Analytic and numerical treatment of motion of dust grain particle around triangular equilibrium points with post-AGB binary star and disc

This paper investigates the motion around the triangular equilibrium points, of a passively gravitating dust particle in the gravitational field of a low-mass post-AGB binary system, surrounded by circumbinary disc. The two bodies of the binary are modeled as a triaxial star and a radiating-oblate star. Due to small deviation of disc stars on circular orbits, we have assumed that the Coriolis and centrifugal forces of the stars are slightly perturbed. The triangular equilibrium points of the particle are found. These points are defined by, triaxiality of the primary star, oblateness and radiation of the secondary one and the gravitational potential from the disc mass. Further, when the disc mass increases, the particle moves nearer to the stars and farther away from the disc. In general, these equilibrium points are linearly stable when μ < μ_C; where μ is the mass ratio and μ_C is the critical mass function, defined by the parameters of the system. The effects of each of these parameters on the size of the stability region are stated, and the periodic motion around the stable points is examined. It is seen that the orbits are ellipses, and the orientation, eccentricities, lengths of the semi-major and semi-minor axes are influenced by the parameters of the problem. In particular, for our numerical linear stability analysis, we have taken an extremely depleted pulsating star, IRAS 11472-0800 as the post-AGB triaxial star, with a weakly-radiating young white dwarf star; G29-38 as the secondary. For this system, the stability result of the triangular points comes out different. Here, μ_C < μ throughout the entire range of the mass ratio and the critical mass function. Hence, the triangular equilibrium points are unstable. The stability of the orbits is tested using the Poincaré surfaces of section (Pss). The region of stability is controlled by the introduced parameters and the Jacobi constant.     

基于R统计分析软件的航空数据作图方法研究

为了快速高效分析航空数据信息,采用R语言分析软件制作了条形图、饼图、直方图、核密度图、箱线图和小提琴图,图片精美实用,便于人们使用.实践证明,该软件便于操作,实用性强,可以成为大数据时代科研人员的研究利器.     

R/S方法求解网络流量自相似参数的实现与应用

基于网络流量具有统计自相似性的理论,通过计算自相似参数Hurst值来检验流量的自相似程度。采用R/S方法对流量数据进行分析,给出了R/S方法详细的实现算法,通过实验的分析与比较,验证了自相似性的存在。自相似性是正常网络流量具备的特征,当流量发生异常时,Hurst值会出现明显的变化,本文将这一变化应用于DDoS攻击检测做了初步的探讨。基于自相似理论的网络流量异常检测技术与传统的基于统计异常技术和数据包特征匹配等方法相比,具有更高的准确性和可靠性。     

R141b在圆形微通道内的沸腾换热实验研究

为提高换热强度、解决设备内部高热流密度散热问题,采用实验方法研究R141b在不同直径(D=0.5mm和1.0mm)水平圆形微通道内的沸腾换热特性,分析了热流密度(q=2.0kW/m~2～47.6kW/m~2)、质量干度(x=0～0.6)、质量流速(G=111.11kg/(m~2·s)～333.33kg/(m~2·s))的变化对平均传热系数h的影响,探究不同情况下影响沸腾换热的主导因素。实验研究表明:平均传热系数h随热流密度q的增加而减小,在不同范围内减小速率有明显差异;热流密度q=2kW/m~2～5kW/m~2时质量流速G对平均传热系数h影响较明显,热流密度较高时质量流速G对换热影响很小;在质量流速G=111.11kg/(m~2·s)～333.33kg/(m~2·s),质量干度x0.3时,平均传热系数h随质量干度x增加而明显下降,在设计微通道换热器时应尽量使R141b处于初始沸腾阶段以获得更好换热效果,并采取一定措施预防干度过高引起的换热恶化。     

R134a的热物理性质计算

氯氟碳化合物（ＣＦＣ）作为制冷与空调设备的工质，长期以来被广泛应用于生产和生活的各个部门。近年来，人们逐步认识到某些ＣＦＣ对臭氧层具有破坏作用和挥发后产生温室效应，因此不得不寻求新的替代工质。替代Ｒ１２的制冷剂方案中，有单一工质，也有混合工质。在单一工质中，从长远意义上最有希望替代Ｒ１２的新工质是民１３４ａ。为了对制冷系统应用Ｒ１３４ａ进行性能评价，而要一套完整的热物理性质公式。目前，有关Ｒ１３４ａ的热力学性质数据较多，但有关它的热物理性质数据却很少。本文列出并推导了Ｒ１３４ａ热物理性质的计算方程式，给出了部分计算数据，为用Ｒ１３４ａ作为制冷剂循环的制冷装置及换热器计算机辅助设计打下基础。     

基于MB86R01的图形显示设计

本文在介绍MB86R01的特点和功能的基础上,以飞机座舱显示系统中常见的姿态画面为例,设计并开发了基于MB86R01的图形显示平台.这种图形显示平台在未来飞机显示系统中具有广阔应用前景。     

机载蒸发循环系统动态仿真

从部件的数学模型出发,根据闭环系统各部件的耦合关系,建立了机载蒸发循环系统的动态数学模型。对充注R142b的机载蒸发循环系统进行了动态仿真,仿真数据与试验数据基本吻合,仿真方法可靠,可以作为机载蒸发循环系统优化及系统控制的依据。     

结合TEC的泵驱两相温控系统的空间应用

为满足天舟一号货运飞船(T Z1)蒸发冷凝科学实验的控温需求,采用半导体制冷片(TEC)和泵驱两相回路结合的控温系统实现了冷凝台-5~40 ℃(±0.2 ℃)的控温要求。对TEC和平行流换热器进行了研究,结果表明该系统能够满足环境温度等于30 ℃工况下的制冷和散热要求。测试结果表明,平行流换热器在地面和在轨的换热相当,说明重力的影响几乎可以忽略。     

纤维增强陶瓷基复合材料中纤维增韧分析模型

对于单向纤维增强陶瓷基复合材料，在考虑纤维桥联和纤维拔出两种主要增韧机理的基础上，建立了研究紧凑拉伸试样断裂行为的理论模型，并利用该模型计算了裂纹扩展的Ｒ－阻力曲线和载荷／位移曲线，计算结果表明：由于纤维桥联与拔出，使得Ｒ－曲线和载荷／位移曲线呈现明显的非线性行为，纤维桥联是主要增韧机制。体积分数５０％ＳｉＣ１／ＬＡＳ复合材料断裂韧性的计算值与实验值吻合。     

Fronts and thermohaline structure of the Brazil–Malvinas Confluence System

Fronts and thermohaline structure of the Brazil–Malvinas Confluence System (BMCS) are studied from climatic data, “Marathon Exp. Leg.8, 1984” data, and Sea surface temperature (SST) data base “ds277-Reynolds” (1981–2000). The South Atlantic Central Water (SACW) is divided in two main types: tropical (TW) and subtropical water (ST). Water masses, Fronts, Inter-Frontal and Frontal Zones are analysed and classified: (a) the water masses: Tropical Low-Salinity Water, Tropical Surface Water, Tropical Tropospheric Water, Subtropical Low-Salinity Water, Subtropical Surface Water, Subtropical Tropospheric Water. T,S characteristics of intermediate, deep and bottom water defined by different authors are confirmed and completed; (b) the Inter-Frontal Zones: Tropical/Brazil Current Zone, Subtropical Zone and Subantarctic Zone; (c) the Frontal Zones: Subtropical, Subantarctic and Polar, and (d) the Fronts: Subtropical Front of the Brazil Current, Principal Subtropical Front, North Subtropical Front, Subtropical Surface Front, South Subtropical Front, Subantarctic Surface Front, Subantarctic Front and Polar Front. Several stable T–S relationships are found below the friction layer and at the Fronts. The maximum gradient of the oceanographic characteristics occurs at the Brazil Current Front, which can be any of the subtropical Fronts, depending on season. Minimum mean depth of the pycnocline coincides with the Fronts of the BMCS, indicating the paths of low-salinity shelf waters into the open ocean. In the work it is shown how to recover the horizontal and vertical thermohaline structure of waters from satellite data RSMAS SST.