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A.D. Danilov A.V. Konstantinova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):359-370
Long-term changes in the E-layer critical frequency, foE, at three stations of the European region (Juliusruh, Slough and Rome) and also at Moscow and Wakkanai stations are analyzed by the method developed by the authors and described in detail in the previous papers. It is found that Juliusruh and Slough stations demonstrate a well-pronounced change in foE (a trend) during two previous decades. At the same time, the same features of the behavior of the aforementioned trend k(foE) are obtained. The trend is positive and negative in the morning and evening hours, respectively. Similar diurnal behavior of k(foE) is found also for Moscow station but with lower absolute values of the trends. A well-pronounced seasonal behavior of k(foE) is detected at Juliusruh and Slough: the trend is minimal and maximal in the summer period and at the end of fall—beginning of winter, respectively. The maximal amplitude in the morning hours reaches +0.04?MHz per year, whereas the minimal amplitude in evening hours is ?0.06?MHz per year. No systematic changes exceeding by the magnitude 0.01?MHz per year are found for Rome and Wakkanai stations. It is assumed that the observed trends are related to changes (trends) in the meridional wind bringing NO molecules from the auroral oval to lower latitudes. 相似文献
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光纤陀螺的标度因数与光纤环的长度、直径及光源的平均波长有关。在温度条件下,光纤环的长度、直径及光源的平均波长均会发生变化,进而导致光纤陀螺在高低温下的标度因数不同,影响温度环境下的光纤陀螺标度因数的重复性。提出了一种基于光纤陀螺波长控制的标度因数温度性能提高方法,该方法在光源驱动电路的桥式回路中增加了铂电阻组件,从而可自动调节光纤陀螺光源的管芯温度,进而控制光源平均波长的变化,以抵消光纤环有效面积因温度变化而对标度因数产生的影响,提高温度环境下光纤陀螺的标度因数重复性。试验表明,该方法将未补偿情况下光纤陀螺全温范围内的标度因数重复性(1σ)由271×10-6~280×10-6减小到了32.5×10-6~43.5×10-6,标度因数重复性误差减小了84%~88%,并验证了该方法的有效性。 相似文献
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Xiaomin Zuo Weixing Wan Chunliang Xia Anshou Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Strong positive correlation between sporadic E layers and the solar activity and the long-term declining trend of Es were found in this paper. Then the feed-forward back propagation neural networks (NNs) were used to simulate the long-term variation of Es at four stations and predict foEs yearly average values. The inputs used for NNs are the yearly mean values of foEs in the daytime of the past ten years and the yearly averaged data of solar 10.7 cm radio flux (F107) of the present year, and the output is the present yearly mean value of daytime foEs. The outputs of trained NNs have high correlation with the desired values and the foEs yearly mean values predicted by NNs have good agreement with the observed data. The results indicate that NNs can make full use of the observed data to simulate the long variation rule of Es. Also, the results confirm the effect of solar activity on Es. 相似文献
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S. Valk A. Lemaître 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(8):1429-1443
This paper investigates the long-term perturbations of the orbits of geosynchronous space debris influenced by direct radiation pressure including the Earth’s shadowing effects. For this purpose, we propose an extension of our homemade semi-analytical theory [Valk, S., Lemaître, A., Deleflie, F. Semi-analytical theory of mean orbital motion for geosynchronous space debris under gravitational influence. Adv. Space Res., submitted for publication], based on the method developed by Aksnes [Aksnes, K. Short-period and long-period perturbations of a spherical satellite due to direct solar radiation. Celest. Mech. Dyn. Astron. 13, 89–104, 1976] and generalized into a more convenient non-singular formalism. The perturbations accounting for the direct radiation pressure with the Earth’s shadow are computed on a revolution-by-revolution basis, retaining the original osculating Hamiltonian disturbing function. In this framework, we compute the non-singular mean longitude at shadow entry and shadow exit at every orbital revolution in opposition to classical approaches where the singular eccentric anomalies at shadow entry and shadow exit are computed. This new algorithm is developed using non-singular variables. Consequently, it is particularly suitable for both near-circular and near-equatorial orbits as well as orbits which transit periodically around null eccentricities and null inclinations.The algorithm is tested by means of numerical integrations of the equations, averaged over the short periods, including radiation pressure, J2, the combined Moon and Sun third body attraction as well as the long-term effects of the 1:1 resonance occurring for geosynchronous objects. As an extension of [Valk, S., Lemaître, A., Anselmo, L. Analytical and semi-analytical investigations of geosynchronous space debris with high area-to-mass ratios influenced by solar radiation pressure. Adv. Space Res., doi:10.1016/j.asr.2007.10.025, 2007b], we especially apply our analysis to space debris with area-to-mass as high as 20 m2/kg. This paper provides numerical and semi-analytical investigations leading to a deep understanding of the long-term evolution of the semi-major axis. Finally, these semi-analytical investigations are compared with accurate numerical integrations of the osculating equations of motion over time scales as high as 25 years. 相似文献
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成功建立带TPS风洞测力试验技术的一个关键问题是确保试验数据具有足够的精度,必须精细地分配误差。为获得满足工程需要的高精度测力试验数据,给出一种基于计算机符号运算的子程序,完成不确定度计算过程中公式自动推导、计算。最后通过对TPS风洞试验数据精度的敏度分析,给出了某运输机在2.4m跨声速风洞TPS试验中各环节的误差分配要求。 相似文献