铝合金搅拌摩擦焊后人工时效力学性能数值模拟

采用KWN模型构建搅拌摩擦焊接中Al-Mg-Si系铝合金沉淀相演化计算模型,通过将屈服强度分为晶粒大小、固溶相和析出相三部分贡献,可以计算平板搅拌摩擦焊后的屈服强度和硬度。进一步研究不同焊后人工时效条件下,焊接平板力学性能变化的机理。结果表明:更长的焊后保温时间有利于搅拌区力学性能的回复;较高的保温温度有利于搅拌区力学性能的快速回复,但是当温度高于200℃时,长时间保温会使母材软化,不利于力学性能回复;通过焊后人工时效不能明显改善热影响区的力学性能。     

雷雨影响空域容量的评估模型及方法

空域容量是实施空中交通流量管理措施的重要依据,尤其在雷雨天气条件下空域运行容量精准预判,是流量管理战术阶段的重点也是难点。本研究目的在于介绍一种量化评估天气对空域容量影响程度的计算模型,以及在流量管理战术阶段应用该模型的方法,并为开发气象和流量管理人员协同决策支持工具提供参考。本研究的创新之处,在于从天气对空中交通管制运行影响出发,选取流量管理员重点关注的五个关键气象指标,包括回波强度、降水强度、云顶高度、覆盖范围、位置趋势。研究结合运行实际进一步给出指标等级划分标准,运用指标权重提高了模型对不同空域结构的适用性。最后,通过选取典型场景进行实证研究,该模型的准确性和实用性得到初步验证,在战术流量管理阶段表现出较高的应用价值。     

A Novel Processing Route for Ni-doped Alumina Composites

Alumina-based composites containing 0-15wt% Ni metallic phase were produced by hot press-sintering Ni-coated alumina pow-ders. The Ni-coated alumina powders were prepared by the aqueous heterogeneous precipitation of alumina micro-powders and nickel sulfate salt followed by reduction process. The microstructural features and dispersion of Ni phase in Ni-coated alumina powders and the subsequent alumina-Ni cermets were investigated using scanning electron microscope (SEM), X-ray diffractometer (XRD), and trans-mission electron microscope (TEM). The relative density of the hot press-sintered composites was measured with the Archimedes’ method while the fracture strength and the fracture toughness were defined with the three-point bending method and the mi-cro-indentation fracture method. In the formation of alumina-Ni cermets from sintered Ni-coated alumina powders, Ni phase to some extent limits the densification rate and stifles the coarsening and growing process of alumina grains. The Ni phase is found to be located at the interfaces and the triple-joint junctions of alumina grains which results into alteration of the fracture mode of alumina and its in-creased fracture strength and fracture toughness if compared with monolithic alumina.     

Phase-field Modeling of the Influence of Elastic Field on the Nucleation and Microstructure Evolution in Precipitation

A phase-field method was employed to study the influence of elastic field on the nucleation and microstructure evolution. Two kinds of nucleation process were considered:one using fixed nucleation probability and the other calculated from the classical nucleation theory. In the latter case, the simulated results show that the anisotropic elastic strain field yields significant effects on the behavior of nucleation. With a large lattice misfit between the matrixes and the precipitates, the nucleation process does not appear fully random but displays some spatial correlation and has a preference for the elastic soft direction. However, with a small lattice misfit, this bias does not look quite clear. On the contrary, in the case of fixed nucleation probability, the elastic field has no influence on the nucleation proc- ess. The lattice mismatch also exerts influences on the microstructure morphology: with lattice mismatch becoming larger, the micro- structure proves to align along the elastic soft direction.     

Investigation of PMSE dependence on high energy particle precipitation during their simultaneous occurrence

This paper is based on the observations of Polar Mesosphere Summer Echoes (PMSE) with the EISCAT VHF 224?MHz radar during the summer month 08–12 July 2013. The effect of high energy particle precipitation on PMSE intensity, particularly during their simultaneous occurrence for longer time interval (longer than or equal to 3-h) has been investigated. The correlation between the two phenomena has been computed using the Spearman rank and Pearson linear correlation coefficient. The variations in high energy particle precipitation reaching down to altitude of 91?km and PMSE intensity in the altitude range of 80–90?km are positively correlated. The electron density irregularity due to ionization caused by precipitating particles might be one of the possible reasons for this positive correlation. Moreover, some other background parameters i.e. K-indices (proxy of high energy particle precipitation) and electron fluxes during the simultaneous occurrence of the two phenomena also support one of the possible reasons given for explanation of the observed positive correlation. The X-rays and proton fluxes have no noticeable effect on PMSE echoes in this study.     

基于ARIMA模型的拉萨降水量时间序列分析与预测

应用差分自回归滑动平均模型（ARIMA）模型对西藏拉萨地区1969年至2009年的年降水量资料进行建模分析。建立的模型通过了参数的显著性检验和模型的显著性检验。模型的实证分析表明在短期内模型具有较高的预测精度,ARIMA模型可以较好的应用于降水量的预测,对相关部门采取措施应对自然灾害提供了理论支持。     

Calculation of yield strength in nickel base single crystal superalloys

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Solar particle precipitation into the polar atmosphere and their dependence on hemisphere and local time

The precipitation of solar energetic particles, protons as well as electrons, at high latitudes is commonly assumed to be homogeneous across both polar caps. Using Low-Earth Orbit POES (Polar Orbiting Environmental Satellites) we determine particle penetration ratios into the polar atmosphere for protons ranging from about 0.1 MeV to 500 MeV and for electrons spanning about one order of magnitude in energy with a maximum of 0.3 MeV. Based on power law fits for the POES spectrum we show, that for energies interesting for middle and lower atmosphere chemistry, particle flux over the poles is comparable in magnitude to flux at the geostationary orbit or at L1 in interplanetary space. The time period under study are the solar energetic particle (SEP) event series of October/November 2003 and January 2005.     

Correlation between the cosmic noise absorption calculated from the SARINET data and the energetic particles measured by MEPED: Simultaneous observations over SAMA region

The cosmic noise absorption is presented in terms of two-dimensional images obtained from the imaging riometers operated at the Southern Space Observatory (geographic coordinate: 29.4° S, 53.1° W), in São Martinho da Serra, Brazil, Concepcion (geographic coordinate: 36.5° S, 73.0° W) and Punta Arenas (geographic coordinate: 53.0° S, 70.5° W) in Chile, which belong to the South American Riometer Network and are located at the central and periphery regions of the South American Magnetic Anomaly. Correlations are performed between the maximum cosmic noise absorption observed at these stations and the energetic electron flux in two energy channels (>30 and >300 keV) and the proton flux in three energy channels (80–240, 800–2500 and >6900 keV) as measured by the Medium Energy Proton and Electron Detector, during a moderate geomagnetic storm that occurred on September 3, 2008. The results show high correlations between the cosmic noise absorption detected at São Martinho da Serra and the flux of protons with energy between 80 and 240 keV, and the flux of electrons with energies higher than 300 keV, while an additional ionization at Concepcion was correlated with electrons of energies higher than 30 keV. The cosmic noise absorption detected at Punta Arenas was probably caused by the increase of the protons flux with energy between 80 and 240 keV.     

TB17钛合金等温时效析出行为

采用X射线衍射( XRD)、透射电子显微镜( TEM)、光学显微镜( OM)等对新型超高强韧 TB17钛合金次生α相转变动力学进行研究。实验结果表明,该合金经β相区固溶,520℃不同保温时间时效后,片层次生α相在β相基体上析出、形核、长大,并且与基体具有柏氏共格关系。短时时效后次生α相呈针状,随着保温时间延长,次生α相粗化呈短棒状。析出相含量对TB17钛合金强化具有重要影响,TB17钛合金在完全析出过程中,次生α相含量增加,时效硬化作用增加。 TB17钛合金次生α相等温相变动力学采用 JMAK方程进行描述。