Can Surface Flux Transport Account for the Weak Polar Field in Cycle 23?

To reproduce the weak magnetic field on the polar caps of the Sun observed during the declining phase of cycle 23 poses a challenge to surface flux transport models since this cycle has not been particularly weak. We use a well-calibrated model to evaluate the parameter changes required to obtain simulated polar fields and open flux that are consistent with the observations. We find that the low polar field of cycle 23 could be reproduced by an increase of the meridional flow by 55% in the last cycle. Alternatively, a decrease of the mean tilt angle of sunspot groups by 28% would also lead to a similarly low polar field, but cause a delay of the polar field reversals by 1.5 years in comparison to the observations.     

翼身融合运输机分布式电推进系统设计及油耗评估

针对翼身融合运输机开展了分布式电推进系统的总体设计与油耗评估。通过数值计算完成了70t载质量翼身融合飞机的气动设计与优化。在巡航马赫数为0.80和10km高度的设计点,最大升阻比达到了24。通过求解积分边界层方程组,完成了电推进系统的总体设计。电推进系统包含10个推进风扇,风扇直径为1.45m,压比为1.35,巡航功率为2.94MW。建立了考虑燃烧过程的发动机一维性能模型,对发动机油耗进行了评估,获得了不同发动机循环参数下燃油消耗。建模结果表明,基于翼身融合布局和分布式电推进技术,可使运输机的油耗较C-17节省近50%。      

地面模拟微重力条件下Cu-Pb合金的制备及微观结构与摩擦性能研究

利用地面上建立的微重力电磁模拟设备成功制备出了Cu-Pb二元难混合金,并对其微观组织结构与摩擦性能进行了分析与测试。样品SEM分析结果表明,模拟微重力状态下制备的合金样品较好地克服了地面上因重力影响而产生的严重成分偏析,少数弥散相较均匀地分布于基体中,少数相含量越低,弥散体尺寸越小,分布越均匀;摩擦性能测试结果显示合金模拟样品的摩擦性能明显好于基体金属,且摩擦系数随少数相Pb的含量的增大而减小,体积磨损率随少数相含量的增大先快速减小而后又缓慢增大。同时对实验结果进行了简单的分析与讨论。     

窄条翼导弹俯仰机动中滚转失稳及其控制过程

窄条翼布局导弹通常具有复杂的横向气动特性,在大迎角飞行及快速机动中很容易诱发出现滚转非指令偏离和连续振荡,可能导致飞行失控,影响落点精度。为了研究窄条翼导弹俯仰快速机动对滚转失稳的诱发过程及滚转失稳对俯仰机动控制效果的影响,并验证三通道解耦控制方法的有效性,针对典型俯仰机动过程,分别利用2.4 m跨声速风洞虚拟飞行试验平台和耦合气动/运动/控制的一体化数值计算方法开展了相关研究。结果表明,风洞试验和数值模拟均成功预测了俯仰拉起和保持过程中的滚转自激失稳运动及其引起的纵、横向耦合运动,针对该机动过程,三通道解耦控制方法能够有效抑制滚转运动,保持姿态稳定。     

加强农民工社会保障建设的对策

改革开放以来,农民工为国家的城市化、工业化、现代化、社会经济的发展与繁荣作出了突出贡献,但是农民工并没有同城市居民一样分享经济发展的成果,农民工社会保障处于缺失状态。随着农民工数量的增多,农民工社会保障缺失问题引起了社会的广泛关注,成了政府、社会亟待解决的问题。文章主要分析了农民工社会保障现状及缺失的原因,并为加强农民工社会保障建设提出了一些政策建议。     

卫星推进剂剩余量测量技术地面试验研究

根据气体注入压力激励测量方法，研制了动态、高精度测量卫星液体推进剂剩余量原理样机，该样机以通信卫星双组元推进系统为测量对象。详细给出了利用该样机进行的地面试验情况，特别是测量数据平滑处理技术和液体蒸汽压误差修正技术。试验结果表明，当推进系统工作状态正常时，剩余液体体积量的测量误差小于贮箱总体积的１．０％，而当推进系统有小泄漏时，则小于２．０％。     

Stable two-sided matching of slot allocation in airport collaborative decision making by top trading cycles mechanism

The problem of capacity shortage in some airports needs to be dealt with sustainable solutions including a more efficient use of the existing runway slots at the airports. The Collaborative Decision Making (CDM) is an important approach applied to Air Traffic Management (ATM) to achieve this efficient use of the slots allocation. Using the Matching approach for two-sided markets of Game theory, the Top Trading Cycle CDM (TTC-CDM) algorithm developed in this research is an extension of the CDM approach aggregating the Ground Delay Program (GDP) of the air sector. The paper compared the developed TTC-CDM model to the existing models such as the conventional Compression algorithm in CDM, the Trade Cycle algorithm and the Deferred Acceptance CDM (DA-CDM) model to evaluate the performance of the proposed model. Through a case study, the results show the effective application of TTC-CDM model to slot allocation in ATM and also presents the advantage of considering the preferences of airport managers beside ATC controllers and airlines in the decision processing.     

基于多层PCB的基板射频信号传输性能研究

随着射频产品的小型化,特别是射频SIP(systems in package)产品的逐渐应用,基于多层PCB的基板射频组件等射频集成产品的应用越来越多,基板内射频信号传输性能的研究也越来越重要。通过对基于多层PCB的基板射频传输性能进行仿真测试,验证了DC-40GHz范围内射频基板传输性能,针对射频传输中极为关注的传输损耗问题,通过改进介质厚度或者铜箔材料实现基板射频传输损耗的优化,单位长度传输线射频传输损耗减小20%以上。同时针对星载等应用环境,通过深层充放电、总剂量试验,表明多层PCB的基板满足星载等航天应用。     

Evolution of the Moon: The 1974 model

The geology of the decade of Apollo and Luna probably will become one of the fundamental turning points in the history of all science. For the first time, the scientists of the Earth have been presented with the opportunity to interpret their home planet through the direct investigations of another. Mankind can be proud and take heart in this fact. The interpretive evolution of the Moon can be divided now into seven major stages beginning sometime near the end of the formation of the solar system. These stages and their approximate durations in time are as follows:

1. The Beginning — 4.6 billion years ago.
2. The Melted Shell — 4.6–4.4 billion years ago.
3. The Cratered Highlands — 4.4–4.1 billion years ago.
4. The Large Basins — 4.1–3.9 billion years ago.
5. The Light-colored Plains — 3.9–3.8 billion years ago.
6. The Basaltic Maria — 3.8–3.0 (?) billion years ago.
7. The Quiet Crust — 3.0 (?) billion years ago to the present.

The Apollo and Luna explorations that permit us to study these stages of evolution each have contributed in progressive and significant ways. Through them we now can look with new insight into the early differentiation of the Earth, the nature of the Earth's protocrust, the influence of the formation of large impact basins in that crust, the effects of early partial melting of the protomantle and possibly the earliest stages of the breakup of the protocrust into continents and ocean basins.     

l1-based calibration of POD-Galerkin models of two-dimensional unsteady flows

This paper discusses a physics-informed methodology aimed at reconstructing efficiently the fluid state of a system. Herein, the generation of an accurate reduced order model of two-dimensional unsteady flows from data leverages on sparsity-promoting statistical learning techniques. The cornerstone of the approach is l₁ regularised regression, resulting in sparsely-connected models where only the important quadratic interactions between modes are retained. The original dynamical behaviour is reproduced at low computational costs, as few quadratic interactions need to be evaluated. The approach has two key features. First, interactions are selected systematically as a solution of a convex optimisation problem and no a priori assumptions on the physics of the flow are required. Second, the presence of a regularisation term improves the predictive performance of the original model, generally affected by noise and poor data quality. Test cases are for two-dimensional lid-driven cavity flows, at three values of the Reynolds number for which the motion is chaotic and energy interactions are scattered across the spectrum. It is found that: (A) the sparsification generates models maintaining the original accuracy level but with a lower number of active coefficients; this becomes more pronounced for increasing Reynolds numbers suggesting that extension of these techniques to real-life flow configurations is possible; (B) sparse models maintain a good temporal stability for predictions. The methodology is ready for more complex applications without modifications of the underlying theory, and the integration into a cyber-physical model is feasible.