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Ayodeji Ashidi Joseph Ojo Adekunle Adediji Oludare Ajewole 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(5):1612-1622
Existing amplitude scintillation prediction models often perform less satisfactorily when deployed outside the regions where they were formulated. This necessitates the need to evaluate the performance of scintillation models developed in one region using data data from other regions while documenting their relative errors. Due to its variation with elevation angle, frequency, other link parameters and meteorological factors, we employed three years (January 2016 to December 2018) of concurrently measured satellite radio beacons and tropospheric weather parameters to develop a location-based amplitude scintillation prediction model over the Earth-space path of Akure (7.17oN, 5.18oE), South-western Nigeria. The satellite beacon measurement used Tektronix Y400 NetTek Analyzer at 1 s integration time while meteorological parameters, namely; temperature, pressure and relative humidity were measured using Davis Vantage Vue weather station at 1 min integration time. Comparative study of the model’s performance with nine (9) existing scintillation prediction models indicates that the best and worst performing models, in terms of root mean square error (RMSE), are the Statistical Temperature and Refractivity (STN) and direct physical and statistical prediction (DPSP) models with values 11.48 and 51.03 respectively. Also, worst month analysis indicates that April, with respective enhancement and fade values of 0.88 and 0.90 dB for 0.01% exceedance, is the overall worst calendar month for amplitude scintillation. 相似文献
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本文主要研究了碳纤维织物增强复合材料的纤维体积含量V_f对开孔层压板的抗拉强度σ、断裂伸长率ε的影响。采用T300碳纤维平纹织物为增强材料,经树脂传递模塑法(RTM工艺)复合而成T300/环氧TDE-85层压板,用岛津强力测试机进行拉伸性能测试。 相似文献
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基于Fokker 27飞机过载-超越数曲线族的严重超越数包线选取 总被引:3,自引:0,他引:3
以Fokker 27机群的过载-超越数曲线族为基础,建立了严重谱对应的严重超越数包线的获取方法。首先对外场使用的Fokker 27飞机机群的过载-超越数曲线进行筛选,得到59架飞机的过载-超越数曲线,采用线性累积损伤理论计算得到59架飞机每次飞行的损伤;假定机群载荷损伤服从对数正态分布,以严重谱下安全寿命满足机群寿命可靠度要求为准则,给出了严重谱的损伤程度。其次,采用对数正态分布描述指定过载下超越数的分布特性,外推得到满足损伤要求的严重超越数包线及对应的概率要求。结果表明,Fokker 27飞机严重过载-超越数曲线包线对应的超越数增量为1.117倍标准差。 相似文献
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QAR超限事件飞行操作风险诊断方法 总被引:4,自引:2,他引:2
利用某机型的快速存取记录器(QAR,Quick Access Record)数据,对飞机着陆阶段出现的某一QAR超限事件,选取飞机下降率、俯仰角等飞行员综合操作指标在无线电高度20 feet(1 feet=0.304 8 m)的数值以及20~0 feet之间的变化率,分析由这些指标构成的"空间"中发生该QAR超限事件的"高风险子空间".对同一机场同一机型的多个航班数据初步分析得到,着陆总重大于62 t、着陆温度小于32℃时,正常样本与QAR超限样本占比接近,表明环境因素并非该样本空间中QAR超限事件的主要因素.为进一步诊断,以超限事件发生率最大化为目标,以划分空间中包含的样本满足一定数量标准为约束,建立数学模型,并以黄金分割法为基础设计了算法,找出这些操作指标上区间的边界值,以此诊断可能触发该QAR超限事件的高风险区域,为飞行员模拟机针对性训练提供指导. 相似文献
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O.E. Ehinlafa O.A. Falaiye J.O. Adeniyi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
This is to investigate ways of improving the Equatorial F2-layer peak heights estimated from M(3000)F2 ionosonde data measured using the Ionospheric Prediction Service (IPS-42) sounder at Ouagadougou, Burkina Faso (Latitude +12.4°N, Longitude +1.5°W, Dip latitude +5.9°N) during a low solar activity year (1995). For this purpose, we have compared the observed hmF2 (hmF2obs) deduced using an algorithm from scaled virtual heights of quiet day ionograms and the predicted hmF2 values which is given by the IRI 2007 model (hmF2IRI 2007) with the ionosonde measured M(3000)F2 estimation of the hmF2 values (hmF2est) respectively. The correlation coefficients R2 for all the seasons were found to range from 0.259 to 0.692 for hmF2obs values, while it ranges from 0.551 to 0.875 for the hmF2IRI 2007 values. During the nighttime, estimated hmF2 (hmF2est) was found to be positively correlated with the hmF2obs values by the post-sunset peak representation which is also represented by the hmF2IRI 2007 values. We also investigated the validity of the hmF2est values by finding the percentage deviations when compared with the hmF2obs and hmF2IRI 2007. 相似文献
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基于模糊关联分类器的民机超限事件诊断方法 总被引:2,自引:0,他引:2
现有的民用飞机超限事件智能诊断模型大多属于“黑盒”模型,不利于分析超限事件发生的原因.为此提出了一种基于模糊关联分类器(FAC,Fuzzy Associative Classifier)的民用飞机超限事件诊断方法.该方法抽取发生超限事件时对应的QAR(Quick Access Recorder)参数快照取值,采用模糊C均值(FCM,Fuzzy C-Means)聚类算法对抽取的QAR参数取值模糊预处理,然后基于Apriori算法生成模糊关联分类规则库,并由遗传算法对其进行裁剪,结合模糊分类推理方法形成FAC.采用B737-800实际样本数据进行了验证.实验结果表明,所提出的FAC能有效诊断超限事件,FAC识别超限事件的错误率与最小二乘支持向量机(LS-SVM,Least Squares Support Vector Machine)模型相当,但其解释性方面优于LS-SVM. 相似文献
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Muhammad Sadiq Zulfiqar Ahmad 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A statistical comparison has been made between gravity field parameters derived from different global geopotential models (GGMs) and observed gravity anomalies, gravimetric geoid and GPS-Leveling data. The motivation behind this study is the selection of best possible global geopotential model that best matches statistically with the local observed data in Pakistan. This will facilitate in decreasing the load on observed data for the development of regional gravimetric geoid in remove-compute-restore technique when used in the Stokes’s integral for computation of the residual part. It is observed that combined geopotential models such as EGM96 and PGM200A, EIGEN-GL04C and EIGEN-CG03C reflect the better match in the total spectral range of gravity and GPS-Leveling data. Results of the precise local geoid model also indicate similar characteristics. A very-high-degree model “EGM2008” (degree/order 2160) exhibits relatively superior statistical fit with observed ground data in Pakistan region. For satellite-only models an increasing trend in the standard deviation can be seen with maximum of about ∼4 m in difference between GPS-Leveling and corresponding GGM’s geoid with increase in the order from 50 to 120 and then it decreases afterwards. However, for the EIGEN-CHAMP03SP, standard deviation saturates to a value of 3.4 m. This is an indication of contamination in the long to medium wavelength part, i.e. 50–100° for the satellite-only models. Moreover, the models DEOS-CHAMP-01C, GGM02C and then ITG-GRACE03 appear to have better fit for medium to long wavelength and can possibly be recommended for use as long wavelength part with the local observed data. While a hybrid geopotential model selection can be achieved through the selection from either of DEOS-CHAMP-01C, GGM02C, GGM02S, EIGEN-GRACE02S or ITG-GRACE03 in the long wavelength (to degree and order 40) and EGM96, PGM200A, EIGEN-GL04C, EIGEN-CG03C or even EGM2008 in medium to short wavelength, i.e. from degree 41 to maximum degree and order. 相似文献