共查询到17条相似文献,搜索用时 203 毫秒
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综述了我层隔热材料的隔热原理、隔热性能表征方法、组成、性能,以及在航天器上的应用。通过选用不同的反射屏和间隔物可得到一系列常温、中温和高温使用的多层隔热材料。对于以双面镀铝聚酯薄膜为反射屏的常温多层材料,采用疏松纤维、网、泡沫塑料的间隔物,均有良好的隔热性能,其当量热导率可达10^-4W/m.K的量级。 相似文献
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将纳米多孔结构和多层反射屏引入柔性隔热毡中,设计出一种具有多层反射结构的柔性纳米隔热材料,并结合材料的微观结构对其隔热机理进行了分析.结果表明:多层反射屏抑制了材料的红外辐射传热量,纳米多孔结构降低了气体导热和对流传热,有效地提高了材料的隔热性能. 相似文献
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为了厘清在轨GEO(Geosynchronous Earth Orbit,地球同步轨道)卫星不时出现异常的原因,提高卫星执行任务的可靠性,首先从机理上介绍了空间环境中的地球辐射带及高能电子的情况,引出GEO卫星所处恶劣空间环境的现实;其次基于我国SEPC(Space Environment Prediction Center,国家空间环境预报中心)以及NSMC(National Satellite Meteorological Center,国家卫星气象中心)的空间环境月报资料,结合某GEO环境业务卫星故障的实际数据,经统计归纳,分析得出了地球辐射带中的高能电子是导致GEO卫星发生故障的主要原因;最后按照事例技术分析、常规按需预报和特殊情况下的实时预报等3个层次对高能电子预报方法进行了初步探讨。通过分析可以看出,为提高卫星完成任务的可靠性、降低长期管理风险,需要加强GEO卫星所处空间环境高能电子的预报工作。 相似文献
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李鹏%程惠尔%秦文波 《宇航材料工艺》2006,36(Z1):18-22
在分析了空间多层打孔隔热材料中导热和辐射的复合传热问题的基础上,提出了空间多层打孔隔热材料反射屏温度计算的模型以及内部辐射数值分析模型.利用该模型对不同几何、物理参数下的对象进行模拟计算,通过对计算结果的分析,明确作为几何参数的层密度和层数以及作为表面特性参数的黑度和打孔率对材料热性能的影响.该热性能的研究对提高空间多层打孔隔热材料的隔热效果,实现材料的优化设计具有积极的指导意义. 相似文献
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为满足多电飞机(MEA)的大功率用电需求,系统工作电压需要进一步提高,而较高电压会增加相关部件的绝缘失效风险。面向多电飞机特定工作场景和参数,搭建了模拟飞机电作动器中的绕组间绝缘故障测试平台,开展了1 kHz范围内的局部放电(PD)大量重复实验,研究了特定电压幅值、正弦波和方波脉冲波形下局部放电幅值、放电重复率和放电相位等统计特征,并计算评估了不同频率值下多电飞机中的局部放电行为。实验结果表明:在设定频域范围内,方波脉冲下的起始放电电压(PDIV)都低于正弦,方波脉冲波形对绝缘影响更大;随着频率升高,放电幅值逐渐降低,但放电重复率几乎呈线性增长;放电时刻集中于上升沿/下降沿末端。以50 Hz作为对比基准频率,1 kHz时的放电幅值降低80%,而放电重复率增加11.92倍,较高频率下多次累积的小幅值击穿成为威胁绝缘失效的主要原因。计算分析认为高频下空间电荷场强变化导致的放电延迟时间减少和周期数目增加分别导致局部放电脉冲幅值降低和放电重复率增加。本实验结果有助于针对多电飞机电气系统和相关装备开展针对性绝缘测试和评估,并有望为多电飞机向大功率高电压方向的设计提供参考和借鉴。 相似文献
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航天器介质盘环结构内带电特性三维仿真分析 总被引:2,自引:1,他引:1
针对航天器内特定结构的内带电(IDC)问题,以航天器典型复杂介质结构——太阳帆板驱动机构介质盘环为研究对象,开展了地球同步轨道恶劣充电环境(Flumic3)下介质内带电三维仿真分析。通过Geant4实现电荷输运模拟,根据电荷守恒定律数值计算得到电场,在此基础上,研究了屏蔽厚度对介质内带电的影响规律,提出了根据屏蔽厚度调整入射电子能谱能量下限以提高计算效率的方法。仿真结果表明,盘环结构内带电最严重部位是盘环最外圈上层介质与金属导电环接触的上边沿;增加屏蔽厚度可以减缓充电风险,但是随着温度降低,屏蔽效果会随之减弱。在地球同步轨道恶劣充电环境(Flumic3)下,当温度低至183 K时,由于辐射诱导电导率成为总电导率的主导部分,从而增大屏蔽的同时也会降低介质电导率,导致即使3 mm铝屏蔽下仍可能出现接近107 V/m的场强峰值。 相似文献
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Auroral investigations by means of rockets 总被引:1,自引:0,他引:1
W. Pfister 《Space Science Reviews》1967,7(5-6):642-688
A survey of rocket experiments undertaken to study auroral zone events includes summary information about instrumentation and results in the field of energetic electrons and protons, of charged particle densities, of optical observations, of magnetic and electric fields, of bremsstrahlung X-rays, of thermal electrons, and of production rates. Other auroral investigations except those involving rockets have been largely ignored. 相似文献
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F. S. Mozer C. A. Cattell M. K. Hudson R. L. Lysak M. Temerin R. B. Torbert 《Space Science Reviews》1980,27(2):155-213
Several previous and new S3-3 satellite results on DC electric fields, field-aligned currents, and waves are described, interpreted theoretically, and applied to the understanding of auroral particle acceleration at altitudes below 8000 km. These results include the existence of two spatial scale sizes (less than 0.1 degree and a few degrees invariant latitude) in both the perpendicular and parallel electric fields; the predominance of S-shaped rather than V-shaped equipotential contours on both spatial saales; the correlated presence of field-aligned currents, low frequency wave turbulence, coherent ion cyclotron wave emissions and accelerated upmoving ions and downgoing electrons; intense waves inside electrostatic shocks and important wave-particle interactions therein; correlations of field-aligned currents with magnetospheric boundaries that are determined by convection electric field measurements; electron acceleration producing discrete auroral arcs in the smaller scale fields and producing inverted-V events in the larger scale fields; ion and electron acceleration due to both wave-particle interactions and the parallel electric fields. Further analyses of acceleration mechanisms and energetics are presented.Also Department of Physics. 相似文献
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L. P. Block 《Space Science Reviews》1967,7(2-3):198-210
The coupling between the ionosphere and the outer magnetosphere depends on the topology of the geomagnetic field. Some aspects of the closed and open magnetospheric models are briefly discussed.The assumption that the geomagnetic field lines are equipotentials is critisized both on observational and on theoretical grounds. Measurements of H Doppler profiles, of precipitating particles above the ionosphere, and of charged particle densities in the magnetosphere indicate the existence of electric fields, E\\, parallel with the magnetic field.Two different models of E\\ are considered. Both models violate the condition of frozen-in magnetic fields. In one of them there are occasional transient electric field impulses along the field lines which cause precipitation splashes. The other model invokes electrostatic fields which vanish occasionally due to instabilities. This gives rise to precipitation splashes of about equal numbers of ions and electrons.The latter model seems to be favoured by known satellite data concerning the pitch angle distributions of electrons above the ionosphere.It is suggested that electric fields in space should be measured by satellites and rockets. Expected values of the fields in different regions of space are given. 相似文献