基于自由胀形的弯曲管材变形行为

随着制造业轻量化的发展趋势,复杂弯曲异形充液成形管件的应用日益广泛。为了更好地研究弯曲异形复杂管件在充液成形过程中的变形规律,进行可靠的工艺设计。本文通过结合薄膜理论和塑性变形理论对弯曲管件在自由胀形状态下的应力应变进行了理论解析,并通过有限元(FE)分析对理论计算模型进行了验证。FE分析结果与理论模型基本吻合。同时分析了管材在绕弯过程的硬化行为,并探索了在不同的弯曲硬化状态下弯曲管材在自由胀形过程下的破裂位置的规律,并且用实验进行了验证,实验结果与FE分析结果吻合。     

高强度铝合金7804-T6板材温拉伸本构方程

通过在293~573K的温度范围内和应变速率为0.0006~0.06s^-1下对高强度铝合金7B04-T6薄板进行温拉伸试验,研究了高强度铝合金温拉伸性能,以及该合金在升温条件下流变应力与变形温度、应变速率之间的关系,可以得出结论:合金的流动应力随温度的升高而降低,随应变速率的升高而升高;延伸率随变形温度的升高而增大,随应变速率的增大而减小,并基于Fields and Backofen方程建立了该型铝合金在温拉伸时应力-应变模型.     

大型网状天线展开过程温度及展开时机分析

大型网状天线在轨展开过程复杂,风险大。反射器在展开过程中的温度影响展开动力与碳纤维管件抗弯能力,是反射器展开安全的关键因素。通过测试得到反射器展开动力的传动效率、桁架管件抗弯能力随温度变化规律,即-65℃时管件抗弯能力最好,而传动效率随温度升高而提高。通过建立大型网状天线有限元模型与节点矩阵转换算法,模拟展开臂与反射器的展开过程,对管件与T型铰链在轨温度变化规律进行分析,确定最佳展开时机,降低展开过程中展开动力不足、管件强度过载等风险。分析结果表明：布置在地球静止轨道卫星东舱板的大型网状天线展开时机为6:00~9:00时,管件抗弯能力最强;展开时机为4:00时,T型铰链展开动力传动效率最高。     

同位素热源高温-冲击复合环境试验

为了考察深空探测器同位素热源模拟样品在高温–冲击复合环境下的环境可靠性,研制了一套高温–冲击复合环境试验装置。该装置由温度加载系统、冲击试验系统、带有热防护功能的夹具和控制系统等组成。该装置可完成室温约500℃热载荷加载。利用该试验装置对同位素热源模拟样品进行了500℃、5 000次的高温–冲击复合环境试验考核,获得了产品温升响应曲线、冲击波形图等相关试验信息。试验结果表明该试验装置能够进行高温–冲击复合环境试验。     

直齿锥齿轮齿根应力的有限元分析

根据展成法加工的直齿圆锥齿轮的齿面和齿根过渡曲面方程，建立了轮齿弯曲强度计算的精确的有限元模型，用柔度矩阵法确定接触线上的载荷分布，进行计算齿根应力，根据上述方法，编制了相应的微机程序，本程序可一次求解多个啮合位置的载荷分布、轮齿变形和齿根应力，并可计算双齿对工作时各对齿上的载荷、变形和应力，便于对直齿锥齿轮弯曲强度进行全面分析，算例表明，本文结果与其它文献结果吻合良好。     

分体对开式高低温发生装置研究

介绍了一种分体对开式高低温发生装置,并详细叙述了其结构组成,测试结果表明高低温发生装置温度范围为-80℃~400℃,温度偏差为±2℃,温度均匀度为2℃,该装置可作为专用实验设备用于力传感器高低温环境下的校准。     

分体对开式高低温发生装置研究

介绍了一种分体对开式高低温发生装置，并详细叙述了其结构组成，测试结果表明高低温发生装置温度范围为-80℃~400℃，温度偏差为±2℃，温度均匀度为2℃，该装置可作为专用实验设备用于力传感器高低温环境下的校准。     

蜂窝夹芯挖补修理结构弯曲性能研究

从试验及有限元2个方面对复合材料蜂窝夹芯挖补修理结构的弯曲性能进行研究。通过3点弯曲试验对无损及修理件弯曲性能进行测试,试验结果表明,蜂窝夹芯结构破坏模式为典型的蜂窝剪切破坏,修理件相比于无损件弯曲强度恢复率为110%,修理后结构弯曲刚度也略高于无损件;基于试验结果建立三维有限元模型对蜂窝夹芯修理结构的弯曲性能进行研究,通过用户自定义子程序VUSDFLD编写Hashin失效准则、基于应力的Besant失效准则,实现复合材料面板及蜂窝芯子2种材料的损伤起始及演化。数值模型得到的破坏模式、破坏载荷及弯曲刚度均与试验结果吻合得较好;改变有限元模型参数,研究损伤直径及补片厚度对修理后弯曲性能影响,结果表明,随着损伤直径从30~70 mm逐渐增加,修理件强度先增加后减小,并在损伤直径为50 mm时取得最大值,此外,补片厚度为1~2.5 mm时弯曲强度恢复率高于100%;本文为复合材料蜂窝夹芯结构的修理设计提供了可靠的数值模拟方法。      

紧缩场反射面板热变形的适应性调整

随着季节的变化,紧缩场反射面板的温度在15~25℃之间变化.热变形量往往超出允许的误差.利用Marc有限元软件,分析了紧缩场在温度、重力和反向力等作用下的变形.针对变形最严重的工况下的变形,用最小二乘法对变形后的数据进行二次多项式曲线拟合,得出与变形后的反射面相一致的新的母线方程和焦距.仿真结果表明调整馈源位置,能够适合于面板焦距的变化.     

用双边切缝试样的高温蠕变裂纹扩展分析

对双边切缝试样切缝根部萌生裂纹进行了有效SIF分析,并用于1Cr18Ni9Ti不锈钢板材的高温蠕变裂纹扩展试验,在所试验的温度T(570～650℃)和应力σ(15.3～16.9kg/mm~2)范围内,试验数据表明:稳态蠕变裂纹扩展是一个热激活过程,相应的综合参量S=S(T,σ,K_(1eff))有效地控制了稳态蠕变裂纹扩展率da/dt。     

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

绳驱动并联机器人张力约束工作空间分析

绳驱动三自由度机器人可以实现空间的自由转动.由于绳索只可拉伸不可压缩的单向特性,研究驱动绳索张力对机器人的控制具有重要意义.运用几何和矩阵的方法可以分析绳索的张力分配情况;在存在张力约束的条件下,提出张力系数作为评价张力分配优劣状况的指标,通过计算可以得到张力系数分布图,从而对机器人工作空间有直观的认识,进而提出有效的张力优化算法;通过对最小预紧力影响因素及选取方法的讨论,可以得到动态最小预紧力实时计算公式,保证绳索时刻处于张紧状态;通过样机的力检测系统张力反馈的实验可以验证理论推导.通过对以上几部分的分析和研究,可以对四绳驱动三自由度机器人的张力问题有综合全面的认识.      

火卫二地形地貌探测综述

火卫二（Deimos）是火星自然卫星之一，研究人员利用火星探测器对其地形地貌开展了大量研究。首先对火卫二的基本参数及起源假说进行了介绍，进而全面梳理了与火卫二相关的航天探测活动，重点对地形地貌探测活动进行了详细介绍，并对围绕火卫二地形地貌的研究成果进行了归纳分析，结果表明火卫二表面分布有撞击坑、风化层、明亮的反射物质及块状物，并存在物质移动。最后针对火卫二探测不全面的情况，给出了中国关于火卫二探测的建议。     

测试有效性对软件可靠性验证测试量的影响

针对传统软件可靠性验证测试方法均不考虑软件测试性可能会对验证测试用例数量产生影响的现状,提出一种引入测试有效性对软件可靠性验证测试最小量进行改进的方法.分析了软件测试性的定义及其对软件可靠性测试集合的影响,提出软件测试有效性的概念.比较了考虑测试有效性前后软件可靠性验证测试集合在数量上的差异,证明经典统计方法和无先验知识的Bayesian统计推断方法确定的均为假定测试有效性为零情况下的保守估计.提出结合测试有效性的验证测试量的量化表示模型和验证测试方案的改进方法,基于统计故障注入的原理,提出测试有效性的定量评估方法,最后通过示例给出定量评估过程和方法.      

H2 and H∞ control options for the combined attitude and thermal control system (CATCS)

The combined attitude and thermal control system (CATCS) combines the conventional attitude control and thermal control subsystems. Its principle is based on circulating a heat conducting fluid inside a closed duct wielding the excess onboard heat in order to produce the attitude control torques. Previously only the proportional-integral (PI) controller has been tested for CATCS. In this paper two other control options for CATCS were designed based on the H₂ and H_∞ control methods to improve the attitude control performance of a small satellite. The control gain matrix with the minimum cost function is obtained by solving the Riccati equation and fed back to the system in order to achieve the system’s performance. The designed controllers can efficiently control the roll, pitch and yaw satellite attitudes. Simulations for the two techniques were carried out using Matlab and Simulink for ideal and non-ideal system models. Results show that the H₂ controller has a better attitude control performance over the H_∞ controller and PI controller itself.     

From Titan’s tholins to Titan’s aerosols: Isotopic study and chemical evolution at Titan’s surface

In the present work, we focused on the possible isotopic fractionation of carbon during the processes involved in the formation of Titan’s tholins. We present the first results obtained on the ¹²C/¹³C isotopic ratios measured on Titan’s tholins synthesized in laboratory with cold plasma discharges. Measurements of isotopic ratio ¹²C/¹³C, done both on tholins and on the initial gas mixture (N₂:CH₄ (98:2)) used to produce them, do not show any evident deficit or enrichment in ¹³C relatively to ¹²C in the synthesized tholins, compared to the initial gas mixture. This observation allows to go further in the analyses of the ACP experiment data, including part of the Cassini–Huygens mission.     

Hemisphere-coupled modeling of nighttime medium-scale traveling ionospheric disturbances

Nighttime medium-scale traveling ionospheric disturbances (MSTIDs), which have tilted frontal structures in the midlatitude ionosphere, are investigated by the midlatitude ionosphere electrodynamics coupling (MIECO) model in this study. It has been proposed that the electrodynamic coupling between the E and F regions plays an important role in generating MSTIDs within a few hours. An intriguing aspect of MSTIDs is that they were simultaneously observed at magnetic conjugate locations in the Northern and Southern Hemispheres. In order to study the hemisphere-coupled electrodynamics, the MIECO model has been upgraded to consist of two simulation domains for both hemispheres in which the electrostatic potential is solved by considering electrodynamics in both hemispheres. The simultaneous occurrence of MSTIDs at the magnetic conjugate stations has clearly been reproduced when the F-region neutral wind satisfies the unstable condition in both hemispheres and a sporadic-E layer is given only at the Northern (summer) Hemisphere. Even if the unstable condition is satisfied in the summer hemisphere, an unfavorable F-region neutral wind in the winter hemisphere largely suppresses the growth of MSTIDs in both hemispheres.     

Nostoc sphaeroides Kützing,an excellent candidate producer for CELSS

Some phytoplankton can be regarded as possible candidates in the establishment of Controlled Ecological Life Support System (CELSS) for some intrinsic characteristics, the first characteristic is that they should grow rapidly, secondly, they should be able to endure some stress factors and develop some corresponding adaptive strategies; also it is very important that they could provide food rich in nutritious protein and vitamins for the crew; the last but not the least is they can also fulfill the other main functions of CELSS, including supplying oxygen, removing carbon dioxide and recycling the metabolic waste. According to these characteristics, Nostoc sphaeroides, a potential healthy food in China, was selected as the potential producer in CELSS. It was found that the oxygen average evolution rate of this algae is about 150 μmol O₂ mg⁻¹ h⁻¹, and the size of them are ranged from 2 to 20 mm. Also it can be cultured with high population density, which indicated that the potential productivity of Nostoc sphaeroides is higher than other algae in limited volume. We measured the nutrient contents of the cyanobacterium and concluded it was a good food for the crew. Based on above advantages, Nostoc sphaeroides was assumed to a suitable phytoplankton for the establishment of Controlled Ecological Life Support System. We plan to develop suitable bioreactor with the cyanobacterium for supplying oxygen and food in future space missions.     

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.     

Attempt to identify a source mechanism of Mercury’s sodium exosphere by a spectrometer using Fabry–Perot etalon

The Mercury’s Sodium Atmosphere Spectral Imager (MSASI) on BepiColombo (BC) will address a range of fundamental scientific questions pertaining to Mercury’s exosphere. The measurements will provide new information on regolith–exosphere–magnetosphere coupling as well as new understanding of the dynamics governing the exosphere bounded by the planetary surface, the solar wind and interplanetary space. MSASI is a high-dispersion visible spectrometer working in the spectral range around sodium D2 emission (589 nm). A tandem Fabry–Perot etalon is used to achieve a compact design. We presents a design of the spectral analyzer using Fabry–Perot interferometer. We conclude that: (1) The MSASI optical design is practical and can be implemented without new or critical technology developments; (2) The thermally-tuned etalon design is based on concepts, designs and materials that have good space heritage.