具有N-策略及Bernoulli反馈的M/M/1工作休假

研究具有N-策略及反馈的M/M/1工作休假排队模型.工作休假策略为空竭服务多重工作休假.在休假期间,服务员并未完全停止工作而是以相对于正常工作时较低的服务率为顾客服务.完成服务的顾客以概率p(0相似文献   

基于负顾客M/M/s/k＋M重试、反馈排队的呼叫中心性能分析

针对顾客到达时遇忙音重试、服务结束后以一定概率重新请求服务、顾客在排队中因不耐烦而放弃等待,以及负顾客等因素对系统产生的影响,研究了一类具有负顾客到达的,且顾客在ACD中排队中会因不耐烦而放弃等待的M/M/s/k＋M重试、反馈排队模型.运用矩阵几何方法求解,给出了解析解和系统的稳态性能指标,并给出数值计算实例以及适当提高服务率能降低总的顾客损失率等结论.     

应用非线性动态门限反馈(MF)模型剖析鞍山地应力异常

为论证鞍山地应力异常的可靠性,应用ＭＦ模型对其干扰和异常作了计算,发现１９９３年以来的长趋势及部分短期变化主要是干扰引起的,悬空元件和同期的室温、水位测值可作为其它受力元件的主要干扰因子．但在某些时段鞍山地应力仍有一定的趋势异常显示．     

对瞬变电磁法回线边长决定探测深度的质疑

质疑瞬变电磁法探测深度取决于场源磁矩（M=IL^2）的强度，当电源能量一定时，改变回线边长就成为控制探测深度的有效措施；认为“大回线有大深度”、“小回线探测浅”等共识是不正确的，它是不计条件应用深度公式的误导。研究认为：瞬变电磁法的探测深度取决于场源含有的低频成分，基频越低，探测越深；磁矩只是决定探测结果的信噪比。     

THE MEANDER OF KUROSHIO AND OSCILLATION IN A COUPLED OCEAN-ATMOSPHERE MODEL

A numerical experiment of an asynchronous coupled ocean-atmosphere model has been described in this paper.Atwo-layer global atmosphere general circulation model(OSU/IAP-AGCM)and a two-layer North Pacific Oceangeneral circulation model(NPOGCM)developed by Liu et al.(1992)are used in numerical experiment.The sea surfacetemperature anomaly(SSTA)corresponding to the meander of the Kuroshio is treated as the initial perturbation in thePacific Ocean and the abnormal phenomena caused by the disturbance and the interaction between atmosphere andocean,have been studied.The numerical experiment showed that the SST anomaly in the North Pacific could induce a new 30—60 dayoscillation through the coupling between atmosphere and ocean and the interaction between the meander of theKuroshio and atmosphere circulation is a positive feedback process.     

沙漠化扩展对区域气候影响的数值模拟研究

利用GCM -SSiB全球大气环流谱模式,设计两组数值模拟试验(即控制试验(CE)和沙漠面积扩大试验(DE)),研究了大陆沙漠化对我国区域气候变化的影响。模拟结果表明:沙区扩展后,大陆年平均地表温度降低,海平面气压上升,纬向风速、季风加强,夏季低空上升运动减弱,冬季下沉运动增强,降雨量显著减少,地表蒸发、感热和潜热通量亦显著减少。我国区域气候随大陆沙漠化扩展趋向冷干、风速加大,沙漠扩展与区域气候恶化存在正反馈。     

江汉盆地马王庙油田自生磁铁矿与烃运移相互关系研究

研究表明，已知油井M36井Ⅱ油组的含油层（位于Ⅱ油组的中—下部）中有明显呈规律分布的强磁性层。以平均值为例，含油岩层屑的饱和磁化强度Js=352.58A/m，饱和剩磁Jc=60.43A/m；而干层的Js=147.34A/m，Jr=22.09A/m。磁滞回线特征表明，含油层岩屑中以偏软的磁性矿物为主（平均矫顽力Hc=33.5mT，饱和磁场Hs=0.25T），而干层岩屑中主要为磁性偏碱的磁性矿物（Hc=44.2mT，H8=0.4T）。重矿物分析结果显示，干井M46井Ⅱ油组岩屑中含沙射影有较多的碎屑磁铁矿。磁学与矿物学参量的对应分析表明，含油层强磁性岩层的载体为自生成因的磁铁矿，而菱铁矿与黄铁矿为非磁性矿物，对Ⅱ油组岩层的磁性没有影响。由此，我们提出M36井含油层中的自生磁铁矿可能是原油的生物降解作用、碎屑矿物中高价铁的被置换及后期菱铁矿的氧化作用等多种不同时空条件下形成的产物。     

瞬变电磁法在煤矿水文地质灾害调查中的应用

以探测某地小煤窑遗留的采空区为例,探讨了瞬变电磁法在探测采空积水区的应用效果。选用同一回线装置形式,结合矿区地质条件,具体分析了采空积水区的地球物理异常特征。结果表明,该方法在煤矿水文地质灾害调查方面具有分辨率高、经济快速、准确有效等优势,能够满足煤矿安全生产的要求。     

复杂网络牵制控制概述

本文回顾了十多年来复杂网络牵制控制的研究进展,对复杂网络现有的牵制控制算法进行了归纳分类,然后基于网络拓扑及节点动力学特性讨论了网络牵制控制的一些必要或充分条件.针对牵制控制下的复杂网络,重点论述了牵制节点的选取策略,综合分析了牵制节点个数、耦合强度、牵制控制增益及节点动力学等因素对复杂网络牵制控制的影响,讨论了具有合作竞争关系符号网络牵制控制的进展,并简要介绍了复杂网络牵制控制的一些应用前景.最后,就复杂网络牵制控制将来的研究方向提了一些建议及展望.     

A new framework for isolating individual feedback processes in coupled general circulation climate models. Part I: formulation

This paper proposes a coupled atmosphere–surface climate feedback–response analysis method (CFRAM) as a new framework for estimating climate feedbacks in coupled general circulation models with a full set of physical parameterization packages. The formulation of the CFRAM is based on the energy balance in an atmosphere–surface column. In the CFRAM, the isolation of partial temperature changes due to an external forcing or an individual feedback is achieved by solving the linearized infrared radiation transfer model subject to individual energy flux perturbations (external or due to feedbacks). The partial temperature changes are addable and their sum is equal to the (total) temperature change (in the linear sense). The decomposition of feedbacks is based on the thermodynamic and dynamical processes that directly affect individual energy flux terms. Therefore, not only those feedbacks that directly affect the TOA radiative fluxes, such as water vapor, clouds, and ice-albedo feedbacks, but also those feedbacks that do not directly affect the TOA radiation, such as evaporation, convections, and convergence of horizontal sensible and latent heat fluxes, are explicitly included in the CFRAM. In the CFRAM, the feedback gain matrices measure the strength of individual feedbacks. The feedback gain matrices can be estimated from the energy flux perturbations inferred from individual parameterization packages and dynamical modules. The inter-model spread of a feedback gain matrix would help us to detect the origins of the uncertainty of future climate projections in climate model simulations.