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1.
简述了冷硬树脂砂型在某些情况下的产生开裂的原因及机理,讨论了几种解决的方法,有利于改进产品质量,减少双方的经济损失。 相似文献
2.
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
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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
6.
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
7.
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
8.
在移除二进制偏移载波(Binary Offset Carrier,BOC)信号跟踪模糊的同时,为了保持BOC信号高的码跟踪精度,提出基于加权鉴别函数(Weighted Discriminator Function,WDF)的BOC信号无模糊跟踪方法。WDF使用非相干超前减滞后功率(Noncoherent Early Minus Late Power,NELP)鉴别器和子载波相位消除(Sub Carrier Phase Cancellation technique,SCPC)鉴别器,生成无误锁点的鉴别函数实现BOC信号跟踪。针对BOC(10,5)信号,仿真结果表明,相比于SCPC、基于伪相关函数的无模糊延迟锁定环(Pseudo correlation function based Unambiguous Delay Lock Loop,PUDLL)方法和对称脉冲模糊移除(Symmetrical Pulse Ambiguity Removing,SPAR)方法,所提WDF方法在码跟踪误差方面分别改善了2.5dB、5.5dB与8.3dB,多径误差分别降为60.4%、32.8%与38.0%。因此,WDF是一种有效的、高性能的BOC信号无模糊跟踪方法。 相似文献
9.
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
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