固相含量对Al2O3料浆及瓷体性能的影响

研究了固相浓度对用于凝胶注成型的Al2O3料浆的粘度和流动性能的影响,并分析了由不同浓度的料浆制得的瓷体结构和性能与料浆浓度的关系.结果表明,控制合适的体浓度对于获得适合浇注的高性能料浆是必要的.同时由于料浆浓度会影响球磨效率和坯体密度,因此会对最终瓷体的质量有较大影响.在本文的实验条件下,料浆中固相的最佳含量为50vol%.     

Chandra imaging spectroscopy of the central region of AWM7

We report on the results of Chandra observations of the galaxy cluster AWM7. The ACIS image reveals new substructures with a spatial extent of more than 8″ (4 kpc at AWM7) near the cD galaxy center, represented by a hard sub-peak and a soft peak. These substructures suggest that a dynamical process related to the formation of the cD galaxy is now taking place. Inside the cluster core within a radius of 2′, annular spectra with every 10″ step are fitted well by single temperature models. The temperature gradually drops from 4.2 keV at a radius of 60 kpc (2′) to 1.8 keV at the cluster center. The radial abundance profile shows a gradient with a peak metallicity of 1.5 solar at a radius of about 15″ (7 kpc). A two-dimensional map shows two high metallicity blob-like regions, which may be the gas expelled from the cD galaxy.     

8mm波段二维综合孔径微波辐射计(BHU-2D)

介绍了二维综合孔径微波辐射计BHU-2D成像原理、系统构成及性能指标、校正方法、部分成像实验及其成像结果.BHU-2D工作在8mm波段,共有10个接收单元,天线阵列为T形结构,接收机为二次变频超外差结构,I/Q解调及相关运算采用了数字方式并通过软件实现,采用点辐射源校正方法及背景对消反演算法校正系统通道间不一致、相关偏置及混叠误差.目前,BHU-2D已经研制完成,并进行了系统测试及成像实验,得到了室内人工场景及人物场景的辐射亮温分布图像.     

光子计数中一种高速可程控参考电压鉴别器的设计

利用数字电位器和高速比较器MAX9012,设计了一种参考电压可程控用于光子计数的鉴别器,通过I~2C总线对数字电位器的阻值调节实现门限调整。实验表明该鉴别器输出信号质量良好,满足了设计要求。具有调整方便,精确,温度系数小等优点,为微弱光信号检测奠定了基础。     

利用F_(10.7)短期预报电离层F_0F_2

通过对电离层历史数据和太阳射电流量F10.7的回归分析,提出了一种单站电离层f0F2的短期预报方法,以F10.7的流动平均值fc为输入,以未米3天的f0F2为输出,分别利用中国地区8个台站的数据进行检验,分析不同太阳活动水平、季节以及地方时预报误差的分布特征.结果表明,该方法能有效地预测未来1～3天的f0F2.该方法还可应用于其他电离层参量的短期预报.     

Comparison of diurnal,seasonal and latitudinal effect of MUF VR and NmF2 VR during some solar cycle epochs

The diurnal and seasonal changes of the variability (VR) of Maximum Useable Frequency (MUF) are compared with those of peak electron density (NmF2) at Ibadan (7.4°N, 3.9°E, 6°S dip) in the African sector. Also compared is the latitudinal effect on both characteristics by combining data from Singapore (1.3°N, 103.8°E, 17.6°S dip) in the East Asian sector and Slough (51.5°N, 359.4°E, 66.5°S dip) in the European sector. MUF VR is found to be about half of NmF2 VR at all the hours and seasons and during the solar cycle epochs considered for the three stations. While nighttime MUF VR is greater in June Solstice and September Equinox during both low and moderate solar activities and in September Equinox and December Solstice during high solar activity, nighttime NmF2 VR is greater in June Solstice and September Equinox during high solar activity and greater at the equinoxes during low and moderate solar activities. This signifies a shift in nighttime MUF peak VR from the middle six months during low and moderate solar activities to the last half of the year during high solar activity. Daytime VR of both characteristics are not observed to show any seasonal variation. MUF VR and that of NmF2 are found to increase and decrease alternately with the Zurich sunspot number (Rz) for Ibadan and Singapore. For Slough, the VR of both characteristics increases with Rz during the first half of the day. It then increases and decreases alternately with Rz during the remaining hours of the day. While nighttime MUF VR decreases with latitude, just like nighttime NmF2 VR, no latitudinal effect is found for daytime VR of both characteristics.     

The response of African equatorial foF2 to geomagnetic storms: Comparison between observations and IRI-2007 predictions

This study examines the response of the African equatorial ionospheric foF2 to different levels of geomagnetic storms, using the foF2 hourly data for the year 1989 from Ouagadougou (12.4°N, 1.5°W, dip: 2.8°N). The study also compares the observed data for the selected storm periods with the latest IRI model (IRI-2007). The foF2 values (both observed and predicted) show typical features of daytime peak and post-midnight minimum peak. The response of the ionospheric foF2 over Ouagadougou to storms events, during the night-time and post-midnight hours indicates negative responses of the ionospheric foF2, while that of the daytime hours indicates positive responses. For the investigation on the variability of the observed foF2 with respect to IRI-2007 model, with the exception of the analysis of the 20–22, October, 1989 data, where a midday peak was also observed on the first day, this study reveals two characteristic daily foF2 variability peaks: post-midnight and evening peaks. In addition, for all the geomagnetic storms considered, the URSI and CCIR coefficients of the IRI-2007 model show reasonable correspondence with each other, except for some few discrepancies. For instance, the event of 28–30 August, 1989 shows comparatively higher variability for the URSI coefficient, and at the foF2 peak values, the event of 20–22 October, 1989 shows that the CCIR coefficient is more susceptible to foF2 variability than the URSI coefficient. This study is aimed at providing African inputs for the future improvement of the IRI model.     

基于五阶容积-二阶平滑变结构滤波算法的捷联惯导系统初始对准技术

为了改进捷联惯导系统大方位失准角初始对准情况下的方位失准角对准精度和稳定性问题,提出了一种组合对准方法。该方法将Kalman滤波对准模型与罗经对准模型相结合构建了一种组合对准机制,并在此模型基础上提出了基于非线性滤波和鲁棒滤波的五阶容积-二阶平滑变结构滤波算法,将五阶容积-二阶平滑变结构滤波算法与组合对准机制相结合,从而实现大方位失准角的初始对准。仿真结果表明,五阶容积-二阶平滑变结构滤波对准方法得到的方位失准角对准精度明显优于常见的几种对准方法,且其对准结果的重现性更高。因此,提出的五阶容积-二阶平滑变结构滤波算法能够很好地适用于大方位失准角的初始对准。     

TiAl合金与ZrB2-SiC陶瓷非晶钎焊接头组织与力学性能

采用Cu_(41.83)Ti_(30.21)Zr_(19.76)Ni_(8.19)(at.%)非晶钎料对Ti48Al2Cr2Nb合金与Zr B_2-Si C陶瓷进行真空钎焊连接,通过扫描电镜、能谱分析、X射线衍射以及万能试验机对接头的微观组织和力学性能进行研究。结果表明:Ti Al合金与Zr B_2-Si C陶瓷钎焊接头的界面结构为Ti Al/Ti_2Al/Al Cu Ti/(Ti,Zr)_2(Cu,Ni)+Ti B+Ti Cu/Ti_5Si_3/ZS。当钎焊温度为910℃,随着保温时间的延长,靠近Zr B_2-Si C一侧反应层宽度逐渐增大,接头中弥散分部的Ti B和Ti Cu聚集长大。接头剪切强度随着保温时间的延长先上升后降低,当钎焊温度为910℃,保温20 min时,接头剪切强度最大,为187 MPa,通过对各工艺的接头断口分析,发现接头均断裂在陶瓷侧,断裂方式为脆性断裂。