火炮首发命中率试验脱靶弹数据处理方法

通过对出现脱靶弹情况下的散布特征参数估计方法进行研究,建立正态双边截尾样本均值和方差估计数学模型,并给出了数值计算方法,为火炮武器系统首发命中概率试验脱靶提供了理论依据。     

国产5056铝蜂窝芯的制备与性能评价

针对太阳翼基板用高性能低密度5056铝蜂窝芯的需求,开展了国产5056超薄铝箔制备及配套阳极氧化表面处理、国产5056铝蜂窝的制备和性能评价。研制的国产5056铝蜂窝芯公称密度17.28 kg/m³,节点强度为1.87 kN/m,蜂窝芯裸压缩、平面压缩、L向剪切、W向剪切强度分别达到了0.29、0.31、0.38、0.27 MPa,力学性能均达到了进口蜂窝芯的水平。蜂窝芯胶膜热破工艺性能较好,网格夹层结构节点无脱开,弯曲刚度和强度测试值均达到了进口蜂窝测试值的水平,可以满足使用需求。试验结果可为后续高性能低密度铝蜂窝芯的型号应用及原材料国内自主保障提供数据基础及技术基础。     

月球风化层钻取采样过程密实度分类研究

钻取采样是月球风化层土壤样品获取的重要方式,密实度是重要的风化层月壤原位特性,对钻进过程中的策略制定有重要影响。本文结合钻取采样过程特点,提出了通过采样机构的力、速度、电流、温度等传感器获取的瞬时信息感知月壤密实度的方法,利用深度学习方法构建一类适应于可变长度序列数据的门控型循环神经网络,实现钻进过程月壤密实度在线分类。研究表明,该分类方法在风化层钻进过程中月壤密实度感知滞后时间约为33 s,对未知序列数据识别正确率大于89.36%,具有较高的分类精度和泛化能力。     

The solar cycle variation of plasma parameters in equatorial and mid latitudinal areas during 2005–2010

Based on the ISL data detected by DEMETER satellite, the solar cycle variation in electron density (Ne) and electron temperature (Te) were studied separately in local daytime 10:30 and nighttime 22:30 during 2005–2010 in the 23rd/24th solar cycles. The semi-annual, annual periods and decreasing trend with the descending solar activity were clearly revealed in Ne. At middle and high latitudes, there exhibited phase shift and even reversed annual variation over Southern and Northern hemisphere, and the annual variation amplitudes were asymmetrical at both hemispheres in local daytime. In local nighttime, the annual variations of Ne at south and north hemispheres were symmetrical at same latitudes, but the annual variation amplitudes at different latitudes differed largely, showing obviously zonal features. As for Te, the phase shift in annual variations was not as apparent as Ne with the increase of latitudes at Southern and Northern hemisphere in local daytime. While in local nighttime the reversed annual variations of Te were shown at low latitudinal areas, not at high latitudes as those in Ne. The correlation study on Ne and Te illustrated that, in local daytime, Ne and Te showed strong negative correlation at equator and low latitudes, but during the solar minimum years the correlation between Ne and Te changed to be positive at 25–30° latitudes in March 2009. The correlation coefficient R between Ne and Te also showed semi-annual periodical variations during 2005–2010. While in local nighttime, Ne and Te exhibited relatively weak positive correlation with R being about 0.6 at low latitudes, however no correlation beyond latitudes of 25° was obtained.     

Unusual nighttime impulsive foF2 enhancements at low latitudes: Phenomenology and possible explanations

This paper is focused on unusual nighttime impulsive electron density enhancements that are rarely observed at low latitudes on a wide region of South America, under quiet and medium/high geomagnetic conditions. The phenomenon under investigation is very peculiar because besides being of brief duration, it is characterized by a pronounced compression of the ionosphere. The phenomenon was studied and analyzed using both the F2 layer critical frequency (foF2) and the virtual height of the base of the F region (h′F) values recorded at five ionospheric stations widely distributed in space, namely: Jicamarca (−12.0°, −76.8°, magnetic latitude −2.0°), Peru; Sao Luis (−2.6°, −44.2°, magnetic latitude +6.2°), Cachoeira Paulista (−22.4°, −44.6°, magnetic latitude −13.4°), and São José dos Campos (−23.2°, −45.9°, magnetic latitude −14.1°), Brazil; Tucumán (−26.9°, −65.4°, magnetic latitude −16.8°), Argentina. In a more restricted region over Tucumán, the phenomenon was also investigated by the total electron content (TEC) maps computed by using measurements from 12 GPS receivers. A detailed analysis of isoheight ionosonde plots suggests that traveling ionospheric disturbances (TIDs) caused by gravity wave (GW) propagation could play a significant role in causing the phenomenon both for quiet and for medium/high geomagnetic activity; in the latter case however a recharging of the fountain effect, due to electric fields penetrating from the magnetosphere, joins the TID propagation and plays an as much significant role in causing impulsive electron density enhancements.     

TEC variability near northern EIA crest and comparison with IRI model

Monthly median values of hourly total electron content (TEC) is obtained with GPS at a station near northern anomaly crest, Rajkot (geog. 22.29°N, 70.74°E; geomag. 14.21°N, 144.9°E) to study the variability of low latitude ionospheric behavior during low solar activity period (April 2005 to March 2006). The TEC exhibit characteristic features like day-to-day variability, semiannual anomaly and noon bite out. The observed TEC is compared with latest International Reference Ionosphere (IRI) – 2007 model using options of topside electron density, NeQuick, IRI01-corr and IRI-2001 by using both URSI and CCIR coefficients. A good agreement of observed and predicted TEC is found during the daytime with underestimation at other times. The predicted TEC by NeQuick and IRI01-corr is closer to the observed TEC during the daytime whereas during nighttime and morning hours, IRI-2001 shows lesser discrepancy in all seasons by both URSI and CCIR coefficients.     

小尺寸应变天平设计方法研究

Φ0.3m高超声速低密度风洞测力试验模型尺寸小、天平载荷小、流场总温高,天平防热结构设计难,刚度要求和灵敏度要求矛盾突出,测力天平的研制难度大。采用数值仿真和风洞试验相结合的研究方法,对应用于该情况下的内式天平在温度影响和结构设计方面进行了研究。采用有限元方法对天平温度影响和结构应力分布做了详细分析,并对分析结果进行了风洞试验验证。结果表明：在实现天平结构优化设计及提高天平设计的准确性和可靠性方面,有限元分析设计方法是非常有效的技术途径。     

机载燃油密度传感器高低温静态试验技术

为了验证航空机载燃油密度传感器在高温燃油和低温燃油中的燃油密度测量精度,运用阿基米德原理对高低温静态验证试验技术进行了研究。设计和提出了一种新的高精度航空机载燃油密度传感器高低温静态试验装置和方法。研究结果表明：试验装置密度测量系统的测量最大误差为-0.077%,符合试验装置测量精度为受试品测量精度4倍及以上的规定（受试品测量精度为0.4%）。结果通过了C919总体设计单位和美国Parker公司的评审,能可靠地验证航空机载燃油密度传感器在高温燃油和低温燃油中的燃油密度测量精度,为航空机载燃油密度传感器工程应用和装机试飞提供了试验数据支撑。     

Variability of the ionospheric electron density at fixed heights and validation of IRI-2007 profile’s prediction at Ilorin

A study on the variability of the equatorial ionospheric electron density was carried out at fixed heights below the F2 peak using one month data for each of high and low solar activity periods. The data used for this study were obtained from ionograms recorded at Ilorin, Nigeria, and the study covers height range from 100 km to the peak of the F2 layer for the daytime hours and height range from 200 km to the peak of the F2 layer for the nighttime hours. The results showed that the deviation of the electron density variation from simple Chapman variation begins from an altitude of about 200 km for the two months investigated. Daytime minimum variability of between 2.7% and 9.0% was observed at the height range of about 160 and 200 km during low solar activity (January 2006) and between 3.7% and 7.8% at the height range of 210 and 260 km during high solar activity (January 2002). The nighttime maximum variability was observed at the height range of 210 and 240 km at low solar activity and at the height range of 200 and 240 km at high solar activity. A validation of IRI-2007 model electron density profile’s prediction was also carried out. The results showed that B0 option gives a better prediction around the noontime.     

Cross testing of ionosphere models IRI-2001 and IRI-2007, data from satellite altimeters (Topex/Poseidon and Jason-1) and global ionosphere maps

In this study, we use a great body of statistical data covering the entire 23rd solar cycle to cross test data of satellite altimeters, Global Ionosphere Maps and the International Reference Ionosphere models, IRI-2001 and IRI-2007. It is revealed that experimental TEC values of the satellite altimeters regularly exceed the model ones by ∼3 TECU (1 TECU = 10¹⁶ m⁻²). The best possible value of difference between TECs obtained from altimeter and GIM-map data significantly differs for different laboratories: the maximum for CODG data falls on 2.5 TECU, ESAG – 3 TECU, JPLG – 0 TECU, UPCG – 2 TECU. The dependence of experimental and model data root-mean-square deviation on the F10.7 index is shown to be nearly linear. IRI-2001 and IRI-2007 relative errors are characterized by considerable 11-year and annual variations. Given the geomagnetic planetary index K_p under 7, IRI-2001 and IRI-2007 reproduce TEC in the ionosphere with an accuracy of ∼30% relative to measurement data from satellite altimeters. The amplitude of absolute error variations resulting from the difference in ionization enhancement between the model and the real ionosphere during the morning solar terminator transit is ∼5 TECU.