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981.
在燕尾榫连接接头的微动疲劳特性分析中,考虑接触表面质量,即摩擦系数的影响.给出了摩擦系数对接头应力水平、摩擦功和微动磨损参数之间的关系.分析表明:按照传统方法,将摩擦系数取为常数时所确定的裂纹萌生位置偏于危险,由于摩擦系数的变化,裂纹既可能在榫头上萌生,也可能在榫槽上萌生;摩擦系数对接头的切向应力和摩擦功等参数也有一定的影响. 相似文献
982.
文章首先论述了任务规划系统和战术飞行管理系统、航路规划系统的联系与区别,分析了无人作战飞机任务规划系统的特点及其体系结构,最后详细分析与研究了任务规划系统需要解决的核心技术——航路规划技术。 相似文献
983.
984.
985.
MHD-Arc-Ramjet联合循环发动机中电弧数目的增加会改变发动机的循环结构,影响发动机的性能。理论上分析了MHD-Arc-Ramjet联合循环发动机中电弧数目的增加对发动机单位推力的影响,讨论了电弧数目趋于无穷大时的发动机性能,定量给出了不同电弧数目下的发动机单位推力。结果表明,MHD-Arc-Ramjet联合循环发动机的单位推力随着电弧数目的增加而增加;当电弧数目趋于无穷大时,发动机单位推力存在最大值;增加电弧数目所获得的发动机单位推力的增益随着电弧数目的增加而不断减缓。 相似文献
986.
采用等离子喷涂工艺在GH4099合金基体上制备了热障涂层,并进行了1050℃恒温氧化试验,综合利用X射线衍射仪、扫描电子显微镜、能谱分析仪等检测手段,分析了涂层的显微结构及高温氧化行为。结果表明:等离子喷涂(APS)热障涂层在高温氧化过程中,黏结层被氧化生成热生长氧化物(TGO)。但长时间氧化后,在与TGO毗邻的金属黏结层中产生了范围较窄但浓度变化较大的贫Al带,TGO层出现保护性Al2O3向非保护性混合氧化物转变的现象,导致致密Al2O3层的连续性被破坏,TGO厚度快速增加。 相似文献
987.
This article introduces a computer numerical control (CNC)-based open hardware architecture system to realize the special functions of automated tape-laying (ATL) in a numerical control system. It associates a programmable multi-axis controller (PMAC) as the motion control unit with programmable numerical controllers (PCL-725, PCL-730) for on-off control. To bring about synchronized movements of the main 5-axis tape-laying head system and the 3-axis ultrasonic tape-cutting sub-system, the tracking-control method associated with time-based mode attributed to PMAC is applied in different cases. In addition, with the goal of realizing real-time tasks in the software system such as synchronizing motion control and on-off control, the real-time Win 2000 system is adopted. As a device driver for PMAC and PCL, a user graphical interface and a numerical control program interpretation module are also designed. This system is helpful to solve complicated problems in designing numerical controls for ATL such as ensuring high requirements for precise machine control and synchronization of motion control and on-off control. 相似文献
988.
The THEMIS Fluxgate Magnetometer 总被引:2,自引:0,他引:2
H. U. Auster K. H. Glassmeier W. Magnes O. Aydogar W. Baumjohann D. Constantinescu D. Fischer K. H. Fornacon E. Georgescu P. Harvey O. Hillenmaier R. Kroth M. Ludlam Y. Narita R. Nakamura K. Okrafka F. Plaschke I. Richter H. Schwarzl B. Stoll A. Valavanoglou M. Wiedemann 《Space Science Reviews》2008,141(1-4):235-264
989.
R. P. Lepping M. H. Acũna L. F. Burlaga W. M. Farrell J. A. Slavin K. H. Schatten F. Mariani N. F. Ness F. M. Neubauer Y. C. Whang J. B. Byrnes R. S. Kennon P. V. Panetta J. Scheifele E. M. Worley 《Space Science Reviews》1995,71(1-4):207-229
The magnetic field experiment on WIND will provide data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the mission, and, where appropriate, relate them to the statics and dynamics of the magnetosphere. The basic instrument of the Magnetic Field Investigation (MFI) is a boom-mounted dual triaxial fluxgate magnetometer and associated electronics. The dual configuration provides redundancy and also permits accurate removal of the dipolar portion of the spacecraft magnetic field. The instrument provides (1) near real-time data at nominally one vector per 92 s as key parameter data for broad dissemination, (2) rapid data at 10.9 vectors s–1 for standard analysis, and (3) occasionally, snapshot (SS) memory data and Fast Fourier Transform data (FFT), both based on 44 vectors s–1. These measurements will be precise (0.025%), accurate, ultra-sensitive (0.008 nT/step quantization), and where the sensor noise level is <0.006 nT r.m.s. for 0–10 Hz. The digital processing unit utilizes a 12-bit microprocessor controlled analogue-to-digital converter. The instrument features a very wide dynamic range of measurement capability, from ±4 nT up to ±65 536 nT per axis in eight discrete ranges. (The upper range permits complete testing in the Earth's field.) In the FTT mode power spectral density elements are transmitted to the ground as fast as once every 23 s (high rate), and 2.7 min of SS memory time series data, triggered automatically by pre-set command, requires typically about 5.1 hours for transmission. Standard data products are expected to be the following vector field averages: 0.0227-s (detail data from SS), 0.092 s (detail in standard mode), 3 s, 1 min, and 1 hour, in both GSE and GSM coordinates, as well as the FFT spectral elements. As has been our team's tradition, high instrument reliability is obtained by the use of fully redundant systems and extremely conservative designs. We plan studies of the solar wind: (1) as a collisionless plasma laboratory, at all time scales, macro, meso and micro, but concentrating on the kinetic scale, the highest time resolution of the instrument (=0.022 s), (2) as a consequence of solar energy and mass output, (3) as an external source of plasma that can couple mass, momentum, and energy to the Earth's magnetosphere, and (4) as it is modified as a consequence of its imbedded field interacting with the moon. Since the GEOTAIL Inboard Magnetometer (GIM), which is similar to the MFI instrument, was developed by members of our team, we provide a brief discussion of GIM related science objectives, along with MFI related science goals. 相似文献
990.
介绍了某联合动力装置中的共底和环形点火器首次采用新研制的3500K高温涂料进行热防护的配方设计、受热计算、涂层制备和试验考核。由环氧改性有机硅树脂基料、专用树脂固体体系和多种形状的硅酸盐填料制成的涂层具有优异的耐高温、隔热和抗烧蚀性能,还能常温固化成形,成功地解决了中型固体火箭发动机中大尺寸、薄壁、复杂型面零件的热防护和过烧蚀难题,有效地提高了发动机的工作可靠性。 相似文献