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711.
民用飞机结构非计划直接维修成本在设计阶段难以预计。介绍DMC构成要素及影响因素,建立DMC预计流程、预计模型及预计调整模型;以前中机身上蒙皮壁板为例,基于工程设计输入及统计报告,计算来自MSG-3,DTA,DSEA的非计划维修任务DMC数值,对比并分析金属及复合材料非计划DMC预计结果。结果表明:该预计方法可行,反映预计模型准确性,金属结构环境退化及疲劳损伤是影响该结构DMC的主要因素,复合材料的使用可显著降低飞机结构非计划DMC。 相似文献
712.
Petri网理论及其在离散事件系统中的应用 总被引:2,自引:0,他引:2
本文扼要介绍Petri网理论及Petri网图。阐明了Petri网的解析方法,举出了用Petri网建立离散事件系统模型的例子。最后用Petri网不变量对系统进行了验证。 相似文献
713.
714.
M. I. Desai G. M. Mason R. E. Gold S. M. Krimigis C. M. S. Cohen R. A. Mewaldt J. E. Mazur J. R. Dwyer 《Space Science Reviews》2007,130(1-4):243-253
Using high-resolution mass spectrometers on board the Advanced Composition Explorer (ACE), we surveyed the event-averaged
∼0.1–60 MeV/nuc heavy ion elemental composition in 64 large solar energetic particle (LSEP) events of cycle 23. Our results
show the following: (1) The Fe/O ratio decreases with increasing energy up to ∼10 MeV/nuc in ∼92% of the events and up to
∼60 MeV/nuc in ∼64% of the events. (2) The rare isotope 3He is greatly enhanced over the corona or the solar wind values in 46% of the events. (3) The heavy ion abundances are not
systematically organized by the ion’s M/Q ratio when compared with the solar wind values. (4) Heavy ion abundances from C–Fe exhibit systematic M/Q-dependent enhancements that are remarkably similar to those seen in 3He-rich SEP events and CME-driven interplanetary (IP) shock events. Taken together, these results confirm the role of shocks
in energizing particles up to ∼60 MeV/nuc in the majority of large SEP events of cycle 23, but also show that the seed population
is not dominated by ions originating from the ambient corona or the thermal solar wind, as previously believed. Rather, it
appears that the source material for CME-associated large SEP events originates predominantly from a suprathermal population
with a heavy ion enrichment pattern that is organized according to the ion’s mass-per-charge ratio. These new results indicate
that current LSEP models must include the routine production of this dynamic suprathermal seed population as a critical pre-cursor
to the CME shock acceleration process. 相似文献
715.
The heliospheric counterparts of coronal mass ejections (CMEs) at the Sun, interplanetary coronal mass ejections (ICMEs),
can be identified in situ based on a number of magnetic field, plasma, compositional and energetic particle signatures as
well as combinations thereof. We summarize these signatures and their implications for understanding the nature of these structures
and the physical properties of coronal mass ejections. We conclude that our understanding of ICMEs is far from complete and
formulate several challenges that, if addressed, would substantially improve our knowledge of the relationship between CMEs
at the Sun and in the heliosphere. 相似文献
716.
R. Schwenn 《Space Science Reviews》2006,124(1-4):51-76
In this paper I will briefly summarize the present status of our knowledge on the four different sorts of solar wind, their
sources and their short- and long-term variations. First: the fast solar wind in high-speed streams that emerges from coronal
hole regions. Second: the slow solar wind emerging from the non-active Sun near the global heliospheric current sheet above
helmet streamers and underlying active regions. Third: the slow solar wind filling most of the heliosphere during high solar
activity, emerging above active regions in a highly turbulent state, and fourth: the plasma expelled from the Sun during coronal
mass ejections. The coronal sources of these different flows vary dramatically with the solar activity cycle. 相似文献
717.
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719.
根据振动理论,分析了直管式科氏质量流量计的最佳理论测量点;由于实际工程中必须考虑噪声条件,而在噪声环境中通常采用信号的最大似然估计算法,所以本文仿真了不同信噪比条件下的信号检测,结果表明最佳测量点同环境的噪声有关,并给出了不同信噪比条件下直管式科氏质量流量计最佳测量点。该结果同实验数据基本吻合。 相似文献
720.
一种适合我国在轨卫星液体推进剂剩余量测量的技术方案 总被引:5,自引:0,他引:5
比较全面地介绍了适合我国卫星液体推进剂测量的气体注入压力激励方法,对相关应用技术问题进行了分析讨论。该方法可实现推进剂测量误差达贮箱总体积的1%的高精度测量要求,具有很好的开发价值。 相似文献