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文中基于每个DMU的区间效率值,给出了区间DEA模型求解的一种方法并研究了它的有效性,同时将这种方法应用于基地伪装方案的选取问题。 相似文献
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基于DCOM技术构建分布式数控故障诊断系统 总被引:5,自引:0,他引:5
简要介绍DCOM技术的特点,对利用DCOM技术构建分布式数控故障诊断系统进行了研究,并提出了系统的组件模型结构。 相似文献
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高职教育技能竞赛和课程群建设间普遍存在着相互独立运行、沟通渠道不畅、缺乏促进机制等问题.针对上述问题,提出了在技能竞赛与课程群建设间建立良性互动机制的构想,设计了互动机制的循环反馈调节模型,分析了互动要素的驱动关系,给出了互动机制在课程群建设中的实现思路和操作方法. 相似文献
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Crider Dana H. Brain David A. Acuña Mario H. Vignes Didier Mazelle Christian Bertucci Cesar 《Space Science Reviews》2004,111(1-2):203-221
We examine the magnetic field in the martian magnetosheath due to solar wind draping. Mars Global Surveyor provided 3-D vector magnetic field measurements at a large range of altitudes, local times, and solar zenith angles as the spacecraft orbit evolved. We choose orbits with very clean signatures of draping to establish the nominal morphology of the magnetic field lines at local times of near-subsolar and near-terminator. Next, using a compilation of data from Mars Global Surveyor, we determine the average magnetic field morphology in the martian magnetosheath due to the solar wind interaction. The topology of the field is as expected from previous observations and predictions. The magnetic field magnitude peaks at low altitude and noon magnetic local time and decreases away from that point. The magnetic field has an inclination from the local horizontal of 5.6° on average in the dayside magnetosheath and 12.5° on the nightside. The inclination angle is closest to zero at noon magnetic local time and low altitude. It increases both upward and to later local times. The magnetic field in the induced magnetotail flares out from the Mars—Sun direction by 21°. Finally, we compare the observations to gasdynamic model predictions and find that the shocked solar wind flow in the martian magnetosheath can be treated as a gasdynamic flow with the magnetic pileup boundary as the inner boundary to the flow. 相似文献
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MESSENGER: Exploring Mercury’s Magnetosphere 总被引:1,自引:0,他引:1
James A. Slavin Stamatios M. Krimigis Mario H. Acuña Brian J. Anderson Daniel N. Baker Patrick L. Koehn Haje Korth Stefano Livi Barry H. Mauk Sean C. Solomon Thomas H. Zurbuchen 《Space Science Reviews》2007,131(1-4):133-160
The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury offers our first opportunity
to explore this planet’s miniature magnetosphere since the brief flybys of Mariner 10. Mercury’s magnetosphere is unique in
many respects. The magnetosphere of Mercury is among the smallest in the solar system; its magnetic field typically stands
off the solar wind only ∼1000 to 2000 km above the surface. For this reason there are no closed drift paths for energetic
particles and, hence, no radiation belts. Magnetic reconnection at the dayside magnetopause may erode the subsolar magnetosphere,
allowing solar wind ions to impact directly the regolith. Inductive currents in Mercury’s interior may act to modify the solar
wind interaction by resisting changes due to solar wind pressure variations. Indeed, observations of these induction effects
may be an important source of information on the state of Mercury’s interior. In addition, Mercury’s magnetosphere is the
only one with its defining magnetic flux tubes rooted beneath the solid surface as opposed to an atmosphere with a conductive
ionospheric layer. This lack of an ionosphere is probably the underlying reason for the brevity of the very intense, but short-lived,
∼1–2 min, substorm-like energetic particle events observed by Mariner 10 during its first traversal of Mercury’s magnetic
tail. Because of Mercury’s proximity to the sun, 0.3–0.5 AU, this magnetosphere experiences the most extreme driving forces
in the solar system. All of these factors are expected to produce complicated interactions involving the exchange and recycling
of neutrals and ions among the solar wind, magnetosphere, and regolith. The electrodynamics of Mercury’s magnetosphere are
expected to be equally complex, with strong forcing by the solar wind, magnetic reconnection, and pick-up of planetary ions
all playing roles in the generation of field-aligned electric currents. However, these field-aligned currents do not close
in an ionosphere, but in some other manner. In addition to the insights into magnetospheric physics offered by study of the
solar wind–Mercury system, quantitative specification of the “external” magnetic field generated by magnetospheric currents
is necessary for accurate determination of the strength and multi-polar decomposition of Mercury’s intrinsic magnetic field.
MESSENGER’s highly capable instrumentation and broad orbital coverage will greatly advance our understanding of both the origin
of Mercury’s magnetic field and the acceleration of charged particles in small magnetospheres. In this article, we review
what is known about Mercury’s magnetosphere and describe the MESSENGER science team’s strategy for obtaining answers to the
outstanding science questions surrounding the interaction of the solar wind with Mercury and its small, but dynamic, magnetosphere. 相似文献
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摘要:针对卫星对于空间动态目标快速、稳定地跟踪、控制目标,同时考虑平台模型的不确定性、外部随机干扰、系统控制力矩与角速度约束等因素,设计PD+控制器实现对于动态目标的快速、稳定跟踪;在经典PD控制器的基础上设计控制添加项使得系统能够按照既定轨迹运动;采用变结构的手段实现系统收敛速度的提升;合理设计Lyapunov函数的结构,引出角速度、四元数的耦合项对V函数进行改良,简化系统稳定性证明与分析的过程;讨论系统最极端情形,通过对V函数上下界的讨论分析系统该情形下的稳定性;最后通过数值仿真验证所提出算法的有效性与优越性. 相似文献
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数控抛光能够达到一致性较高的表面粗糙度要求。试验研究了羊毛毡轮数控抛光层数对磨削后GH4169表面残余应力的影响,进给方向表面残余正应力随深度增加先升高后下降,而垂直进给方向表面残余正应力先基本不变后下降,优化抛光层数为3层。针对磨削后抛光工艺,提出了"加强筋"模型,将羊毛毡轮抛光过程分为两个阶段,解释了抛光对表面残余应力的影响机理,并改变抛光参数进行了初步的试验验证。 相似文献