航空发动机分布式控制系统指数稳定性分析

建立具有时延与数据包丢失的航空发动机分布式控制系统模型,模型为一类异步动态系统,基于Lyapunov第二法和线性矩阵不等式方法推导了系统的指数稳定性判定定理,根据该判据可以得到分布式控制系统的指数稳定意义下的状态反馈控制律,数字仿真说明了该判据的有效性.      

ZrB2 / C 复合材料的微观结构与高温氧化机理

在碳基体材料中添加ZrB2抗烧蚀组元,经过热压固化成型、炭化处理制得改性碳基复合材料。经过1 500℃静态抗氧化实验后,对比发现添加ZrB2的复合材料抗氧化能力得到提高。通过SEM观察发现ZrB2在高温下被氧化形成致密保护层,能有效阻止氧气扩散进入碳基体。通过热力学计算进一步分析了碳基复合材料在制备和高温氧化过程中的化学反应机理。     

FY-2C星用户利用站分系统

介绍了风云二号(FY-2)气象卫星地面应用系统中用户利用站(USS)的构成和特点.给出了其中规模用户利用站(MDUS)、低速率用户利用站(LRUS)和数据收集平台(DCP)的配置、特点、主要功能及部分硬件的技术指标.     

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%.     

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.