排序方式: 共有60条查询结果,搜索用时 890 毫秒
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全量程标度因数不对称性是高精度石英挠性加速度计的一项重要指标,其大小对于惯导系统的导航精度具有非常大的影响。在加速度计精密离心机测试中,由离心加载引起的各种误差是进行加速度计标定的主要影响因素,论文给出了适用于精密离心机测试的加速度计输出模型与数据求解方法。为提高标定精度,以标度因数测试误差作为衡量指标,对输入数据进行迭代与修正;对修正后的测试数据进行三阶拟合,计算正向与负向标度因数,从而得到全量程标度因数不对称性。经试验验证,测试数据修正后可将标度因数误差从10-4降低至10-9,标度因数不对称性水平从10-4提高至10-5。 相似文献
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L.L. Lazutin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Temporal variations of the radiation belt particle during the magnetic storms are investigated using measurements by the low altitude satellite spectrometer. Along with several known effects, such as the outer radiation belt intensity decrease at the main phase, the radial diffusion with the particle acceleration and the recovery of the radiation belt during the recovery phase, some less known features were investigated, such as the dawn–dusk asymmetry of the radiation belt. 相似文献
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通过在背风母线处沿纵向对称面嵌入隔离板,观测了大攻角旋成体在这种背风涡被隔离状态下的表面压力分布情况。隔离板的作用旨在削弱、隔阻两侧背风涡间的相互联系和诱导,以便考察背风涡诱导作用对物面流动的影响。不同隔离(包括无隔离情况)状态下的实验结果表明,背风涡的隔离对表面压力分布有不同程度的影响,故这一研究和结果可供探讨大攻角流动非对称性成因作参考。 相似文献
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非对称空战体系对抗研究 总被引:2,自引:1,他引:1
对战斗机分代及其空战能力评估进行了研究,提出了空战体系对抗中,交战双方武器装备非对称度的概念和计算方法.基于体系对抗物理描述和数学模型,发展了非对称战役优势参数的概念.通过对典型的对称、非对称和极限非对称战役想定的作战模拟和分析,探讨了战斗机武器装备的数量与质量关系问题,装备质量太差就很难用数量去弥补.计算结果表明考虑非对称度影响的分析更接近当今战争的实际. 相似文献
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三相变压器的联结组标号必须判别确定。选较复杂的 Dy和 Yd类联结组为例 ,对其进行理论分析 ,获得作筛选法判别基准的理想计算值的规律性。在实测时考虑三相电源电压不对称的影响 ,用实测计算值代替理想计算值作判别基准。经微机的硬件与软件系统联试 ,能对全部联结组标号快捷地判别 ,不仅能判定对与错 ,还能指出错误联成何种标号 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(4):1915-1921
This paper presents the results of the analysis of the evolution of coronal holes (CHs) on the Sun during the period May 13, 2010 – March 20, 2022, covering Solar Cycle 24. Our study uses images in the extreme-ultraviolet iron line (Fe XII 193 Å) obtained with the Atmospheric Imager Assembly of the Solar Dynamics Observatory (AIA/SDO). To localize CHs and determine their areas, we used the Heliophysics Event Knowledgebase (HEK). We separate the CHs into polar and non-polar and study the evolutionary features of each group. During this period, an asymmetry between the Northern (N) and Southern (S) Hemispheres (N-S or hemispheric asymmetry) is detected both in the solar activity (SA) indices and in the localization of the maximum areas of the polar and non-polar CHs. It is shown that the hemispheric asymmetry of the areas of polar and non-polar CHs varies significantly over time and that the nature of these changes is clearly related to the SA cycle. We find that for most of the period, the polar CHs were predominated generated in the S- hemisphere while the non-polar CHs were dominant in the N- hemisphere. It is found that the maximum and minimum of the hemispheric imbalance in the areas of non-polar CHs are close in time to the maximum and minimum of the asymmetry of the SA indices (the number and areas of sunspots). The maximum hemispheric imbalance of the polar CH areas is observed at the maximum of Cycle 24, and the minimum imbalance is found at the cycle minimum. These results confirm our assumption that these two types of CHs are of a different nature and that the non-polar CHs, like sunspots, are elements of the general magnetic activity. 相似文献