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Ⅰ型极值分布的环境因子 总被引:1,自引:0,他引:1
本文通过对Ⅰ型极值分布的理论分析和环境因子的二因子法,分别得到了Ⅰ型极大值分布和Ⅰ型极小值分布的环境因子,它们与正态分布的环境因子^[1]具有相同的形式,对Ⅰ型极值分布的环境因子进行了点估计,提出了用环境因子进行数据转换和综合的步骤。 相似文献
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为了探究当量比对甲烷-空气连续旋转爆轰燃烧室(CRDC)特性的影响,利用二维可压缩欧拉方程对CRDC进行了数值研究,分析了爆轰波的发展过程和贫燃熄火过程,对比了不同工况下CRDC特性参数的变化情况。结果表明:CRDC起爆后燃烧场在由不稳定状态到相对稳定状态的过程中发生了2次碰撞,当进气当量比较低时,CRDC未能完全发生2次碰撞过程就已经熄爆。随着进气当量比的降低,爆轰波传播速度、轴向平均速度、出口平均温度、出口平均总压均呈下降趋势;增压比随当量比降低而减小的根本原因在于旋转爆轰燃烧过程和等压燃烧过程的熵增差减小,使吉布斯自由能增量差减小。CRDC的燃料驻留时间处于亚毫秒量级,燃烧热效率保持在99%以上。 相似文献
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《中国航空学报》2021,34(10):20-35
Aiming to maximize the aerodynamic performance of the Distributed Electric Propulsion (DEP) aircraft, a hybrid design framework which focuses on the aerodynamic performance of the propeller/wing integration has been developed and validated numerically. Variable-fidelity modelling for propeller aerodynamics has been used to achieve computational efficiency with reasonable accuracy. By optimizing the aerodynamic loading distributions on the tractor propeller disk, the induced slipstream is redistributed into a form that is beneficial for the wing downstream, based on which the propeller blade geometry is generated through a rapid inversed design procedure. As compared with the Minimum Induced Loss (MIL) propeller at a specified thrust level, significant improvements of both the lift-to-drag ratio of the wing and the propeller/wing integrated aerodynamic efficiency is achieved, which shows great promise to deliver aerodynamic benefits for the wing within the propeller slipstream without any additional devices. 相似文献
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S.-Y. Su C.H. Liu C.-K. Chao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1628-1635
Longitudinal distributions of post-midnight equatorial ionospheric irregularity occurrences observed by ROCSAT-1 (1st satellite of the Republic of China) during moderate to high solar activity years in two solstices are studied with respect to the vertical drift velocity and density variations. The post-midnight irregularity distributions are found to be similar to the well-documented pre-midnight ones, but are different from some published distributions taken during solar minimum years. Even though the post-midnight ionosphere is sinking in general, longitudes of frequent positive vertical drift and high density seems to coincide with the longitudes of high irregularity occurrences. Large scatters found in the vertical drift velocity and density around the dip equator in different ROCSAT-1 orbits indicate the existence of large and frequent variations in the vertical drift velocity and density that seem to be able to provide sufficient perturbations for the Rayleigh-Taylor (RT) instability to cause the irregularity occurrences. The need of seeding agents such as gravity waves from atmospheric convective clouds to initiate the Rayleigh-Taylor instability may not be necessary. 相似文献
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在文[1-4]的基础上进一步研究了带有不完全信息的随机截尾试验模型(IRCT)。着重讨论了对数正态分布参数的统计分析问题,建立了参数所满足的似然方程组,给出并证明了似然方程组解即参数的极大似然估计(MLE)的存在唯一性定理,所得的结论对于正态分布也同样适用。文末给出了随机模拟数值解例子,结果表明,参数的MLE具有较高的精度。 相似文献
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Knowledge of the observable properties of orbital debris is necessary to validate debris models for both the low Earth orbit (LEO) and the geosynchronous Earth orbit (GEO). Current methods determine the size and mass of orbital debris based on knowledge or assumption of the material type of the piece. Improvement in the knowledge of material is the goal of the research described herein. The process of using spectral absorption features to determine the material type is explored. A review of the optical measurements of orbital debris as well as current research in the area is discussed. Reflectances of common spacecraft materials are compared. The need for, and advances made possible by obtaining real data are explored. The prospects of the venture are investigated. 相似文献
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Ashavani Kumar Summit JalotaRenu Gupta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Study of depth–dose distributions for intermediate energy ion beams in tissue-like media such as polyethylene (CH2)n provides a good platform for further improvements in the fields of hadrontherapy and space radiation shielding. The depth–dose distributions for 12C ions at various energies and for light and intermediate ion beams (3He, 16O, 20Ne and 28Si) as well as for heavy ions 56Fe in polyethylene were estimated by using simulation toolkit: Geant4. Calculations were performed mainly by considering two different combinations of standard electromagnetic (EM), binary cascade (BIC), statistical multifragmentation (SMF) and Fermi breakup (FB) models. The energies of the ion beams were selected to achieve the Bragg peaks at predefined position (∼60 mm) and as per their availability. Variations of peak-to-entrance ratio (from 7.44 ± 0.05 to 8.87 ± 0.05), entrance dose (from 2.89 ± 0.01 to 203.71 ± 0.63 MeV/mm) and entrance stopping power (from 3.608 to 208.858 MeV/mm, calculated by SRIM) with atomic number (Z) were presented in a systematic manner. The better peak-to-entrance ratio and less entrance dose in the region Z = 2 to 8 (i.e. 3He to 16O) may provide the suitability of the ion beams for hadrontherapy. 相似文献
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