it is tuned to use the geometric properties of its innovation for failure detection. The innovation, that is, the difference between the thermally and electrically estimated temperatures, is monitored and compared against appropriate thresholds to detect failures. Failure detection is demonstrated experimentally, and shown to be capable of distinguishing the conditions of normal operation, and operation with obstructed cooling 相似文献
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Kenneth R. Lang Robert F. Willson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(7):105-110
Very Large Array (V.L.A.) measurements at 20 cm wavelength map emission from coronal loops with second-of-arc angular resolution at time intervals as short as 3.3 seconds. The total intensity of the 20 cm emission describes the evolution and structure of the hot plasma that is detected by satellite X-ray observations of coronal loops. The circular polarization of the 20 cm emission describes the evolution, strength and structure of the coronal magnetic field. Preburst heating and magnetic changes that precede burst emission on time scales of between 1 and 30 minutes are discussed. Simultaneous 20 cm and soft X-ray observations indicate an electron temperature and electron density during preburst heating in a coronal loop that was also associated with twisting of the entire loop in space. We also discuss the successive triggering of bursts from adjacent coronal loops; highly polarized emission from the legs of loops with large intensity changes over a 32 MHz change in observing frequency; and apparent motions of hot plasma within coronal loops at velocities V > 2,000 kilometerspersecond. 相似文献
9.
Kenneth R. Lang Robert F. Willson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(11):91-100
We present observations of flaring active regions with the Very Large Array (V.L.A. at 6 cm and 20 cm wavelengths) and the Westerbork Synthesis Radio Telescope (W.S.R.T. at 6 cm wavelength). These are compared with photospheric magnetograms (Meudon) and with Hα and offband Hα photographs (Big Bear and Ottawa River Solar Observatories). The 6 cm radiation of these active regions marks the legs of dipolar loops which have their footpoints in lower-lying sunspots. The intense, million degree radiation at 6 cm lies above sunspot umbrae in coronal regions where the longitudinal magnetic field strength H? = 600 Gauss and the height above the sunspot umbrae h = 3.5±0.5 × 109 cm. Circularly polarized horseshoe structures at 6 cm ring the sunspot umbrae. The high degree of circular polarization (?c = 95%) of the horseshoes is attributed to gyroresonant emission above sunspot? penumbrae. The 20 cm radiation of these active regions exhibits looplike coronal structures which extend across regions of opposite magnetic polarity in the underlying photosphere. The 20 cm loops are the radio wavelength counterparts of the X-ray coronal loops. We infer semilengths L = 5 × 109 cm, maximum electron temperatures Te(max) = 3 × 106 K, emission measures ∫Ne2d = 1028 cm?5, and electron densities Ne = 109 cm?3 (or pressures p = 1 dyn cm?2) for the 20 cm bremsstrahlung. A total of eight solar bursts were observed at 6 cm or 20 cm wavelength with second-of-arc angular resolution. The regions of burst energy were all resolved with angular sizes between 5″ and 30″, brightness temperatures between 2 × 107 K and 2 × 108 K, and degrees of circular polarization between 10% and 90%. The impulsive phase of the radio bursts are located near the magnetic neutral lines of the active regions, and between the flaring Hα kernels which mark the footpoints of magnetic loops. In one case there was preburst heating in the coronal loop in which a burst occurred. Snapshot maps at 10 s intervals reveal interesting burst evolution including rapid changes of circular polarization and an impulsive burst which was physically separated from both the preburst radio emission and the gradual decay phase of the burst. 相似文献
10.
李朗 《长沙航空职业技术学院学报》2014,14(3):18-21
在技术发展、教育时空领域扩大、党和政府政策支持、师生媒介素养提升的条件下,大学生思想政治教育新媒体利用迎来了一系列的机遇。与此同时,也遭遇了以下挑战:信息风暴带来了大学生思想政治教育新媒体利用的难以分辨和选择;虚拟空间交往方式的异化产生了大学生思想政治教育新媒体利用的隐痛;依赖的强化造就了大学生思想政治教育新媒体利用过程中的控制和反控制;身心健康受影响,成为大学生思想政治教育新媒体利用的忧患。 相似文献