机翼弹性变形对气动特性的影响

在非结构混合网格框架下,采用有限体积法求解了Euler方程和N-S方程。使用结构影响系数法计算机翼结构的弹性变形,通过动态网格技术实现了气动力与结构变形之间的耦合运算,计算和分析了在气动载荷作用下的机翼变形和此时的气动特性,算例分析表明：典型后掠机翼的弹性变形会使机翼产生了正的挠度和负的剖面扭转角,在弯曲和扭转的相互作用下,机翼的有效迎角减小,从而导致机翼的升力系数减小。在Euler方程和N-S方程算例中,考虑弹性变形条件下的机翼升力系数比刚性机翼的升力系数分别减小了25.3%和24.1%。     

基于控制理论方法的翼型最大升力优化设计

使用控制理论方法建立了对翼型最大升力优化设计的模型.并且在给定约束力矩系数和约束翼型面积条件下对GAW-1低速高升力翼型进行了最大升力状态实例优化设计,验证了使用粘性伴随方法建立的以翼型最大升力为目标的多约束优化模型的有效性。     

The COMPLEIK subroutine of the IONORT-ISP system for calculating the non-deviative absorption: A comparison with the ICEPAC formula

The present paper proposes to discuss the ionospheric absorption, assuming a quasi-flat layered ionospheric medium, with small horizontal gradients. A recent complex eikonal model (Settimi et al., 2013b) is applied, useful to calculate the absorption due to the ionospheric D-layer, which can be approximately characterized by a linearized analytical profile of complex refractive index, covering a short range of heights between h₁ = 50 km and h₂ = 90 km. Moreover, Settimi et al. (2013c) have already compared the complex eikonal model for the D-layer with the analytical Chapman’s profile of ionospheric electron density; the corresponding absorption coefficient is more accurate than Rawer’s theory (1976) in the range of middle critical frequencies. Finally, in this paper, the simple complex eikonal equations, in quasi-longitudinal (QL) approximation, for calculating the non-deviative absorption coefficient due to the propagation across the D-layer are encoded into a so called COMPLEIK (COMPLex EIKonal) subroutine of the IONORT (IONOspheric Ray-Tracing) program ( Azzarone et al., 2012). The IONORT program, which simulates the three-dimensional (3-D) ray-tracing for high frequencies (HF) waves in the ionosphere, runs on the assimilative ISP (IRI-SIRMUP-P) discrete model over the Mediterranean area ( Pezzopane et al., 2011). As main outcome of the paper, the simple COMPLEIK algorithm is compared to the more elaborate semi-empirical ICEPAC formula (Stewart, undated), which refers to various phenomenological parameters such as the critical frequency of E-layer. COMPLEIK is reliable just like the ICEPAC, with the advantage of being implemented more directly. Indeed, the complex eikonal model depends just on some parameters of the electron density profile, which are numerically calculable, such as the maximum height.     

Assessment of depth to magnetic sources using high resolution aeromagnetic data of some parts of the Lower Benue Trough and adjoining areas,Southeast Nigeria

High resolution airborne magnetic data acquired between 2005 and 2010 were used to determine depth to shallow and deep magnetic sources in some parts of Southeastern Nigeria. Various depth estimation methods such as standard Euler deconvolution (SED), source parameter imaging (SPI), spectral depth analysis (SDA) and two dimensional (2-D) forward modeling were applied. Results obtained from SED, SPI and models of profiles 1 and 2 indicate that the Abakaliki Anticlinorium (AA) and Ikom-Mamfe Rift (IMR) regions are dominated by short wavelength magnetic anomalies caused by extensive tectonic events. The SED map showed depth to shallow and deep magnetic sources ranging from ~ 16.6 to ~ 338.3 m and ~ 394.3 to ~ 5748.1 m respectively. Likewise, depth estimates from the SPI map varies from ~ 147.1 to ~ 554.2 m (shallow magnetic sources) and ~ 644.2 to ~ 6141.6 m (deep magnetic sources). The result obtained from SDA revealed depths to deep magnetic basement in the range of ~ 769 to ~ 6666 m with an average of ~ 3449 m. Also, it showed that depth to shallow magnetic sources vary between ~ 119 and ~ 434 m with mean of ~ 269 m. The 2-D forward modelling showed maximum depth values of ~ 4700, ~4600 and ~ 6500 m in the models of profiles 1, 2 and 3 within the Anambra Basin (AB), Afikpo Syncline (AS) and Calabar Flank (CF) respectively. Generally, from all the various methods applied the results indicate that AB, AS and CF are dominated by long wavelength anomalies. The 2-D models indicated that the basement framework is undulant. Also, depth estimates involving the various methods used in this study correlate strongly with each other in the AB, AS and CF geological regions.     

The calculation of ionospheric absorption with modern computers

New outcomes are proposed for ionospheric absorption starting from the Appleton–Hartree formula, in its complete form. The range of applicability is discussed for the approximate formulae, which are usually employed in the calculation of non-deviative absorption coefficient. These results were achieved by performing a more refined approximation that is valid under quasi-longitudinal (QL) propagation conditions. The more refined QL approximation and the usually employed non-deviative absorption are compared with that derived from a complete formulation. Their expressions, nothing complicated, can usefully be implemented in a software program running on modern computers. Moreover, the importance of considering Booker’s rule is highlighted. A radio link of ground range D = 1000 km was also simulated using ray tracing for a sample daytime ionosphere. Finally, some estimations of the integrated absorption for the radio link considered are provided for different frequencies.     

三维机翼结冰模拟

针对机翼结冰问题,利用欧拉法求解空气水滴两相流流场,通过Fluent软件用户自定义函数功能编程求解三维机翼表面水滴局部收集系数以及结冰情况.在计算中.将水溢流方向沿机翼弦向和展向分解,以此对Messinger结冰热力学模型进行改进,使之更符合三维情况,并在此基础上进行三维传质传热分析;修正传统的二维表面对流换热系数求解...     

竟拍过程的概率延拓分析

到拍卖行去竟拍拍品,已经成为我们生活中越来越平常的经济行为,在竟拍过程中,两人轮流举牌,甲先乙后,谁先拍到呢?结合概率论中的全概率公式,给出了甲先拍到的充要条件;在此基础上进行延拓,探讨随着竟价的提升,两人心理承受能力的等差下降和非等差下降对竟拍的影响,甲先拍到的概率变化,并推导出相应的概率计算公式.     

Space debris mitigation in geosynchronous orbit

In order to preserve the geosynchronous region, the Inter-Agency Space Debris Coordination Committee (IADC) proposed and endorsed a re-orbiting strategy for spacecraft at the end-of-life: they should be disposed above the synchronous altitude and passivated, to reduce the risk of inadvertent explosions. The recommended perigee altitude of the disposal orbit took into account all relevant perturbations and was a function of the expected perturbing acceleration induced by solar radiation pressure. It was intended to prevent any further interference with a properly defined geostationary protected region.     

改进的万有引力公式

根据广义相对论给出的行星运动方程，导出如下改进的万有引力公式F＝－GMm/r^2-3G^2M^2mp/c^2r^4应用该公式可给出光线近日偏折问题的准确解。     

广义Lefschetz数的粘接公式的应用

本文通过研究拓扑空间上幂等自映射在基本群上诱导的作用和点同伦，得到与之同伦的，具有较好性质的自映射。并利用自映射这些性质，使用广义Lefschetz数的粘接公式，得到幂等自映射的Nielsen数不超过1的结论。