三种不锈钢材料抗固体颗粒冲蚀性能研究

采用增压气流固体颗粒冲蚀试验方法研究1Cr11Ni2W2Mo2V、1Cr12Ni2WMoVNb、1Cr17Ni2三种不锈钢材料的抗冲蚀性能。结果表明,三种不锈钢材料在固体颗粒冲击下均发生冲蚀磨损,30°稳定冲蚀速率大于90°稳定冲蚀速率。在相同冲蚀条件下,三种不锈钢材料抗冲蚀性能1Cr17Ni2>1Cr12Ni2W2MoVNb>1Cr11Ni2W2MoV,即1Cr17Ni2不锈钢抗冲蚀性能最好。     

固体火箭发动机喷管喉部凝相颗粒粒度分布实验

设计了一种新的收集固体火箭发动机喷管凝相颗粒的实验装置,针对典型的HTPB复合推进剂,开展了喷管喉部凝相颗粒的收集实验和粒度分析,研究了燃烧室压强和收敛角度对喷管喉部颗粒粒度分布的影响规律。研究结果表明,喷管喉部的凝相颗粒在0.27～50μm之间都有颗粒存在,凝相颗粒主要集中在0.3～15μm之间,粒径大于15μm的颗粒较少;燃烧室压强对颗粒粒径有较大影响,随着燃烧室压强的升高,凝相颗粒粒径变小,粒度分布更为集中;燃烧室压强相同的条件下,收敛角度对喷管喉部的凝相颗粒粒度分布影响较小。     

空间环境下的有机热控涂层

本文综述了国外在空间有机热控涂层领域中的研究工作和试验，着重分析了空间极端环境中紫外光辐照和原子氧侵蚀这两大因素对有机热控涂层的影响。     

环形扩压叶栅流动非定常控制方法的PIV研究

利用合成射流发生器对于一台环形扩压叶栅进行了流动主动控制的探索,发现适当的非定常激励方式可以使得环形叶栅的总压损失明显减小。同时利用二维粒子图像测速仪(ParticleImageVelocimetry,简称PIV)测量了扩压叶片绕流流场。获得了不同攻角下,在不同的激励频率和激励强度下,流场结构的变化。结果表明非定常激励可以使叶片绕流流场结构发生明显变化。在合适的非定常激励下,扩压叶片的叶背分离流动得到明显抑制,尾迹漩涡的强度和尾迹宽度均明显减小,流线分布比无非定常激励时更加平滑。实验结果能够与环形叶栅时均总压损失的变化相吻合。对于这一非定常控制方法的作用机理也进行了初步的分析。      

颗粒冲刷对C/C材料烧蚀影响的实验研究

为研究粒子直接撞击模式下C/C材料的烧蚀形貌及性能,丰富C/C材料烧蚀研究,开展了粒子侵蚀实验.利用扫描电镜和三维微观成像等测量手段进行微观烧蚀形貌的研究,结果表明颗粒冲刷条件下由于粒子的直接撞击,侵蚀区域出现小凹坑,但轴棒纤维突出,轴棒表面出现大小不同的凹坑,部分单丝从基体中断裂,形成微观锥形孔穴形貌,径向纤维束部分区域出现孔和开槽,整体形貌不再连续一致;未侵蚀部位的微观形貌和烧蚀试验中的喉部形貌一致,单丝呈现笋尖状.     

某典型振动条件下发动机点火试验研究

以某飞行器主动段飞行故障中屡屡出现低频振动现象为背景,通过设计振动点火试验台,模拟空中飞行的振动环境,进行了低频振动条件下的发动机点火试验,研究了该低频振动对固体发动机药柱结构完整性、发动机内弹道性能以及燃烧室内绝热层烧蚀性能等的影响,研究结果初步证明,飞行过程中出现的低频振动不破坏发动机药柱的结构完整性,对发动机主要内弹道性能也不产生较大影响,但对振动方向上的推进剂燃速与绝热层的烧蚀率产生一定影响。该项研究可为相关的工程问题提供依据。     

固体粒子在压缩机叶栅内的部分沉积模型研究

针对轴流压缩机叶栅内固体微粒沉积的问题,发展了新的粒子沉积模型(部分沉积模型)。采用此模型和普遍采用的完全沉积模型进行了计算,计算结果表明两种模型对叶栅前缘处的粒子沉积影响明显。采用部分沉积模型时,叶片前缘处不会出现短时间内不合实际的大量沉积现象,而表现为一种比较均匀的粒子沉积。     

一种用于解决粒子滤波粒子退化现象的重要性重采样算法的研究

粒子滤波通过蒙特卡罗模拟来实现递推贝叶斯估计,在非线性非高斯系统中体现出良好的特性;但粒子滤波存在粒子退化现象的缺陷,针对这一问题,提出一种新的重采样算法,即分区重采样算法,其主要思想是根据多项式重采样与分层重采样算法的特点,把随机数区间划分成若干个区,每个区内的随机数任意排列,而区与区之间按升序排列。与目前常用的其他重采样算法相比,该方法提高了粒子滤波的平均性能,仿真实验验证了该算法的有效性和实用性。     

MESSENGER: Exploring Mercury’s Magnetosphere

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury offers our first opportunity to explore this planet’s miniature magnetosphere since the brief flybys of Mariner 10. Mercury’s magnetosphere is unique in many respects. The magnetosphere of Mercury is among the smallest in the solar system; its magnetic field typically stands off the solar wind only ∼1000 to 2000 km above the surface. For this reason there are no closed drift paths for energetic particles and, hence, no radiation belts. Magnetic reconnection at the dayside magnetopause may erode the subsolar magnetosphere, allowing solar wind ions to impact directly the regolith. Inductive currents in Mercury’s interior may act to modify the solar wind interaction by resisting changes due to solar wind pressure variations. Indeed, observations of these induction effects may be an important source of information on the state of Mercury’s interior. In addition, Mercury’s magnetosphere is the only one with its defining magnetic flux tubes rooted beneath the solid surface as opposed to an atmosphere with a conductive ionospheric layer. This lack of an ionosphere is probably the underlying reason for the brevity of the very intense, but short-lived, ∼1–2 min, substorm-like energetic particle events observed by Mariner 10 during its first traversal of Mercury’s magnetic tail. Because of Mercury’s proximity to the sun, 0.3–0.5 AU, this magnetosphere experiences the most extreme driving forces in the solar system. All of these factors are expected to produce complicated interactions involving the exchange and recycling of neutrals and ions among the solar wind, magnetosphere, and regolith. The electrodynamics of Mercury’s magnetosphere are expected to be equally complex, with strong forcing by the solar wind, magnetic reconnection, and pick-up of planetary ions all playing roles in the generation of field-aligned electric currents. However, these field-aligned currents do not close in an ionosphere, but in some other manner. In addition to the insights into magnetospheric physics offered by study of the solar wind–Mercury system, quantitative specification of the “external” magnetic field generated by magnetospheric currents is necessary for accurate determination of the strength and multi-polar decomposition of Mercury’s intrinsic magnetic field. MESSENGER’s highly capable instrumentation and broad orbital coverage will greatly advance our understanding of both the origin of Mercury’s magnetic field and the acceleration of charged particles in small magnetospheres. In this article, we review what is known about Mercury’s magnetosphere and describe the MESSENGER science team’s strategy for obtaining answers to the outstanding science questions surrounding the interaction of the solar wind with Mercury and its small, but dynamic, magnetosphere.     

喷丸强化对AISI420不锈钢固体粒子冲蚀行为的影响

研究了喷丸强化(SP)对AISI 420马氏体不锈钢抗同体粒子冲蚀(SPE)行为的影响.探讨了喷丸引起的表面残余压应力,表面粗糙度增大和表面加工硬化等三因素对SPE抗力的作用机制.结果表明:SP处理对AISI 420不锈钢在30°攻角下的SPE抗力无明显影响,但却降低了该钢在90°攻角下的SPE抗力.SP处理后进行表面抛光,则使该钢在两种攻角下的SPE抗力均得以提高.SP三因素对SPE抗力的作用机制主要有:表面粗糙化增大了试样表面对冲蚀粒子的有效暴露面积,因而降低了不锈钢在两种攻角下的SPE抗力;表面残余压应力能够有效抑制疲劳裂纹萌生和早期扩展,因而能有效提高AISI 420不锈钢的SPE抗力,特别是对90°垂直冲击条件下SPE抗力的提高作用更为明显;表面加工硬化提高了材料表面的微犁削抗力,因而对提高AISI 420钢在30°攻角下的SPE抗力有贡献,但是表面加工硬化层的抗多冲疲劳性能差,却不利于AISI 420钢在90°攻角下抗SPE性能的改善.