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991.
采用大涡模拟LES方法计算了火箭发动机超声速过膨胀射流形态及近场声压分布,研究了入口温度与环境温度的比值(温度比)对声场的影响;将声源分解,基于Ffowcs Williams-Hawkings (FW-H)方程获取了不同位置噪声源的远场噪声,并根据声压级频谱和湍流形态分析了超声速射流噪声的产生机理。研究表明,超声速过膨胀射流气动噪声由湍流混合噪声和宽频激波噪声组成,近场噪声源以马赫波形式向大方位角辐射中高频噪声,下游大尺度湍流向低方位角范围辐射低频噪声,声压级峰值频率随观测角度增大而升高;随温度比升高,马赫波辐射角度增大,噪声指向性发生改变。该研究可为运载火箭发动机地面试车或火箭发射段声学环境设计提供参考。 相似文献
992.
V. V. Kalegaev W. O. Barinova I. N. Myagkova V. E. Eremeev D. A. Parunakyan M. D. Nguyen O. G. Barinov 《Cosmic Research》2018,56(1):32-37
An empirical model of the high-latitude boundary of the outer Earth’s radiation belt (ERB) has been presented, which is based on the measurement data of electron fluxes on the polar low-orbit CORONAS-Photon, Meteor-M1, and Meteor-M2 satellites. The boundary was determined by a sharp decrease to the background level of the flux of trapped electrons with energies of 100 or 200 keV in the polar part of the profile of the outer radiation belt. A numerical algorithm has been implemented to determine the time moment, when the fastest flux changes are recorded. The primary search was carried out, first, on 30 s averaged data, then repeated on data with a higher resolution. A functional dependence was obtained in order to approximate the obtained set of intersections of the boundary by elliptical curve. The empirical model constructed using the CORONAS-Photon measurement data in the epoch of anomalously low geomagnetic activity reflects the longitude structure of the high-latitude boundary of the outer radiation belt associated with the internal Earth’s magnetic field (MF), as well as its dependence on the universal time. Based on the data of intersections of the high-latitude boundary of the outer ERB (OERB) in the epoch of 2014–2016, the latitudinal shift of the boundary to the equator dependent on geomagnetic activity has been determined, as well as the nightside shift of the boundary due to the diurnal rotation of the Earth. 相似文献
993.
A design procedure is outlined for optimizing stiffened, thin circular, cylindrical shells subject to a given set of destabilizing loads, in the presence of a specified initial geometric imperfection. The procedure incorporates two distinct steps (a) optimization based on linear buckling analyses and (b) imperfection sensitivity studies of the optimum design point from (a) as well as of the surrounding design space. A comparison of all these designs yield the true optimum in the presence of the specified geometric imperfection. The present methodology is fully demonstrated through two illustrative examples, one dealing with an axially loaded stiffened cylinder and one with a torsionally loaded one. 相似文献
994.
Joel S. Greenberg 《Space Policy》1987,3(3)
Rather than aiming at overall preemenence in space, as in the past, it is important for the USA now to specify goals and objectives for its space programme. In the space transportation market, the USA faces long-term competition. Planned properly, the Space Shuttle, Space Station and transfer stages can be used as a unique transport system, forcing other suppliers to compete on US terms. Such a total transport service system could also include ELV support. In entering into international space agreements, the government must take into account the objective of maintaining the competitiveness of the US commercial sector. 相似文献
995.
996.
在丁羟/铝粉/高氯酸铵组成的三组元推进剂体系中,通过药浆流变性测试、动态力学分析(DMA)、单向拉伸性能、凝胶分数和相对交联密度的测定,研究了一些功能组分如氮丙啶类化合物MAPO、醇胺络合物TEA·BF3、胺类化合物H对推进剂工艺性能和力学性能的影响.结果表明,MAPO可以降低药浆屈服值和表观粘度,改善工艺性能,显著增加最大抗拉强度,但对最大伸长率无影响;TEA·BF3大幅度增加药浆屈服值,使工艺性能变差,一定程度上提高最大抗拉强度和发挥熵弹性而增加最大伸长率,H可以显著改善推进剂工艺性能和增加最大伸长率.文中还对功能组分在推进剂中的作用机理进行了分析探讨. 相似文献
997.
丁羟推进剂粘合剂网络结构调控方法探讨 总被引:4,自引:2,他引:4
把扩链剂的使用作为调整丁羟推进剂粘合剂网络及其形态结构的一个重要手段。采用扩链剂、交联剂和真实固化参数(Rt)等综合的方法调控丁羟推进剂性能,可望比单纯控制名义固化参数(Ro)获得更好的力学性能及其稳定性。推导了丁羟推进剂粘合剂系统网络调整的通用计算公式和各种特定条件下的计算公式。 相似文献
998.
Determination of the Microacceleration Quasisteady Component onboard the International Space Station
Babkin E. V. Belyaev M. Yu. Efimov N. I. Sazonov V. V. Stazhkov V. M. 《Cosmic Research》2004,42(2):155-164
A comparison of two methods of determination of the microacceleration quasisteady component arising onboard the International Space Station was performed. In the first method the acceleration was calculated using the relative motion of the station reconstructed on the basis of telemetry data. The second method was a direct measurement of the microacceleration by a low-frequency accelerometer and a smoothing of the data obtained. The used measurements were made by the American accelerometer MAMS. The above comparison can theoretically be used to refine the position of the station center of mass relative to its body. 相似文献
999.
Eiges P. E. Zastenker G. N. Safrankova J. Nemecek Z. Eismont N. A. 《Cosmic Research》2001,39(5):432-438
Based on simultaneous measurements of ion fluxes made onboard the closely separated satellites Interball-1and Magion-4, the propagation velocity of middle-scale plasma structures in the Earth's foreshock relative to the solar wind flow is estimated. The derived value of this velocity allows these structures to be identified as a fast magnetosonic wave propagating upstream of the solar wind inflowing the Earth's bow shock. An evaluation is also made of the correlation length of these disturbances in the plane perpendicular to the Sun–Earth line. This length is approximately equal to 2R
E. 相似文献
1000.