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941.
Yu. M. Ignatkin P. V. Makeev V. I. Shaidakov A. I. Shomov 《Russian Aeronautics (Iz VUZ)》2018,61(3):396-403
The research is conducted of aerodynamic performance of the Mi-8 helicopter main rotor in the hover state and the vertical descent state, including vortex ring states (VRSs). Total and distributed aerodynamic performance, wake patterns, and main rotor flow patterns are calculated. The findings and results were compared with those provided by other researchers. 相似文献
942.
E.I. Daibog Yu.I. Logachev S. Kahler K. Kecskemty S. McKenna-Lawlor 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,32(12):2661-2666
The values of the characteristic decay time of particle fluxes in SEP events vary, as a rule, considerably from event to event. We point out, however, that at times sequences of events having similar decay times were observed over long time intervals (up to one month, and even longer in a few cases). The values of the decay times, however, differed among different sequences. The constancy of the decay phase in each consecutive event of these series suggests that the interplanetary medium was in steady state during the event series, and, because of solar rotation, its uniformity within sectors extended to 90–180° in heliolongitude. The very rarely observed long series (up to 2–3 solar rotations) indicate the steadiness and homogeneity of the plasma and the interplanetary magnetic field (IMF) in the entire inner solar system in the course of this time span. It is pointed out that the neutral current sheet of the IMF does not represent a substantial obstacle for energetic charged particles. Both hemispheres are (above and below the current sheet), at least during the series of solar events, invariant with time, uniform and alike from the viewpoint of the propagation of charged particles. The investigation of such sequences of events can also be useful for forecasting characteristics of SEP events. 相似文献
943.
S. Yashiro N. Gopalswamy P. Mäkelä S. Akiyama W. Uddin A.K. Srivastava N.C. Joshi R. Chandra P.K. Manoharan K. Mahalakshmi V.C. Dwivedi R. Jain A.K. Awasthi N.V. Nitta M.J. Aschwanden D.P. Choudhary 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Active region NOAA 11158 produced many flares during its disk passage. At least two of these flares can be considered as homologous: the C6.6 flare at 06:51 UT and C9.4 flare at 12:41 UT on February 14, 2011. Both flares occurred at the same location (eastern edge of the active region) and have a similar decay of the GOES soft X-ray light curve. The associated coronal mass ejections (CMEs) were slow (334 and 337 km/s) and of similar apparent widths (43° and 44°), but they had different radio signatures. The second event was associated with a metric type II burst while the first one was not. The COR1 coronagraphs on board the STEREO spacecraft clearly show that the second CME propagated into the preceding CME that occurred 50 min before. These observations suggest that CME–CME interaction might be a key process in exciting the type II radio emission by slow CMEs. 相似文献
944.
945.
Yu. A. Kovalev V. I. Vasil’kov M. V. Popov V. A. Soglasnov P. A. Voitsik M. M. Lisakov A. M. Kut’kin N. Ya. Nikolaev N. A. Nizhel’skii G. V. Zhekanis P. G. Tsybulev 《Cosmic Research》2014,52(5):393-402
The results of a large number of the antenna radiometric measurements at bands of 92, 18, 6.2, 1.35, and 1.7-1.2 cm are presented by the data of the standard telemetry system of the Spektr-R spacecraft. Both special sessions of calibration object observations in the mode of a single space radio telescope (SRT) operation and numerous observations of researched sources in the mode of the ground-space interferometer were used. The obtained results agree with the first results of Kardashev et al. (2013), i.e., within 10–15% at bands of 92, 18, and 6.2 cm and 20–25% at the band of 1.35 cm. In the main, the measurements for the eight subbands at wavelengths of 1.7-1.2 cm indicate a monotonic increase in the spectral system equivalent flux density (SEFD) of noise radiation with a frequency consistent with the calculated estimates for the discussed model. The sensitivity of the ground-space interferometer for the five subbands at wavelengths from 1.35 to 1.7 cm can be higher by a factor of 1.5, and for the three subbands from 1.35 to 1.2 cm lower by a factor of 1.5 than at the band of 1.35 cm. The SRT contribution to the interferometer sensitivity proportional to the square root of SEFD is close to the design one at the bands of 92 and 18 cm and decreases the design sensitivity approximately by a factor of 1.5 and 2 at the bands of 6.2 and 1.35 cm, respectively. These differences of implemented values from the design ones were not significantly affected the scientific program implementation. 相似文献
946.
提出航天铝合金深腔零件整体成形方法,开展预制坯优化设计。对比分析直筒和变径筒两种预制筒坯结构变形规律,数值模拟研究了底部圆角对开口球形件液压成形的影响规律。以直径D=450 mm的球形整体零件为验证对象,进行底部圆角r=60 mm的变径筒形件的液压成形试验验证。结果表明:直筒坯液压成形时,赤道位置发生破裂;变径筒坯液压成形时,当胀形压力为16 MPa即发生贴模;液压成形时,筒端口自适应补料,所以上半球的壁厚分布均匀;随着底部圆角越大,筒底部减薄越小,筒壁厚越均匀;当底部圆角为r=60 mm时,开口球壳赤道位置壁厚减薄最严重,减薄率为11.1%,球底部减薄率为9.8%,开口球壳上半球壁厚差为0.17 mm,下半球壁厚差为0.43 mm。 相似文献
947.
概述了机载雷达技术发展的基本情况,总结出有源相控阵雷达相对于传统的机械雷达所具有的独特优势,指出有源相控阵雷达是未来机载雷达的一个发展方向。 相似文献
948.
为了解塞式喷管底部压强特点,找出快速、准确计算底部压强的方法,实验研究了不同反压下塞式喷管的底部压强.在认识外界反压对塞式喷管流动作用机理的基础上分析如何确定不同的底部气动状态,将塞式喷管底部在不同外界反压下的气动状态划分为"三段",即底部开放段、底部闭合段和底部由开到闭的过渡段,在各段,底部压强使用不同的计算方法.把数值模拟、实验研究及塞式喷管底部自身特点结合起来,找出塞式喷管底部压强的一般规律,建立了适合于工程应用的底部压强计算模型.结合40%和20%截短塞式喷管的实验数据,验证了底部模型的正确性.塞式喷管底部流动是超声速流的大分离流动,该模型对底部压强的预示比有限差分法具有更高的精度. 相似文献
949.
为充分利用舰空导弹中制导段所获信息并减小导弹中制导段的弹道曲率,给出一种弹目预测遭遇点的解算方法,并据此设计比例导引制导律。在初始发射坐标系中,假设目标由当前位置以当前速度大小沿当前速度方向匀速运动至遭遇点,导弹由当前位置以当前速度大小按照一定的导引规律匀速运动至遭遇点。在该假设条件下,导弹到达遭遇点的总航路大小一方面... 相似文献
950.