Ionospheric behavior of the F2 peak parameters foF2 and hmF2 at Hainan and comparisons with IRI model predictions

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with hourly time interval resolution for the diurnal variation, obtained with DPS-4 digisonde observations at Hainan (19.4°N, 109.0°E) are used to study the low latitude ionospheric variation behavior. The observational results are compared with the International Reference Ionospheric Model (IRI) predictions. The time period coverage of the data used for the present study is from March 2002 to February 2005. Our present study showed that: (1) In general, IRI predictions using CCIR and URSI coefficients follow well the diurnal and seasonal variation patterns of the experimental values of foF2. However, CCIR foF2 and URSI foF2 IRI predictions systematically underestimate the observed results during most time period of the day, with the percentage difference ΔfoF2 (%) values changing between about −5% and −25%, whereas for a few hours around pre-sunrise, the IRI predictions generally overestimate the observational ones with ΔfoF2 (%) sometimes reaching as large as ∼30%. The agreement between the IRI results and the observational ones is better for the year 2002 than for the other years. The best agreement between the IRI results and the observational ones is obtained in summer when using URSI coefficients, with the seasonal average values of ΔfoF2 (%) being within the limits of ±10%. (2) In general, the IRI predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the observational results. However, when using the measured M(3000)F2 as input, the diurnal variation pattern of hmF2 given by IRI2001 has a much better agreement with the observational one with the detailed fine structures including the pre-sunrise and post-sunset peaks reproduced reasonably well. The agreement between the IRI predicted hmF2 values using CCIR M(30,000)F2 option and the observational ones is worst for the afternoon to post-midnight hours for the high solar activity year 2002. During daytime hours the agreement between the hmF2 values obtained with CCIR M(30,000)F2 option and the observational ones is best for summer season. The discrepancy between the observational hmF2 and that obtained with CCIR M(30,000)F2 option stem from the CCIR M(3000)F2 model, which does not produce the small scale structures observed in the measured M(3000)F2.     

The effective temperatures of O-type stars from UV spectroscopy

We present an analysis of high resolution spectra in the far-UV – UV range (∼905–2000 Å) with non-LTE, spherical, hydrodynamical, line-blanketed models, of three O-type Galactic stars, and derive their photospheric and wind parameters. These data extend previously analyzed samples and fill a gap in spectral type coverage. The combined sample confirms a revised (downward) T_eff scale with respect to canonical calibrations, as found in our previous works from UV and optical spectra, and in recent works by other authors.     

真实气体流动的相似规律

本文从具有化学反应的NS方程出发导出了真实气体流动的相似律,分别给出了高温空气非平衡流、平衡流和冻结流的相似参数。文中还讨论了航天飞机轨道器各种Mach数范围内的真实气体流动的相似参数和实验模拟问题。     

Influence of the 27-day solar flux variations on the ionosphere parameters measured at Irkutsk in 2003–2005

We present an investigation of the influence of the 27-day solar flux variations, caused by solar rotation, on the ionosphere parameters such as the F2 layer critical frequency (foF2) and the total electron content (TEC). Our observational data were obtained with the Irkutsk Digisonde (DPS-4) located at 52.3 North and 104.3 East during the period from 2003 to 2005. In addition, we use TEC data from the Global Ionosphere Maps (GIM) based on Global Positioning System (GPS) satellites. The solar radiation flux at a wavelength of 10.7 cm (F10.7 index) is used as an index characterizing the solar activity level. A good correlation between observed ionosphere parameters and solar activity variations is found especially in autumn-to-winter season. We estimate the impact of the 27-day solar flux variations on the day-to-day variability and determine the time delay of the ionosphere response.     

新型航空润滑油油膜拖动力计算研究

在自制的试验装置上测量了新型航空润滑油油膜拖动力;给出了高剪切率弹流润滑下的Ery-ing特征应力、极限剪切应力、剪切弹性模量的新型航空油流变参数拟合计算式;确定了该油本构方程;建立了该油油膜拖动力计算式, 并进行了试验验证.试验结果表明:该油在试验条件下表现为粘弹性;拖动力的理论计算值与试验测量值相当吻合.给出的拖动力计算方法可用于指导润滑分析领域的工程计算.      

不确定性系统鲁棒H∞/H2混合控制在航空发动机中的应用

将结构参数不确定性问题引入到参数化的一般 H∞ 控制器中 ,并考虑 H2 性能指标 ,提出了 1种被控系统中存在结构参数不确定性的混合 H∞ /H2 控制器的设计方法 ,给出了相应问题求解的充分必要条件 ,问题的解归结为求解 3个 Riccati方程。设计的控制器在某型双转子涡喷发动机气动热力学非线性模型上进行了仿真验证     

软件可靠性参数研究

确定软件可靠性的定量要求是软件可靠性工程面临的首要工作内容.本文讨论了软件可靠性定量要求的意义、特点、描述,对一般的软件可靠性参数进行了分析,提出了结合武器装备特点的软件可靠性参数,并给出了软件可靠性参数的选取及其指标确定应考虑的因素.      

复杂薄壁、薄板类零件高速加工技术初探

从加工方法,加工参数,工装夹具等方面对薄壁、薄板类零件的加工进行深入探讨,有效地解决了薄壁、薄板类零件的加工,为今后进行此类零件的加工进行了有益的技术储备。     

Weibull分布参数估计值对细节疲劳额定强度的影响

将新材料、新工艺应用于民机结构设计时,细节疲劳额定强度（DFR）法仍是重要的评估方法。根据新型铝合金疲劳试验数据,全面分析了Weibull分布形状参数对DFR计算参数的影响;分析标准S-N曲线斜度参数对DFR的影响时,应考虑可靠性寿命的变化,采用低可靠度寿命计算曲线斜度参数可降低Weibull分布形状参数的影响;比较了采用不同分布参数估计值与传统上采用波音公司给定值进行DFR计算的差异。结果表明,对于通过符合性检验的试验数据,使用不同Weibull分布的参数估计值计算得到的DFR都大于按传统方法（用波音公司给定值）的计算结果,其中,三参数Weibull分布计算的DFR最大,至少增加10%以上。