高温长期时效对一种镍基单晶合金拉伸和持久性能的影响

研究了高温长期时效对一种镍基单晶合金在室温条件下瞬时拉伸强度和在950℃/240MPa条件下持久性能的影响。结果表明:1000℃短期时效100h,合金室温拉伸强度σb与屈服强度σ0.2与时效前相比没有明显变化,时效超过500h后σb和σ0.2开始显著下降,时效超过1000h后,σb和σ0.2随时效时间延长下降幅度减小;短期时效100h和500h样品在950℃/240MPa条件下的持久寿命大幅度降低,延伸率快速上升,时效时间超过1000h后,持久寿命的下降幅度减小,合金的持久寿命与延伸率均趋于稳定。长期时效后γ'相形貌改变及γ/γ'相界面高密度位错网的破坏是时效后合金室温及高温持久性能持续降低的主要原因。     

相对论性离子束（环束）流引起的电磁不稳定性

在相对论性框架下，研究了冷离子流产生的右旋共振模，非共振模电磁不稳定性的特征结果表明，非共振模不稳定性增长率受离子流初始参数影响较大，而右旋共振模的增长率则受离子流初始参数影响较小。此结果可应用于太阳高能离子流通过低日冕区和地球磁层辐射带俘获的高能质子情形。     

Cluster observations showing the indication of the formation of a modified-two-stream instability in the geomagnetic tail

This study presents several observations of the Cluster spacecraft on September 24, 2003 around 15:10 UT, which show necessary prerequisites and consequences for the formation of the so-called modified-two-stream instability (MTSI). Theoretical studies suggest that the plasma is MTSI unstable if (1) a relative drift of electrons and ions is present, which exceeds the Alfvèn speed, and (2) this relative drift or current is in the cross-field direction. As consequences of the formation of a MTSI one expects to observe (1) a field-aligned electron beam, (2) heating of the plasma, and (3) an enhancement in the B-wave spectrum at frequencies in the range of the lower-hybrid-frequency (LHF). In this study we use prime parameter data of the CIS and PEACE instruments onboard the Cluster spacecraft to verify the drift velocities of ions and electrons, FGM data to calculate the expected LHF and Alfvèn velocity, and the direction of the current. The B-wave spectrum is recorded by the STAFF instrument of Cluster. Finally, a field aligned beam of electrons is observed by 3D measurements of the IES instrument of the RAPID unit. Observations are verified using a theoretical model showing the build-up of a MTSI under the given circumstances.     

Shock Wave Interaction with the Magnetopause

The magnetopause is in continuous motion and shock waves and impulsive acceleration events can occur. As an example, we show that the interaction of an interplanetary shock with the bow shock can generate a shock wave that after passing through the magnetosheath can interact with the magnetopause. In fluid dynamics, when a shock wave encounters a fluid discontinuity, the interface may become unstable and form bubbles and spikes. We consider this Richtmyer-Meshkov instability in magnetohydrodynamics. At the dayside magnetopause, the instability tends to be stabilized by the magnetic field. However, the shock wave interaction can initiate magnetic field reconnection for the southward IMF, which may be important in strong interplanetary shock events. This revised version was published online in August 2006 with corrections to the Cover Date.     

新型工具电极制造方法

用电火花加工复杂形状模腔的关键之一是工具电极的制造。为了解决一般电极材料价高，复杂型腔难以加工等问题，通过试验研究，推出了一种以石膏和塑料为基本材料，采用非金属电镀工艺制造工具电极的新方法。     

细晶铸造对K418合金拉伸性能的影响

测试了不同温度下细晶铸造和普通铸造Ｋ４１８合金的拉伸性能。结果表明，细晶铸造明显改善了合金的极限位伸强度和屈服强度，室温和６００℃的合金拉伸强度和晶粒平均直径符合Ｈａｌｌ－Ｐｅｔｃｈ关系。     

同轴离心式喷嘴热声不稳定性递归分析

为获得同轴离心式喷嘴燃烧动力学特性，开展了喷注单元稳定性试验研究。试验中燃料流量不变，随氧化剂流量增加，热声系统依次经历了燃烧噪声状态、阵发状态和准周期振荡状态。采用递归方法对实验结果进行分析。首先，利用交互信息法和虚假最邻近法分别求解最优延迟时间和嵌入维数，获得了典型工况下的相空间轨迹图。其次，递归图分析表明系统出现了第II类阵发现象，意味着系统发生了亚临界Hopf分叉，与实验结果一致。最后，递归量化分析表明，确定率可以将阵发状态和准周期振荡状态与燃烧噪声状态区分出来，并可以对热声振荡进行预报。     

Daytime VHF amplitude scintillations recorded at an Indian low-latitude station,Waltair (17.7°N, 83.3°E) during 1997–2003

In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased.     

Two-stream instability generation in the lunar ionosphere

The Two-stream Instability (TSI) generation is studied analytically in the lunar ionosphere. The TSI is a tiny perturbation in the electron plasma density, due to which an electric field grows with time and this growth is facilitated by the electron plasma in the background. In lunar ionosphere, the TSI comes into existence when the solar wind interacts unhindered with the tenuous lunar electron plasma in the surface bound exosphere. In this study, the conditions which allow the TSI to form and the subsequent instability growth with time i.e. the growth factor, is estimated. Initially, the threshold condition for the TSI to take place is determined. Thereafter, the solar wind and lunar plasma parameter contribution to trigger TSI is investigated along with the effect of these parameters in the evolution of TSI. The plasma TSI evolution with the passage of time is also depicted in phase space diagram with Particle-In-Cell simulations.     

碳纤维复合材料基体改性/铜网组合雷击防护性能的研究

传统碳纤维复合材料（CFRP）树脂基体导电性差易遭受雷击损伤,本文使用石墨烯-镀镍碳纤维粉作为导电填料,对树脂基体进行电导率改性,并在表面铺设铜网,进行模拟雷电流冲击试验,检验基体改性/铜网组合雷击防护效果。试验结果表明,树脂基体改性后CFRP层压板在0°、90°纤维方向及厚度方向电导率分别为1.1571×10⁴、1.0871×10⁴、204.2 S/m,分别提高1.54倍、1.16倍、433.47倍。200 kA模拟雷电流A波冲击下,无防护试件雷击附着后明火燃烧,次生效应持续,而单一铜网防护和组合防护则能抑制次生效应;无防护表面最大损伤直径14.62 cm,此能量下铜网被击穿,单一铜网防护表面最大损伤直径19.05 cm,而组合防护表面最大损伤直径8.93 cm,下降53.12%;相比无防护试件,单一铜网和组合防护内部损伤面积分别下降66.2%和96.7%。单一铜网击穿后,树脂烧蚀后产生汽化反冲,增大损伤铜网脱落面积;组合防护铜网击穿后,改性树脂迅速导走电流,减小铜网脱落和内部烧蚀面积。