MoS2自润滑复合材料的空间摩擦学性能研究

在模拟空间原子氧与高真空条件下,分别对微米MoS₂、MoS₂纳米球与MoS₂-IC 3种复合润滑材料的摩擦学性能进行了测试。结果显示MoS2纳米球复合材料具有最优的抗磨性能,MoS₂-IC复合材料的抗磨性能次之,微米MoS₂复合材料最差。3种复合材料的减摩性能相差较小,MoS₂纳米球复合材料的摩擦系数仅比其他两种复合材料略低。MoS₂-IC具有较高的化学活性,在摩擦过程中发生转移并形成转移润滑膜,从而具有较优的抗磨性能,MoS₂纳米球优异的摩擦学性能与其独特的球形封闭结构相关。     

真空条件下冷板传热分析

当两个或多个试件在同一空间环境模拟器内进行热真空试验时,减少互相之间热影响的有效措施就是用液氮冷板将两个试件隔开。文章根据节点网络法的原理建立了冷板热模型,利用Thermal Desktop热分析软件进行了数值分析计算,得出了冷板管路的流量分布及管路内流体的温度分布,并对不同的翅片结构在相同工况下的温度分布进行了分析。通过冷板结构对热流分布影响的分析结果为今后冷板的设计和利用提供了依据。     

探讨反舰导弹突防编队防御阵的航路规划

针对舰群编队强大的反导能力,建立描述反舰导弹威胁源的广义数字高程模型,探讨以提高生存力和突防能力为目标的航路规划对策。     

HJ-1B卫星红外多光谱相机星上定标精度分析

介绍了"环境一号"B(HJ-1B)卫星红外多光谱相机在轨辐射定标的目的以及星上定标的原理,分析了星上定标算法的精度。利用星上零级数据对星上定标系统的测控精度和工作稳定性进行研究,并在此基础上分析了定标数据的处理精度。HJ-1B卫星发射以来共对红外相机热红外通道进行了7次星上定标,为了监测定标系统的精度变化,文章利用MODIS-31、32通道辐亮度对HJ-1B卫星上定标系统精度进行检验,考虑MODIS传感器本身定标的不确定度恒定,分析结果表明自HJ-1B卫星发射以来星上定标系统相对精度发生了衰减。     

超空泡推进发动机燃料能量特性比较

超空泡鱼雷实现高航速、远航程的有效途径之一是携带高能燃料--金属粉末燃料或金属基燃料.为了说明这些燃料的能量特性,结合水冲压发动机的工作特点,采用最小自由能法对各种燃料进行热力计算,并进一步进行能量比较.分析结果表明,铝粉是较为理想的燃料,镁基燃料不可取.热力计算和能量比较法可为燃料的选择提供依据,进而指导水冲压发动机的设计和试验.     

基于电动力绳系的航天器离轨方式初步研究

为寻找适合近地轨道上使用的航天器离轨技术,文章对目前各种离轨策略的基本原理及优缺点作了分析与对比,重点对电动力绳系离轨装置进行了深入研究,建立了数学模型,推导出离轨时间预估公式,对离轨的过程进行了数学仿真,结果证实电动力阻力能使近地轨道上航天器的轨道高度迅速降低,电动力绳系离轨策略具有很高的工程实用性。     

真空热试验热电偶测温参考点分析改进

热电偶测温系统是真空热试验中最常用的温度测量系统,温度参考点是热电偶测温系统的重要组成部分。文章分析了热电偶温度参考点的各项技术要求,为参考点结构设计、热设计、电装工艺等提供了依据;同时结合温度参考点的现状,为简化操作,降低使用风险,提出了一种优化改进结构方案,并进行了热分析计算以及试验验证,结果表明该方案完全满足参考点各项技术要求。     

Sensor calibration impacts on dust detection based on MODIS and VIIRS thermal emissive bands

Dust detection using remotely sensed measurements has been one of the challenging problems encountered by atmospheric scientists. MODerate Resolution Imaging Spectroradiometer (MODIS) on the Terra (T) and Aqua (A) platforms have been a versatile sensor for well over 21 and 18 years respectively, and have been extremely useful in the retrieval of aerosol information over the entire globe. The MODIS radiances from the Level 1B in general are expected to be within 5% accuracy in the reflective wavelengths and within 1% in the thermal emissive wavelengths. In this paper, we evaluate the sensitivity of previously developed dust detection technique based on thermal emissive wavelengths, which correspond to MODIS bands 20, 29, 31, and 32 respectively. The Thermal Emissive Dust Index (TEDI) performed very comparably to the traditional Aerosol Optical Thickness (AOT) retrievals by MODIS reflective channels. Since the MODIS Thermal Emissive Bands (TEB) are well calibrated on-orbit using a BlackBody (BB) source, the calibration of these long wave infrared bands is quite robust. As A-MODIS continues to perform well beyond its designed lifetime of 6 years, the instrument has undergone various levels of degradation during its mission time. As a consequence, it is imperative to check the impacts of calibration on the higher-level retrievals. In this paper, we rigorously analyze the sensitivity of TEDI due to the impact of calibration by the afore-mentioned TEB. The perturbation of the dominant (linear) calibration term demonstrated the following: first, there was a correlation in the sensitivity of the TEDI due to the uncertainty in the linear calibration term. Based on a perturbation in the linear calibration term for all aforementioned bands over a range of ±5% yielded the TEDI sensitivity to vary from approximately ?3.2% to about ?3.6%. When considering the uncertainty in each individual band significant changes were observed. The least change was observed for the perturbation in the calibration of band 20 with the TEDI sensitivity and the largest sensitivity in TEDI was observed in the perturbation of band 31 calibration. Thus, in the case of TEDI, noticeable sensitivity due to calibration uncertainty was observed in bands 29, 31, and 32, reiterating the importance of the TEB calibration in these bands. Also, the dust detection scheme based on A-MODIS was successfully transferred to the follow-on sensors such as Suomi (SNPP) and NOAA 20 (N20) VIIRS. The results presented in this paper would be extremely helpful in understanding impacts of calibration on the higher-level products for both current and future missions based on the MODIS heritage. Finally, the work also identifies the importance of radiometric fidelity in maintaining the accuracy of the dust detection. Results presented will show drastic improvement of the Saharan dust detection after the reduction of the electronic crosstalk in the 8.5 µm channel of T-MODIS.