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21.
《中国航空学报》2020,33(10):2770-2781
In the machining process of aircraft monolithic parts, the initial residual stress redistribution and structural stiffness evolution often lead to unexpected distortions. On the other hand, the stress redistribution and stiffness reduction during the machining process depend on the material removal sequence. The essence of the stress redistribution is releasing the initial elastic strain energy. In the present study, the influence of the material removal sequence on the energy release is studied. Moreover, a novel optimization method is proposed for the material removal sequence. In order to evaluate the performance of the proposed method, the mechanism of the machining distortion is firstly analyzed based on the energy principle. Then a calculative model for the machining distortion of long beam parts is established accordingly. Moreover, an energy parameter related to the bending distortion and the procedure of the material removal sequence optimization is defined. Finally, the bending distortion analysis and material removal sequence optimization are performed on a long beam with a Z-shaped cross-section. Furthermore, simulation and experiments are carried out. The obtained results indicate that the optimized sequence results in a low distortion fluctuation and decreases the bending distortion. 相似文献
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用两颗GPS卫星确定低轨卫星轨道的初值方法 总被引:1,自引:1,他引:0
研究了用两颗全球定位系统(GPS)卫星粗略确定低轨卫星轨道的问题,并着重讨论了其中的初值问题,给出了一种有效的初值方法。实验结果证明:这种方法能给出一个确定的、实用的初值,大大减少了初轨计算的计算量,并使得算法收敛更加有保障。在工程实用方面比传统的猜测方法具有较大的优势。 相似文献
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论火工装置的抽样试验与可靠性评估问题 总被引:1,自引:0,他引:1
郭维长 《中国空间科学技术》1999,19(3):51-57
对航天器用的火工装置,提出运用序贯检验方法制定其抽样试验方案以及运用贝叶斯方法评定其可靠性的建议。算例表明,文章所提建议适用于解决小子样成败型产品的可靠性设计、试验和验证等问题,对节省产品研制经费有重要意义。 相似文献
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为了获得固体燃料超燃冲压发动机燃烧室初始型面和研究不同台阶高度下的初始型面的变化规律,将固体燃料燃面退移速率模型耦合到准一维流动方程中,发展了一种计算固体燃料超燃冲压发动机燃烧室性能的准一维数值计算方法。利用该方法,将燃空比和流场马赫数作为燃烧室性能的优化参数,得出了不同台阶高度下满足优化目标的燃烧室型面。根据所得的优化型面,归纳了型面参数随着台阶高度的变化规律。结果表明,随着台阶高度的增大,燃烧室的整体长度增大,等直段的长度增大,扩张段的扩张比减小,扩张段的长度减小。 相似文献
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Feasibility of performing space surveillance tasks with a proposed space-based optical architecture 总被引:1,自引:0,他引:1
T. Flohrer H. Krag H. Klinkrad T. Schildknecht 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Under ESA contract an industrial consortium including Aboa Space Research Oy (ASRO), the Astronomical Institute of the University of Bern (AIUB), and the Dutch National Aerospace Laboratory (NLR), proposed the observation concept, developed a suitable sensor architecture, and assessed the performance of a space-based optical (SBO) telescope in 2005. The goal of the SBO study was to analyse how the existing knowledge gap in the space debris population in the millimetre and centimetre regime may be closed by means of a passive optical instrument. The SBO instrument was requested to provide statistical information on the space debris population in terms of number of objects and size distribution. The SBO instrument was considered to be a cost-efficient with 20 cm aperture and 6° field-of-view and having flexible integration requirements. It should be possible to integrate the SBO instrument easily as a secondary payload on satellites launched into low-Earth orbits (LEO), or into geostationary orbit (GEO). Thus the selected mission concept only allowed for fix-mounted telescopes, and the pointing direction could be requested freely. Since 2007 ESA focuses space surveillance and tracking activities in the Space Situational Awareness (SSA) preparatory program. Ground-based radars and optical telescopes are studied for the build-up and maintenance of a catalogue of objects. In this paper we analyse how the proposed SBO architecture could contribute to the space surveillance tasks survey and tracking. We assume that the SBO instrumentation is placed into a circular sun-synchronous orbit at 800 km altitude. We discuss the observation conditions of objects at higher altitude, and select an orbit close to the terminator plane. A pointing of the sensor orthogonal to the orbital plane with optimal elevation slightly in positive direction (0° and +5°) is found optimal for accessing the entire GEO regime within one day, implying a very good coverage of controlled objects in GEO, too. Simulations using ESA’s Program for Radar and Optical Observation Forecasting (PROOF) in the version 2005 and a GEO reference population extracted from DISCOS revealed that the proposed pointing scenario provides low phase angles together with low angular velocities of the objects crossing the field-of-view. Radiometric simulations show that the optimal exposure time is 1–2 s, and that spherical objects in GEO with a diameter of below 1 m can be detected. The GEO population can be covered under proper illumination nearly completely, but seasonal drops of the coverage are possible. Subsequent observations of objects are on average at least every 1.5 days, not exceeding 3 days at maximum. A single observation arc spans 3° to 5° on average. Using a simulation environment that connects PROOF to AIUB’s program system CelMech we verify the consistency of the initial orbit determination for five selected test objects on subsequent days as a function of realistic astrometric noise levels. The initial orbit determination is possible. We define requirements for a correlator process essential for catalogue build-up and maintenance. Each single observation should provide an astrometric accuracy of at least 1”–1.5” so that the initially determined orbits are consistent within a few hundred kilometres for the semi-major axis, 0.01 for the eccentricity, and 0.1° for the inclination. 相似文献
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交会对接是空间站任务中一项非常重要的技术。基于C—W方程,推导了用直角坐标和轨道根数描述的远程导引段多冲量变轨段策略的方程,同时给出了求解方程组的迭代算法。随着冲量的施加,剩下的变轨量不足以瞄准交会时刻目标的全部状态时,给出了瞄准部分变量的方法。通过算例验证发现,存在定轨误差的情况下,部分变量瞄准法能精确地瞄准任务所关心的变量。 相似文献