A new method to predict fatigue crack growth rate of materials based on average cyclic plasticity strain damage accumulation

By introducing a fatigue blunting factor, the cyclic elasto-plastic Hutchinson-Rice-Rosengren (HRR) field near the crack tip under the cyclic loading is modified. And, an average damage per loading-cycle in the cyclic plastic deformation region is defined due to Manson-Coffin law. Then, according to the linear damage accumulation theory-Miner law, a new model for predicting the fatigue crack growth (FCG) of the opening mode crack based on the low cycle fatigue (LCF) damage is set up. The step length of crack propagation is assumed to be the size of cyclic plastic zone. It is clear that every parameter of the new model has clearly physical meaning which does not need any human debugging. Based on the LCF test data, the FCG predictions given by the new model are consistent with the FCG test results of Cr2Ni2MoV and X12CrMoWVNbN 10-1-1. What’s more, referring to the relative researches, the good predictability of the new model is also proved on six kinds of materials.     

基于Keystone变换和MDCFT的高机动弱目标检测与参数估计

 常规雷达对隐身、超声速和高机动目标存在回波信噪比不足、距离徙动和多普勒谱扩展问题。将Keystone变换和修正离散Chirp-Fourier变换(MDCFT)相结合,提出了一种新的雷达信号处理算法。该算法通过Keystone变换补偿距离徙动问题,利用MDCFT对多普勒谱严重扩展的目标回波进行相参积累,提高目标检测性能的同时完成了对目标参数的估计,且该算法在方位向欠采样时仍可适用。最后对算法运算量及性能进行了分析,通过仿真验证了该算法的有效性。     

The Middle Atmospheric Ozone Response to the 11-Year Solar Cycle

Because of its chemical and radiative properties, atmospheric ozone constitutes a key element of the Earth’s climate system. Absorption of sunlight by ozone in the ultraviolet wavelength range is responsible for stratospheric heating, and determines the temperature structure of the middle atmosphere. Changes in middle atmospheric ozone concentrations result in an altered radiative input to the troposphere and to the Earth’s surface, with implications on the energy balance and the chemical composition of the lower atmosphere. Although a wide range of ground- and satellite-based measurements of its integrated content and of its vertical distribution have been performed since several decades, a number of uncertainties still remain as to the response of middle atmospheric ozone to changes in solar irradiance over decadal time scales. This paper presents an overview of achieved findings, including a discussion of commonly applied data analysis methods and of their implication for the obtained results. We suggest that because it does not imply least-squares fitting of prescribed periodic or proxy data functions into the considered times series, time-domain analysis provides a more reliable method than multiple regression analysis for extracting decadal-scale signals from observational ozone datasets. Applied to decadal ground-based observations, time-domain analysis indicates an average middle atmospheric ozone increase of the order of 2% from solar minimum to solar maximum, which is in reasonable agreement with model results.     

The Response of the Middle Atmosphere to Solar Cycle Forcing in the Hamburg Model of the Neutral and Ionized Atmosphere

This paper studies the response of the middle atmosphere to the 11-year solar cycle. The study is based on numerical simulations with the Hamburg Model of the Neutral and Ionized Atmosphere (HAMMONIA), a chemistry climate model that resolves the atmosphere from the Earth’s surface up to about 250 km. Results presented here are obtained in two multi-year time-slice runs for solar maximum and minimum conditions, respectively. The magnitude of the simulated annual and zonal mean stratospheric response in temperature and ozone corresponds well to observations. The dynamical model response is studied for northern hemisphere winter. Here, the zonal mean wind change differs substantially from observations. The statistical significance of the model’s dynamical response is, however, poor for most regions of the atmosphere. Finally, we discuss several issues that render the evaluation of model results with available analyses of observational data of the stratosphere and mesosphere difficult. This includes the possibility that the atmospheric response to solar variability may depend strongly on longitude.     

基于并口EPP协议的软件加密卡的设计与开发

本文主要阐述了基于并口EPP协议的软件加密卡的硬件设计。根据实践经验，重点介绍了器件选型与EPP并口时序关键点等注意事项。具有较强的实践意义。     

超/亚声速混合层压力不匹配时流动特征

为了获得压力不匹配对超/亚声速混合层空间分布与增长、压力分布和相似性等特征的影响规律,开展试验和数值模拟研究。通过粒子图像测速技术PIV测量混合层空间分布,标准k-ω模型模拟稳态流场特征。超声速气流马赫数为1.32,亚声速气流马赫数为0.11,五组不同压比分别为0.82,0.95,1.11,1.22和1.47。研究结果表明：压力不匹配对混合层增长的影响较弱;当压比>1时,混合层沿流向呈现波纹分布,静压呈现高、低压交替分布;压比增加,混合层内无量纲速度分布不变,无量纲总压减小,而湍流强度增加。基于无粘假设的预测模型捕捉了波节的基本结构与分布。     

基于直升机飞行性能需求的涡轴发动机设计参数选取方法研究

以直升机性能计算方法为基础,辅以考虑尺寸效应及设计能力的涡轴发动机设计方法,建立了以直升机旋翼桨盘载荷及最大起飞功重比为特征参数的直升机/涡轴发动机性能约束分析模型、任务分析模型及基于直升机飞行性能需求的涡轴发动机设计参数选取模型。针对涡轴发动机部件/系统设计能力及直升机飞行性能需求,首先开展了给定涡轴发动机循环参数下的流量匹配计算,然后开展了涡轴发动机循环参数选取研究。研究表明,所建立的直升机/涡轴发动机性能约束分析模型、任务分析模型可实现给定飞行任务的直升机/涡轴发动机性能耦合设计;在给定涡轴发动机循环参数条件,由于尺寸效应,涡轴发动机部件效率受进口流量的影响,其设计点功率并不随流量等比例变化,从而使得直升机起飞总重呈现非等比例变化;在涡轴发动机循环参数选择时,在满足直升机飞行性能需求下,存在涡轴发动机耗油率与单位功率之间权衡下的循环参数选取,使得直升机起飞总重最小。     

间接起爆对脉冲爆震发动机热效率影响

建立了基于整个燃烧室内经历不同燃烧方式下所有工质来评估脉冲爆发动机平均循环热效率的方法,通过二维数值方法对两种采用不同数目障碍物的爆震管模型的起爆特性及循环热效率进行了研究,并分析了燃烧波传播的距离与DDT距离之比（定义为ξ）对模型热效率的影响.结果表明:①间接起爆方式及不同DDT强化装置都会影响系统的循环热效率;②就计算模型,当ξ接近1时,其系统平均循环热效率仅为理想爆震循环热效率的60%左右;③随着ξ的增加,间接起爆方式的影响迅速减弱;④当ξ为1.5时,系统平均循环热效率可达爆震燃烧热效率的93%.      

3 外涵变循环发动机循环参数匹配模拟

3外涵技术能使发动机涵道比调节范围更宽,使其在所有推力范围和全包线下性能最优。分析了带核心机驱动风扇级（CDFS）的3外涵变循环发动机工作机理,利用稳态性能数值仿真程序,开展了3外涵变循环发动机循环参数匹配模拟研究,得到发动机循环参数取值范围。研究结果表明：3外涵变循环发动机工作范围更广,重点是通过改变其涵道比来实现压比的变化和发动机模态的转变,最终实现3外涵变循环发动机的优越性能。     

Solar and interplanetary precursors of geomagnetic storms in solar cycle 23

Estimating the magnetic storm effectiveness of solar and associated interplanetary phenomena is of practical importance for space weather modelling and prediction. This article presents results of a qualitative and quantitative analysis of the probable causes of geomagnetic storms during the 11-year period of solar cycle 23: 1996–2006. Potential solar causes of 229 magnetic storms (Dst ? −50 nT) were investigated with a particular focus on halo coronal mass ejections (CMEs). A 5-day time window prior to the storm onset was considered to track backward the Sun’s eruptions of halo CMEs using the SOHO/LASCO CMEs catalogue list. Solar and interplanetary (IP) properties associated with halo CMEs were investigated and correlated to the resulting geomagnetic storms (GMS). In addition, a comparative analysis between full and partial halo CME-driven storms is established. The results obtained show that about 83% of intense storms (Dst ? −100 nT) were associated with halo CMEs. For moderate storms (−100 nT < Dst ? −50 nT), only 54% had halo CME background, while the remaining 46% were assumed to be associated with corotating interaction regions (CIRs) or undetected frontside CMEs. It was observed in this study that intense storms were mostly associated with full halo CMEs, while partial halo CMEs were generally followed by moderate storms. This analysis indicates that up to 86% of intense storms were associated with interplanetary coronal mass ejections (ICMEs) at 1 AU, as compared to moderate storms with only 44% of ICME association. Many other quantitative results are presented in this paper, providing an estimate of solar and IP precursor properties of GMS within an average 11-year solar activity cycle. The results of this study constitute a key step towards improving space weather modelling and prediction.