超高强度300M钢电子束深缝焊接力学性能及破坏机理研究

超高强度300M钢具有优异的力学性能,广泛应用于飞机起落架。通过静力拉伸、三点弯曲及动态Charpy冲击试验,揭示300M钢电子束深缝焊接的力学性能及破坏机理;对试验后的典型试样进行断口宏观与微观分析,并采用场发射扫描电镜(SEM)对断口形貌进行观察、分析。结果表明:母材与焊接件都出现明显的拉伸塑性段,二者的刚度和强度相差不大,但是焊接件的断裂应变较母材小,焊接件焊缝的韧性略低于母材;焊接件弯曲强度与母材相当,但是破坏时的弯曲变形较母材也有所下降,焊接件的延性较差;在冲击试验中焊接件吸收能量与断裂韧性均低于母材,冲击韧度降低。     

TiAl合金粉床电子束选区熔化成形研究进展

粉床电子束选区熔化成形是增材制造脆性TiAl合金复杂构件的理想技术。从原料粉末、致密化、化学成分、微观组织、凝固及相变、后处理、力学性能、成形精度与表面粗糙度等几个方面综述了粉床电子束选区熔化成形TiAl合金的研究现状,对目前存在的问题及应对措施进行了评述,并对其未来研究方向进行了展望。     

放电发射光谱在金属微弧氧化表面处理中的应用研究进展

液相火花放电现象是金属微弧氧化表面处理时典型特征,发射光谱(OES)技术是表征微弧放电光谱特征和探索微弧氧化机理的有效手段。本文综述了铝、镁、钛等金属微弧氧化过程中发射光谱的研究现状。介绍微弧放电区等离子体的电子温度、电子密度等特征参数计算原理。重点关注了不同金属基体材料、电参数及电解液组成条件下,等离子体放电行为对微弧氧化膜结构的影响规律,并比较不同放电模型的异同。基于OES谱线评估得到的各种金属微弧等离子体温度为3000~10000 K,为放电通道内快速熔化-凝固过程促进陶瓷膜生长机制提供证据。     

电子束区熔定向凝固Nb基高温合金的组织和性能

研究了Nb-Si-Ti-Hf-Cr-Al-B-Y合金在电子束区熔炉上的定向凝固组织、室温断裂韧性和高温瞬时拉伸性能.合金的组织主要由Nb基固溶体(Nbss)、α-(Nb)5Si3和(Nb)3Si相组成.定向凝固后,初生Nbss枝晶以及Nbss α-(Nb)5Si3/(Nb)3Si层片状或棒状共晶团均沿着试棒轴线定向排列.当电子枪移动速率R=2.4 mm/min时,定向效果最好.定向凝固使合金在1250℃的拉伸强度及室温断裂韧性均显著提高.R=2.4 mm/min试棒的抗拉强度最高,达85.0 MPa,同时其室温断裂韧性也达到19.4 MPa·m1/2.     

环氧树脂辐射固化反应速率及速率常数的研究

研究了环氧树脂溶液的电子束辐射固化反应速率常数以及树脂特性对反应速率的影响.研究结果显示,辐射反应增长速率常数k_p和终止速率常数k_t在反应进行的不同阶段表现出不同的控制机制.环氧树脂的分子量及其分布,分子化学结构对辐射反应速率都有很大影响,反应速率大的树脂体系最终达到的反应程度也高.     

上游太阳风中高能电子向同步轨道区的传输

通常认为，同步轨道区的电子通量增加是由于磁暴或者上游太阳风高速流的扰动所引起．近来的观测表明，起源于太阳活动的行星际高能电子也是引起同步轨道电子通量增加的重要原因之一．Zhao等在研究2000年7月14日太阳剧烈活动时发现，同步轨道区相对论电子通量巨幅增加时没有观察到上游太阳风高速流的扰动，并且磁暴发生在电子通量事件之后．采用解析磁场模型和实际磁场模型(T96模型)模拟来自太阳的相对论电子在磁尾中的运动特性．计算结果表明，当行星际磁场南向时，进入到磁尾的行星际相对论电子可以从较远的磁尾区域运动到同步轨道区域．这一研究结果从理论上论证了起源于太阳活动的高能电子可以对同步轨道区相对论电子通量的增加产生重要的作用．     

卫星介质深层充电中的主要物理问题

卫星介质深层充电效应是诱发地球同步轨道卫星运行故障和异常的重要因素之一，通过计算机模拟对介质深层充电的时间常数、电场特征、以及屏蔽、介质厚度和接地方式对充电所致最大电场的影响等主要物理问题进行了详细的分析，并给出了初步的防护措施．     

Ionospheric response to the 17 March and 22 June 2015 geomagnetic storms over Wuhan region using GNSS-based tomographic technique

By using the data of GNSS (Global Navigation Satellite System) observation from Crustal Movement Observation Network of China (CMONOC), ionospheric electron density (IED) distributions reconstructed by using computerized ionospheric tomography (CIT) technique are used to investigate the ionospheric storm effects over Wuhan region during 17 March and 22 June 2015 geomagnetic storm periods. F-region critical frequency (foF2) at Wuhan ionosonde station shows an obvious decrease during recovery phase of the St. Patrick’s Day geomagnetic storm. Moreover, tomographic results present that the decrease in electron density begins at 12:00 UT on 17 March during the storm main phase. Also, foF2 shows a long-lasting negative storm effect during the recovery phase of the 22 June 2015 geomagnetic storm. Electron density chromatography presents the evident decrease during the storm day in accordance with the ionosonde observation. These ionospheric negative storm effects are probably associated with changes of chemical composition, PPEF and DDEF from high latitudes.     

Global characteristics of ionospheric electric fields and disturbances during the first hours of magnetic storms

The ionospheric plasma density can be significantly disturbed during magnetic storms. In the conventional scenario of ionospheric storms, the negative storm phases with plasma density decreases are caused by neutral composition changes, and the positive storm phases with plasma density increases are often related to atmospheric gravity waves. However, recent studies show that the global redistribution of the ionospheric plasma is dominated primarily by electric fields during the first hours of magnetic storms. In this paper, we present the measurements of ionospheric disturbances by the DMSP satellites and GPS network during the magnetic storm on 6 April 2000. The DMSP measurements include the F region ion velocity and density at the altitude of ∼840 km, and the GPS receiver network provides total electron content (TEC) measurements. The storm-time ionospheric disturbances show the following characteristics. The plasma density is deeply depleted in a latitudinal range of ∼20° over the equatorial region in the evening sector, and the depletions represent plasma bubbles. The ionospheric plasma density at middle latitudes (20°–40° magnetic latitudes) is significantly increased. The dayside TEC is increased simultaneously over a large latitudinal range. An enhanced TEC band forms in the afternoon sector, goes through the cusp region, and enters the polar cap. All the observed ionospheric disturbances occur within 1–5 h from the storm sudden commencement. The observations suggest that penetration electric fields play a major role in the rapid generation of equatorial plasma bubbles and the simultaneous increases of the dayside TEC within the first 2 h during the storm main phase. The ionospheric disturbances at later times may be caused by the combination of penetration electric fields and neutral wind dynamo process.     

Dynamics of global electron content in 1998–2005 derived from global GPS data and IRI modeling

We analyzed the dynamics of global electron content (GEC) for the period 1998–2005 and compared the estimated GEC with variations of the 10.7-cm solar radio emission and with and with GEC values obtained with IRI-2001. We found a strong resemblance between the curves’ shapes for the experimental and modeled GEC: strong semiannual variations are discernible in these series and both curves tend to increase the absolute GEC value during the period of maximum of solar activity. However, there are some significant distinctions, such as absence of 27-day fluctuations in the series of GEC computed by the IRI-2001. On the contrary, observational GEC reflects well dynamics of solar activity: 27-day variations of GEC are very similar to the ones of the index F10.7, but GEC undergoes a lagging of about of 30–60 h as compared to value of the F10.7 index. The relative amplitude of 27-day variations decreases from 8% at the rising and falling solar activity to 2% at the period of its maximum.