新型结构粘接材料对航空有机玻璃性能的影响

选用新型结构粘接材料中低温固化环氧结构胶膜J-351和改性丙烯酸酯液体胶胶黏剂SY-50s,表征胶黏剂对有机玻璃的粘接性能以及应力-溶剂银纹性能,并研究胶黏剂对有机玻璃力学性能的影响。结果表明:两种胶黏剂对有机玻璃具有良好的粘接性能,J-351抗应力溶剂银纹性能优于SY-50s;有机玻璃表面施胶后力学性能下降,与定向有机玻璃相比,浇注有机玻璃力学性能下降更为明显。通过对拉伸试样断口形貌分析发现,拉伸试样带有胶黏剂的一侧首先发生破坏。因SY-50s与有机玻璃界面结合紧密,导致带有SY-50s胶黏剂的有机玻璃力学性能下降程度较大;而J-351环氧胶膜与有机玻璃界面清晰,对有机玻璃力学性能影响相对较小。因胶黏剂对有机玻璃性能的影响,导致采用SY-50s胶黏剂粘接的试样边缘连接强度低于J-351胶黏剂粘接的试样,新型结构粘接材料J-351环氧胶膜在有机玻璃粘接中应用性能良好。     

基于一种新的均匀化实施方法的FRP刚度预测

基于一种新的渐近均匀化(AH)实施方法,预测并讨论了单向纤维增强复合材料(FRP)的宏观等效弹性性能及纤维排列方式对等效力学性能的影响。该方法方便地将有限元分析(FEA)软件作为一个工具箱使用,只需在单胞上施加简单位移周期边界条件开展静力学分析,即可经过简单计算得到等效弹性常数,相比传统均匀化实施方法显著降低了实施难度并简化了计算过程。通过对比不同数值方法的结果验证了该方法的有效性和精确性。数值结果表明:六边形排列下单向纤维增强复合材料呈现横观各向同性,而正方形排列下则呈现宏观正交各向异性,经过刚度平均化过程可得到横观各向异性材料性质,纤维体积含量对两种排列方式下材料等效弹性模量影响显著但有所差别。     

阻燃钛合金Ti40的热物理性能及力学性能

作为一种功能性钛合金,Ti40阻燃钛合金的热物理性能数据首次被报道。采用真空自耗电弧熔炼技术制备的Ti40合金铸锭成分均匀,利用热挤压开坯+包套保护锻造方法制备的板坯组织均匀。性能测试结果表明:Ti40合金的室温抗拉强度为950 MPa级,且在500℃下具有良好的热暴露性能、高温蠕变性能和高温持久性能。在室温到600℃范围内,合金的杨氏模量和剪切模量随着温度的升高呈线性下降,泊松比随着温度升高而缓慢增加;线性热膨胀曲线随着温度升高呈抛物线增加,平均线膨胀系数随着温度的升高呈线性增加。     

WC/C复合涂层海水环境的耐蚀性与摩擦性能

采用非平衡磁控溅射技术在304L不锈钢和单晶硅基底上沉积WC/C多层复合涂层,利用扫描电镜、Raman光谱仪、X射线衍射仪等研究WC/C复合涂层的微观结构,采用纳米压痕仪、划痕测试系统测试涂层的力学性能,利用电化学测试系统和摩擦磨损试验机分别研究涂层在人工配置的海水环境的耐蚀性能和摩擦性能。结果表明:WC/C复合涂层内含有较多类石墨sp2键结构,存在WC1-x相并镶嵌在非晶碳基质中。较之于304L不锈钢基底,WC/C复合涂层在海水环境中表现出更好的耐蚀性与更优异的摩擦适应性。     

CVD技术制备Ta/W层状复合材料

运用化学气相沉积(Chemical Vapor Deposition,CVD)技术制备了W体积分数分别10%,13%和18%的Ta/W两层层状复合材料,采用金相显微镜(OM)、扫描电镜(SEM)和室温拉伸实验对复合材料的性能进行分析。结果表明:运用CVD技术可以制备W体积分数不同,且密度优于理论密度99.4%的层状复合材料;复合材料中Ta,W层的晶粒均为柱状晶粒,离界面越近,晶粒越细;沉积态复合材料的力学性能优于纯CVD Ta和CVD W;1600℃×2 h的热处理后,复合材料的界面扩散层宽度显著增大,力学性能高于沉积态的力学性能,最高抗拉强度可达660 MPa。     

两种MCrAlY涂层/DD6合金的循环氧化和互扩散行为

在DD6单晶高温合金基体上,利用电子束物理气相沉积(EB-PVD)技术制备Ni Co Cr Al Y涂层,采用低压等离子喷涂(LPPS)技术制备Ni Co Cr Al YHf Si涂层,通过扫描电镜(SEM)、X射线能谱(EDS)、X射线衍射(XRD)、电子探针显微分析(EPMA)等手段研究了在1100℃下的热循环氧化和互扩散行为。结果表明,涂层显著提高了DD6基体的抗氧化能力,经100h的循环氧化后,涂层表面氧化层主要成分仍为α-Al2O3,依然发挥着较好的抗氧化保护作用。这两种涂层与基体之间形成了互扩散区(IDZ)和二次反应区(SRZ),IDZ和SRZ的厚度均随着循环氧化时间延长而增大;SRZ中析出的棒状与颗粒状的拓扑密堆相(TCP)含有W、Re、Mo等高熔点元素,其质量分数分别高达37.51%、14.22%和10.61%,TCP含量随着氧化时间而增多。活性元素Si、Hf对涂层中富Cr相和TGO的增长速率均有一定的抑制作用。     

先进的热防护方法及在飞行器的应用前景初探

随着航天技术的发展,飞行器的热环境面临着新的变化,对热防护提出了挑战。对各类主动热防护方式的原理、研究进展和应用现状进行了归纳总结。结合飞行器未来发展,提出了适应于未来应用的基于相变工质的对流冷却、自适应膜相变冷却和发汗冷却的系统性主动热防护方式。并以此为基础,提出了结合被动、半被动和主动热防护的飞行器全时域综合热管理思路。     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).     

Performance of a small and low-cost chamber to simulate lunar surface environment

The performance of a small and low-cost metal chamber built to simulate the pressure and temperature conditions of lunar surface was assessed and the results are presented. This chamber is intended for studying the physical properties of lunar surface and subsurface (using soil simulants) and also to validate the technology readiness of certain newly developed payloads planned for future lunar surface missions (Lander/Rover). It is possible to reach down to ∼10⁻⁷ Pa under specific conditions and maintain the temperature of the sample under investigation to lunar day and night temperatures. The designed system has been subjected to various tests to evaluate its performance and suitability for carrying out experiments in a simulated lunar environment.     

航天飞行器热防护涂层研究进展

近年来,新研航天飞行器气动热环境往往具有高焓、高热流密度和长时间加热等特点,这促使防热材料的研制朝着低密度、高抗烧蚀、优良隔热等性能的方向发展。受自身材料类型的限制,无论烧蚀型(树脂基)或非烧蚀型(陶瓷基)防热材料都可以通过对烧蚀表面进行涂层处理的手段达到弥补材料性能短板,提高使用性能的目的。本文试图梳理、总结国内外近年来热防护系统用涂层材料的发展状况,探讨各自的优势和缺点,并提出了针对树脂基复合材料热防护涂层可能趋势的推测。