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951.
舰载直升机着舰过程复杂。与地面降落相比,舰面的不稳定气流使得直升机姿态难以保持,下降的速度更大,且由于直升机通常都是单轮着舰,导致起落架载荷很大。为了研究直升机在不同条件下着舰时起落架的动态响应,建立了机体/起落架/舰船耦合模型,将着舰过程中直升机的运动和舰船的运动联系起来,通过仿真计算得出起落架的动态响应。仿真计算结果表明:直升机着舰质量越大,起落架压缩量和载荷越大;直升机低头着舰会导致前起落架载荷显著增大;直升机着舰下沉速度过大会导致着舰载荷急剧增大,可能会对结构造成破坏。 相似文献
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T.S. Kiss N. Gyenge R. Erdélyi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):611-616
Jets, whatever small (e.g. spicules) or large (e.g. macrospicules) their size, may play a key role in momentum and energy transport from photosphere to chromosphere and at least to the low corona. Here, we investigate the properties of abundant, large-scale dynamic jets observable in the solar atmosphere: the macrospicules (MS). These jets are observationally more distinct phenomena than their little, and perhaps more ubiquitous, cousins, the spicules. Investigation of long-term variation of the properties of macrospicules may help to a better understanding of their underlying physics of generation and role in coronal heating. Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory, a new dataset, with several hundreds of macrospicules, was constructed encompassing a period of observations over six years. Here, we analyse the measured properties and relations between these properties of macrospicules as function of time during the observed time interval. We found that cross-correlations of several of these macrospicule properties display a strong oscillatory pattern. Next, wavelet analysis is used to provide more detailed information about the temporal behaviour of the various properties of MS. For coronal hole macrospicules, a significant peak is found at around 2-year period. This peak also exists partially or is shifted to longer period, in the case of quiet Sun macrospicules. These observed findings may be rooted in the underlying mechanism generating the solar magnetic field, i.e. the global solar dynamo. 相似文献
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Hiroya Yamaguchi Midori Ozawa Takao Ohnishi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We report the discovery of recombining plasmas in three supernova remnants (SNRs) with the Suzaku X-ray astronomy satellite. During SNR’s evolution, the expanding supernova ejecta and the ambient matter are compressed and heated by the reverse and forward shocks to form an X-ray emitting hot plasma. Since ionization proceeds slowly compared to shock heating, most young or middle-aged SNRs have ionizing (underionized) plasmas. Owing to high sensitivity of Suzaku, however, we have detected radiative recombination continua (RRCs) from the SNRs IC 443, W49B, and G359.1–0.5. The presence of the strong RRC is the definitive evidence that the plasma is recombining (overionized). As a possible origin of the overionization, an interaction between the ejecta and dense circumstellar matter is proposed; the highly ionized gas was made at the initial phase of the SNR evolution in dense regions, and subsequent rapid adiabatic expansion caused sudden cooling of the electrons. The analysis on the full X-ray band spectrum of IC 443, which is newly presented in this paper, provides a consistent picture with this scenario. We also comment on the implications from the fact that all the SNRs having recombining plasmas are correlated with the mixed-morphology class. 相似文献
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在一个群通信体系中,最基本并且最具有实际意义的认证系统是指关于动态发送者的多接收认证码(简称DMRA-code).但目前,许多学者对其研究仅仅局限于对一个信源的认证.然而在网络通信中,常常会有多信源传播的场景.基于这个问题,利用多项式构造一个具有动态发送功能的多信源认证码,并且验证了该模型的合理性以及计算出了可能的攻击概率,从而保证了所构造的方案的安全性. 相似文献
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960.
在分析研究直升机桨叶耐颗粒物/砂磨蚀标准主要技术要素的基础上,全面对比分析了MIL-STD-3033、ГОСТР52560-2006、GJB 1171-1991等国内外标准的基本内容,提出了装备研制及标准化工作相关建议。 相似文献