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为了降低飞机限时派遣(TLD)的运行成本,提出了全权限数字式电子控制(FADEC)系统TLD分析的运行成本优化方
法。构建了TLD分析的典型马尔可夫模型,推导了该模型各状态稳态频度公式,从而建立了系统单位时间运行成本与派遣时间间
隔的函数关系,并以此作为运行成本优化的目标函数;推导了发动机控制系统平均安全性水平表达式,建立了平均安全性水平对
派遣时间间隔的约束。针对FADEC系统建立了3种不同的形式的系统单位时间运行成本函数模型,并提出了相应的派遣间隔决
策建议。结果表明:应用基于成本优化的FADEC系统TLD分析方法进行带故障派遣决策,能够在满足安全性要求的情况下,降低
飞机运行成本。 相似文献
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Li-xue Zou Shao-yan CuiJian Zhong Zong-chun YiYan Sun Yu-bo FanFeng-yuan Zhuang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Hematopoietic progenitor cell proliferation can be altered in either spaceflight or under simulated microgravity experiments on the ground, however, the underlying mechanism remains unknown. Our previous study showed that exposure of the human erythropoietin (EPO)-dependent leukemia cell line UT-7/EPO to conditions of simulated microgravity significantly inhibited the cellular proliferation rate and induced cell apoptosis. We postulated that the downregulation of the erythropoietin receptor (EPOR) expression in UT-7/EPO cells under simulated microgravity may be a possible reason for microgravity triggered apoptosis. In this paper, a human EPOR gene was transferred into UT-7/EPO cells and the resulting expression of EPOR on the surface of UT-7/EPO cells increased approximately 61% (p < 0.05) as selected by the antibiotic G418. It was also shown through cytometry assays and morphological observations that microgravity-induced apoptosis markedly decreased in these UT-7/EPO–EPOR cells. Thus, we concluded that upregulation of EPOR in UT-7/EPO cells could inhibit the simulated microgravity-induced cell apoptosis in this EPO dependent cell line. 相似文献
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Linfeng He Liang Lang Qingxia Li Wenchao Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
A hybrid method, combining the radiative transfer theory and the method of moments (MoM), is proposed to study the potential effect of the lunar surface roughness on the microwave brightness temperature. The total upward emission reaching the lunar surface from below media is calculated by the radiative transfer theory, and then the brightness temperature is obtained by weighting the bidirectional transmission coefficients which is computed using the MoM. The method is validated by both flat and rough surface models with analytic solutions. With the hybrid method, brightness temperatures from simulated lunar model are calculated and compared to those from a flat layered model. The comparisons show that the effect of rough surface on brightness temperature cannot be ignored and also depends on many other factors, such as observation angle and polarizations. For vertical polarization, an optimal observation angle may exist to reduce the effect of surface roughness. These results indicate that the knowledge of lunar surface roughness is important in microwave remote sensing to the Moon and may probably provide a guide to lunar projects in future. 相似文献
587.
Liang Li Zhiqiang Chen Ronglan Xu Ya Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The plasma density distribution of plasmasphere in the geomagnetic equatorial plane can help us study the magnetosphere like plasmasphere, ionosphere and their kinetics. In this paper, we introduce a new inversion method, GE-ART, to calculate the plasma density distribution in the geomagnetic equatorial plane from the Extreme Ultraviolet (EUV) data of IMAGE satellite under the assumption that the plasma density is constant along each geomagnetic field line. The new GE-ART algorithm was derived from the traditional Algebraic Reconstruction Techniques (ART) in Computed Tomography (CT) which was different from the several existing methods. In this new method, each value of the EUV image data was back-projected evenly to the geomagnetic field lines intersected by this EUV sight. A 3-D inversion matrix was produced by the contributions of all the voxels contained in the plasmasphere covered by the EUV sensor. That is, we considered that each value of the EUV image data was relative to the plasma densities of all the voxels passed through by the corresponding EUV radiation, which is the biggest difference to all the existing inversion methods. Finally, the GE-ART algorithm was evaluated by the real EUV data from the IMAGE satellite. 相似文献
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测量并分析计算了角分辨紫外光电子谱仪的电子能量分析器的聚焦特性 ,分析计算了紫外光斜入射时光电信号的校正因子。结果表明 :偏离分析器聚焦中心 β角的光电子被分析器接收的几率为高斯函数exp( - β2 /β0 2 ) ,且 β0 =3.5° ;斜入射光电信号的校正因子是光入射角α的函数且大于cosα 相似文献