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采用室温拉伸力学性能测试、X射线织构检测、EBSD分析等方法,对比研究了10 mm与2 mm厚度2A55超高强铝锂合金板材的平面各向异性,阐释热处理制度与晶粒组织对板材各向异性的影响。结果表明,热处理后板材屈服强度最高的取向为轧向(0°)与横向(90°);Taylor因子能较好地预测固溶态与T6态时效板材屈服强度的各向异性,织构是平面各向异性的重要原因;厚板更高含量的织构与长条状的晶粒形貌导致其各向异性强于薄板;时效热处理使10 mm厚度板材各向异性减弱,使2 mm厚度薄板各向异性增强;T3态、T8态板材的各向异性分别强于T4态、T6态,时效前的预变形增强了板材的平面各向异性。 相似文献
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板料异向性对拉深成形的影响 总被引:2,自引:0,他引:2
推导出了异向性板料在两向应力状态下的塑性方程,分析了厚向异向性和面内异向性对拉深成形的影响,提出了利用异向性现象来提高拉深工艺水平的途径。 相似文献
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V.G. Grigoryev S.A. StarodubsevP.A. Krivoshapkin A.N. PrikhodkoA.G. Yegorov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):943-946
The method has been developed to calculate galactic cosmic ray anisotropy parameters by using on-line data of the neutron monitor 24-NM-64 and muon telescope at the Yakutsk station. The preliminary analysis shows that characteristic changes in the anisotropy parameters caused by the first spherical harmonics of cosmic ray angular distribution are observed 1–2 days before the onset of the most part of large-scale geophysical disturbances on the Earth. There is reason to believe that the attraction of data of geophysical observations of other kinds will allow to develop the forecast methods for the arrival of large-scale interplanetary disturbances at the Earth. 相似文献
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运用波动理论,讨论背景为各向异性、不均匀的随机起伏电离层中高频电波的传播和散射问题,给出了电离层不均匀体散射引起的反射回波波场的起伏,并在垂测条件下计算了接收波场的相位与振幅起伏的谱分布。 相似文献
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应用二维三维量磁流体动力学方程组模拟,数值研究了压力各向异性等离子体周期多重电流片的演化,发现在β<<1时,微弱的各向异性仅仅使电流片中磁场重联的速度加快,而当β≈1(即热压与磁压相当时,微弱的垂直各向异性不仅大大加速了磁场重联的速度,还使重联位置发生显著变化。初始反对称的磁场重联位形逐步转化为对称的磁场位形,进而再演化为与初始反相的反对称磁场位形,场向各向异性和强的垂直各向异性都导致不稳定性增长率成倍增加。但在场各向异下磁场位形基本不变,只在电流片中心出现不规则扰动,同样参数下向向异性等离子体多重电流片中磁场重联形成的磁岛比各向同性多层电流要小。 相似文献
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Francis F. Badavi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The completion of the international space station (ISS) in 2011 has provided the space research community an ideal proving ground for future long duration human activities in space. Ionizing radiation measurements in ISS form the ideal tool for the validation of radiation environmental models, nuclear transport codes and nuclear reaction cross sections. Indeed, prior measurements on the space transportation system (STS; shuttle) provided vital information impacting both the environmental models and the nuclear transport code developments by indicating the need for an improved dynamic model of the low Earth orbit (LEO) trapped environment. Additional studies using thermo-luminescent detector (TLD), tissue equivalent proportional counter (TEPC) area monitors, and computer aided design (CAD) model of earlier ISS configurations, confirmed STS observations that, as input, computational dosimetry requires an environmental model with dynamic and directional (anisotropic) behavior, as well as an accurate six degree of freedom (DOF) definition of the vehicle attitude and orientation along the orbit of ISS. 相似文献
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M. Verigin D. Vignes D. Crider J. Slavin M. Acua G. Kotova A. Remizov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,33(12):2222-2227
The origin of the anisotropy in the shape of the Martian obstacle and bow shock is analyzed using Mars Global Surveyor observations. The influence of MHD or ion pick-up effects on Martian obstacle position was to be small found, however, localized Martian crustal magnetization increases the thickness of the downstream planetary magnetotail by 500–1000 km in agreement with earlier Phobos 2 observations. A new analytical model is presented for Martian obstacle shape variation for different solar wind ram pressure. Elongation of the Martian BS cross-section in the direction perpendicular to IMF was confirmed while the shift of this cross section in the +Y direction of Martian interplanetary medium reference frame was discovered. The shift of BS cross section in the direction of interplanetary electric field was not revealed thus not conforming the idea that mass-loading play some role in BS control. 相似文献