Three dimensional temperature field in a conducting sphere due to an arbitrarily located split ring heating source

Thermal control of spacecrafts plays an important role in space missions. In the design stage the preliminary thermal analysis of the spacecraft requires an estimate of the conductive thermal resistance between the various spacecraft components. With this in mind, the fully three dimensional problem of determining the thermal field in a conducting sphere with an asymmetric split ring current carrying heating source is resolved in an analytical or almost analytical form, implying either a closed form solution or utmost expressions involving a simple numerical integration. This has immediate application for evaluation of thermal resistance in spacecrafts. Green's function integral techniques are used. Comparisons are made with series solutions and also with purely numerical solutions to contrast the simplicity and highlight the elegance of the present method. Parametric studies reveal expected behavior.     

Influence of lunar topography on simulated surface temperature

The surface temperature of the Moon is one of the essential parameters for the lunar exploration, especially to evaluate the Moon thermophysical features. The distribution of the temperature is heavily influenced by the Moon topography, which, however, is rarely studied in the state-of-art surface temperature models. Therefore, this paper takes the Moon topography into account to improve the surface temperature model, Racca model. The main parameters, such as slopes along the longitude and latitude directions, are estimated with the topography data from Chang’E-1 satellite and the Horn algorithm. Then the effective solar illumination model is then constructed with the slopes and the relative position to the subsolar point. Finally, the temperature distribution over the Moon surface is obtained with the effective illumination model and the improved Racca model. The results indicate that the distribution of the temperature is very sensitive to the fluctuation of the Moon surface. The change of the surface temperature is up to 150 K in some places compared to the result without considering the topography. In addition, the variation of the surface temperature increases with the distance from the subsolar point and the elevation, along both latitude and longitude directions. Furthermore, the simulated surface temperature coincides well with the brightness temperature in 37 GHz observed by the microwave sounder onboard Chang’E-2 satellite. The corresponded emissivity map not only eliminates the influence of the topography, but also hints the inherent properties of the lunar regolith just below the surface. Last but not the least, the distribution of the permanently shadowed regions (PSRs) in the lunar pole area is also evaluated with the simulated surface temperature result.     

应用计算几何的月面太阳辐照度仿真模型

月面太阳辐照度对月面环境分析、月面巡视器设计具有重要意义。文章提出了一种应用计算几何的月面任意位置太阳辐照度仿真模型。首先,计算太阳、地球等天体相对月面点的位置;然后,将各天体投影至以月面点为球心的天球球面,并通过裁剪运算和二维布尔运算得到太阳未被遮挡的形状;最后,利用太阳可见面积对理想太阳辐照度模型进行修正,得到通用的模型。为验证提出模型的有效性,将仿真结果与STK软件进行比较。结果表明,文章中的模型综合考虑了地球、月面等多种因素对太阳辐射的耦合影响,其与STK软件获得的结果相比,更符合真实的太阳光照状态。     

太阳帆日心定点悬浮转移轨道设计

研究了太阳帆航天器日心定点悬浮轨道(HFDO)的转移轨道设计问题,以球坐标形式建立了太阳帆的动力学模型,基于该模型给出在日心悬浮轨道基础上实现定点悬浮的条件,提出了一种实现日心定点悬浮的转移轨道设计方法。首先,确定定点悬浮的位置;然后,设计经过该位置的绕日极轨轨道;最后,实施轨道减速实现定点悬浮,并给出了解析形式的轨道控制律。结合太阳极地观测任务,设计了定点悬浮在太阳北极1AU处的太阳帆转移轨道。仿真结果表明:该轨道转移方案总耗时3.5年,太阳帆定点到黄北极距日心1AU处,此后只要保持太阳光垂直照射帆面,即可维持稳定的悬浮状态。     

纳米铝粉及纳米铝粉/煤油凝胶体系能量性能研究

测定了各单组分及纳米铝粉／煤油凝胶体系的燃烧热,表征了纳米铝粉及纳米铝粉／煤油凝胶体系的能量性能。实验结果表明,随着纳米铝粉含量的增加,纳米铝粉／煤油凝胶体系的质量恒容燃烧热呈降低趋势,这是由于煤油的燃烧热值较高,铝粉的燃烧热值较低所致;而各纳米铝粉／煤油凝胶体系的密度随纳米铝粉含量的增加呈升高趋势,体系的体积燃烧热也随纳米铝粉含量增加而升高。     

Study of Solar Corona in China

Considerable progress for the study of solar corona physics has been achieved by China's space physics community. It involves the theoretical study of coronal process of solar active phenomena, solar wind origin, acceleration of solar wind and coronal mass ejections, observational and numerical study of these problems and prediction methods of solar eruptive activities (such as flares/CMEs). Here is a brief summary of the progress in this area. Main progress is put upon the following three topics: corona and solar wind, numerical method, prediction method.     

中间相沥青基碳纤维表面特性和界面粘结性能

针对高模量、高热导率中间相沥青基碳纤维复合材料界面性能弱等瓶颈问题,深入研究该类纤维表面特性及其与树脂的界面粘结性能。选取3种典型中间相沥青基碳纤维,测试分析其微观形貌、表面能和极性与色散分量、表面元素种类与含量,利用微脱黏方法表征中间相沥青基碳纤维与环氧树脂的界面剪切强度。研究结果表明:中间相沥青基碳纤维表面均存在明显沟槽结构,但其呈化学惰性,选用的中间相沥青基碳纤维与环氧树脂界面剪切强度最高约为50 MPa,明显低于聚丙烯腈基碳纤维;纤维表面能越高,尤其是极性分量越高,中间相沥青基碳纤维/环氧树脂界面剪切强度越大,这些结果揭示了中间相沥青基碳纤维与树脂基体界面性能主控因素。     

光伏发电系统中高升压比DC-DC变换器

光伏发电作为太阳能的重要应用方式正受到越来越广泛的关注,普遍采用前级DC-DC变换和后级逆变的结构。单相逆变器的输出电压通常为220 V(AC),这就要求前级DC-DC变换器具有很高的升压比。由于单级式DC-DC变换器难以满足要求,本文采用Boost变换器加ZVS全桥直流变压器的两级式结构。针对ZVS全桥直流变压器的不足,将LLC谐振网络应用于全桥直流变压器电路,提出了一种全桥LLC谐振直流变压器,从而实现整个负载范围内开关管的ZVS和整流二极管的ZCS。最后,分别制作了两台1 kW的原理样机进行实验验证,实验结果验证了理论分析的正确性。     

FGM零件快速原型制造中支撑自动生成模块设计

功能梯度材料是一种新型非均质材料,有着广泛的应用前景.传统的制造设备无法满足加工这种材料零件的要求,快速原型制造技术使得功能梯度材料零件的制造加工得以实现.支撑设计决定快速原型制造产品精度.针对功能梯度材料零件数字化设计制造中的支撑生成问题,采用了基于邻边排序的Stereo Lithography模型切片算法并提出了基于多边形布尔运算的支撑生成算法.根据功能梯度材料零件几何信息及零件内部材料分布信息实现支撑间距自适应改变,提高了快速原型产品精度.通过对支撑自动生成实例的分析,验证功能梯度材料零件快速原型制造中支撑自动生成算法的正确性.      

综合路由的无线传感器网络覆盖调度

利用目前公认为理论上最好的无线传感器网络集中式覆盖控制算法MCLC(Most-Constrained Least-Constraining),结合DD(Directed Diffusion)和LEACH(Low Energy Adaptive Clustering Hierarchy)路由协议,基于节点最小剩余能量调度覆盖集,观察最小剩余能量不同选取对节点能耗和均衡性以及网络生存期的影响.研究能耗均衡性和网络生存期的关系,提出了一种新的一般性能耗均衡的覆盖集调度的方法.仿真结果表明:所提方法可以有效提高网络生存期,同时为设计覆盖控制算法和覆盖集调度策略提供理论指导.