CM2程控稳流电源电流稳定性的自动化测试

文章将零磁通电流互感器技术应用到了大电流稳定性测试中,从而解决了CM2航天器磁环境模拟设备中的程控稳流电源输出电流稳定性测试的难题,稳定性指标高达10-5/8h。文章简述了零磁通电流互感器技术的基本原理,介绍了采用零磁通电流互感器技术对CM2程控稳流电源电流稳定性进行自动测试的方法,分析了影响大电流稳定性现场自动测试的因素并提出了相应解决方案。     

基于遗传优化算法的微通道紫铜热交换器扩散连接工艺

基于遗传优化算法,进行了T2紫铜同种材料扩散连接工艺研究。采用正交试验方法,结合BP神经网络和多目标遗传算法,以扩散连接时的温度、压力、保温时间为输入变量,以扩散连接后的试样焊合率和变形量为输出变量,对扩散连接工艺参数进行优化,并实施相应的扩散连接验证试验。结果表明:T2紫铜合适的扩散连接工艺参数为:温度780℃、压力7. 5 MPa、保温时间120 min,此条件下焊合率可达95. 26%,变形量为0. 166 mm。采用此工艺参数进行微通道热交换器零件制造,厚度方向变形量0. 162 mm,经超声C扫描后连接情况良好,经耐压防漏检测后满足密封性及设计要求。     

基于微观图像及内聚力模型的复合材料裂纹扩展模拟

为研究材料微观结构及晶界强度对材料力学性能的影响,在晶界处引入内聚力单元模型,模拟晶间破坏过程。以ZrB_2-SiC复合材料为研究对象,将其扫描的微观结构图片进行矢量化处理,并导入ABAQUS有限元软件中建立模型,同时在其晶界处,设置内聚力单元模拟晶界破坏过程。通过改变Zr B2与Si C相界面强度,得到了晶界及材料不均匀对材料应力分布及裂纹扩展的影响。结果表明,由于晶界的存在,材料内部出现应力分布不均匀现象并产生应力集中。随着晶界强度的改变,裂纹起始位置及扩展方向发生改变,且裂纹沿低强度的界面进行扩展。随着ZrB_2-SiC界面强度增大,材料的强度提高,拉伸模量不变。     

弹性体运载火箭建模及控制器设计

考虑运载火箭飞行过程中的弹性振动特性,对运载火箭进行全量动力学建模以及控制器设计。首先将运载火箭考虑为一维梁模型并建立全量动力学模型,分别引入自适应滤波姿态控制算法和H_2范数鲁棒增益调度控制算法设计控制器。仿真结果表明:在考虑舵机非线性情况下两种控制方法均能够满足精度要求,在具有较大外部扰动情况下,鲁棒增益调度控制算法相较于自适应滤波算法具有较强的鲁棒性。     

Beam-Park-Experiment-1/2000 with TIRA

A monostatic 24-h debris observation campaign (BPE-1/2000) has been prepared and conducted using FGAN's TIRA L-Band system. Based on experiences from previous Beam-park experiments a similar largely automated data processing is applied on an extended range window of 300–2000km. More than 1500 detections are encountered, 471 of them are verified as being real objects in Low-Earth-Orbit (LEO). PROOF's observation forecasting of catalogued objects is evaluated against the observed objects, and the difficulties obtaining radar cross-sections (RCSs) and object sizes from Beam-park experiments are discussed. Sidelobe detections are identified by using background information like two-line element (TLE) sets and/or catalogued RCSs.In comparison with previous experiments, the statistics show similarities confirming the concept of Beam-park experiments for space debris observations, despite the snapshot character of 24-h experiments. The comparison with MASTER/PROOF'99 and ORDEM2000 leads to a reasonable agreement between models and observations.     

2219铝合金搅拌摩擦焊缝Al2Cu相聚集行为特征分析

对2219C10S状态铝合金进行搅拌摩擦焊接试验,发现焊缝中存在聚集物的异常聚集现象,聚集相在X光检测中显示为亮白色聚集物,主要形态分为团块状、线状和指状三种,聚集相处焊缝的力学性能与无聚集相焊缝的力学性能基本相同。各形态聚集相的分布位置受搅拌头焊接影响区域的不同而不同,团块状聚集相主要存在于焊核中心或偏焊缝上表面位置处,线状和指状聚集相主要存在于焊核中心或偏焊缝根部位置处。对异常聚集相进行能谱分析知,聚集相主要组成元素为Al和Cu,原子百分比近似为2∶1,确定聚集相主要成分为Al2Cu。对聚集相的成因进行分析认为,聚集相的产生主要受搅拌摩擦焊接热输入及搅拌头机械搅拌作用的影响,在焊接过程中,塑态软化金属中的Al2Cu在填补搅拌针后方空腔的过程中出现了聚集行为,随着塑态金属的凝固,聚集行为开始变得缓慢并结束。     

骨特异性转录因子Runx2对抗空间骨丢失效应的初步研究

为了构建稳定过表达Runx2 (骨特异性转录因子)的C2C12 (小鼠成肌细胞)和MG63 (前成骨细胞)细胞株, 并用于研究Runx2在对抗空间骨丢失效应中的作用. 利用实时定量聚合酶链式反应鉴定Runx2下游基因I型胶原、碱性磷酸酶表达情况, 在二维回转器中培养稳定细胞株, 通过定量聚合酶链式反应,观察在模拟失重效应下Runx2基因对其下游基因表达的影响. 结果表明, 通过筛选获得稳定转染的C2C12-Runx2和MG63-Runx2细胞株, 经鉴定都能过表达Runx2. 转染后的细胞 I 型胶原和碱性磷酸酶mRNA表达增高. 回转组与对照组相比, MG63, C2C12-Runx2, MG63-Runx2细胞的I型胶原和碱性磷酸酶mRNA表达降低, 但在模拟失重效应下, 转染细胞中I型胶原和碱性磷酸酶的mRNA表达下降程度明显低于未转染细胞株. 所构建的C2C12-Runx2和MG63-Runx2细胞株比较稳定, 并证实Runx2能部分对抗失重引起的成骨特异性分子的降低.     

Midlatitude ionospheric F2-layer response to eruptive solar events-caused geomagnetic disturbances over Hungary during the maximum of the solar cycle 24: A case study

In our study we analyze and compare the response and behavior of the ionospheric F2 and of the sporadic E-layer during three strong (i.e., Dst?<??100nT) individual geomagnetic storms from years 2012, 2013 and 2015, winter time period. The data was provided by the state-of the art digital ionosonde of the Széchenyi István Geophysical Observatory located at midlatitude, Nagycenk, Hungary (IAGA code: NCK, geomagnetic latitude: 46.17° geomagnetic longitude: 98.85°). The local time of the sudden commencement (SC) was used to characterize the type of the ionospheric storm (after Mendillo and Narvaez, 2010). This way two regular positive phase (RPP) ionospheric storms and one no-positive phase (NPP) storm have been analyzed. In all three cases a significant increase in electron density of the foF2 layer can be observed at dawn/early morning (around 6:00 UT, 07:00 LT). Also we can observe the fade-out of the ionospheric layers at night during the geomagnetically disturbed time periods. Our results suggest that the fade-out effect is not connected to the occurrence of the sporadic E-layers.     

Estimating the spin axis orientation of the Echostar-2 box-wing geosynchronous satellite

For the first time, the spin axis orientation of an inactive box-wing geosynchronous satellite has been estimated from ground-based optical photometric observations of Echostar-2’s specular reflections. Recent photometric light curves obtained of Echostar-2 over four years suggest that unusually bright and brief specular reflections were occurring twice within an observed spin period. These bright and brief specular reflections suggested two satellite surfaces with surface normals separated by approximately 180°. The geometry between the satellite, the Sun, and the observing location at the time of each of the brightest observed reflections, was used to estimate Echostar-2’s equatorial spin axis orientation coordinates. When considering prograde and retrograde rotation, Echostar-2’s spin axis orientation was estimated to have been located within 30° of either equatorial coordinate pole. Echostar-2’s spin axis was observed to have moved approximately 180° in right ascension, within a time span of six months, suggesting a roughly one year spin axis precession period about the satellite’s angular momentum vector.