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排序方式: 共有128条查询结果,搜索用时 15 毫秒
1.
用正交试验与系列试验相结合的方法,研究了五元素风帆的气动特性及其各参数之间的最佳配合问題。设计的4个五元素风帆,均是由3个固定小翼、2个活动小翼及上下两块制流板所组成,但小翼的形状及分布曲线不同。 通过风洞试验,得到了各个风帆攻角与两个活动小翼转角之间的最佳配合,并对各帆的气动特性作了比较。试验结果表明,在最佳配合状态下,4个帆的升力系数可分别达到2.64、2.87、2.69和2.08,均比常规帆有较大的增长;而且,只要打开活动小翼,就能释放大部分风能,从而保证船舶在大风中的安全,这些帆的结构并不复杂,是具有广泛应用前景的高效帆具。 相似文献
2.
高益庆 《南昌航空工业学院学报》1994,(2):28-36
本文通过计算机模拟研究,结合气体折射率场的光验知识.考查了将Radon变换迭代法用于光学干涉层析计量含有遮挡物的三维折射率场的重建精度。作为一个应用实例,测量和计算了某一截面的气体温度分布,并与热电偶测量的值进行了比较。 相似文献
3.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(3):1070-1082
Solar sail halo orbits designed in the Sun-Earth circular restricted three-body problem (CR3BP) provide inefficient reference orbits for station-keeping since the disturbance due to the eccentricity of the Earth’s orbit has to be compensated for. This paper presents a strategy to compute families of halo orbits around the collinear artificial equilibrium points in the Sun-Earth elliptic restricted three-body problem (ER3BP) for a solar sail with reflectivity control devices (RCDs). In this non-autonomous model, periodic halo orbits only exist when their periods are equal to integer multiples of one year. Here multi-revolution halo orbits with periods equal to integer multiples of one year are constructed in the CR3BP and then used as seeds to numerically continue the halo orbits in the ER3BP. The linear stability of the orbits is analyzed which shows that the in-plane motion is unstable while the out-of-plane motion is neutrally stable and a bifurcation is identified. Finally, station-keeping is performed which shows that a reference orbit designed in the ER3BP is significantly more efficient than that designed in the CR3BP, while the addition of RCDs improve station-keeping performance and robustness to uncertainty in the sail lightness number. 相似文献
4.
Matteo Ceriotti Gregory May-Wilson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(9):2865-2877
The direction and magnitude of a solar sail acceleration are strongly related. For this reason, once the characteristic acceleration has been fixed, it is not possible to modulate the acceleration in a particular direction. In this work, a semi-analytical switching control law is derived, enabling a solar sail to emulate a smaller effective characteristic acceleration (without changes in geometry or optical properties); by periodically changing the pitch (cone) angle of the sail, in average over time, the acceleration produced by the sail matches exactly (in both direction and magnitude) that of a “smaller” sail. The range in which this is possible is determined, and the limitations on this range due to the size difference is computed. The method is validated on optimal Earth-Mars trajectories. 相似文献
5.
Ariadna Farrés Àngel Jorba 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this work we focus on the dynamics of a solar sail in the Sun–Earth Elliptic Restricted Three-Body Problem with solar radiation pressure. The considered situation is the motion of a sail close to the L1 point, but displacing the equilibrium point with the sail so that it is possible to have continuous communication with the Earth. In previous works we derived a station keeping strategy for this situation but using the Circular RTBP as a model. 相似文献
6.
Tommaso Pino Christian Circi Giovanni Vulpetti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3675-3690
A good model of solar-radiation pressure induced thrust is one of the key points in sailcraft trajectory design. The sail membrane’s local topographic deformations, i.e. wrinkles and creases, are among the main aspects that such a model should include. We have analyzed the influence of wrinkles/creases, as a whole, by measuring the related deformations on small samples of sail membrane, 2.5?μm thick, consisting of CP1 and physical-vapor-deposition Aluminum. Experimental outcomes from our laboratory facility have been processed, statistically investigated, and inserted into the lightness vector formalism. We have used such formalism for accurate sailcraft trajectory computation via a non-ideal reflection sail thrust model. Finally, we computed the deviations of wrinkled-sail sailcraft final orbital states with respect to the no-wrinkle sail final orbital ones for a circular to circular 2D inward transfer. The radii of the orbits are 1?AU and the semi-major axis of Mercury, respectively. It appears that sail wrinkles and creases are no longer negligible in the sailcraft trajectory design. 相似文献
7.
太阳帆航天器动力学建模与求解 总被引:2,自引:2,他引:2
太阳帆航天器动力学建模与求解是姿态控制与结构振动抑制的基础,具有重要的理论与工程意义。针对带有控制杆和控制叶片的太阳帆航天器,进行结构的合理简化。应用矢量力学基本原理,推导出考虑弹性振动的太阳帆航天器姿态动力学方程,再对其进行简化,分别得到基于控制叶片和控制杆的两类太阳帆航天器的姿态动力学方程,联立太阳帆支撑杆振动方程,结合非约束模态的定义对运行于超地球同步转移轨道的太阳帆航天器动力学方程进行了求解及分析,结果表明所建立的太阳帆动力学模型可准确地描述柔性太阳帆航天器的动力学特性。 相似文献
8.
铰链展开式构型航天器设计及其动力学仿真 总被引:3,自引:0,他引:3
基于航天器结构的模块化设计概念,设计了一种空间可展开航天器模块化结构构型,即铰链展开式构型。利用虚拟样机技术,建立了模块化本体和太阳翼虚拟样机模型。在空间失重环境下,分析了模块化本体和太阳翼在3种展开顺序下(本体各模块和太阳翼同时展开、太阳翼先展开本体各模块后展开和本体各模块先展开太阳翼后展开)对航天器姿态的影响,同时对比了不同扭簧参数对姿态角和展开时间的影响。仿真结果表明该模型可为未来高机动、多型态、多用途自适应变构型航天器的设计以及空间姿态控制提供技术支持和借鉴。 相似文献
9.
研究基于遗传算法的太阳帆行星际转移轨道的全局优化问题.通过极小值原理推导了太阳帆全局优化控制律,并以太阳帆飞行时间最短为优化目标函数,运用遗传算法对发射时间、到达时间和协态变量初值进行参数优化设计.为了解决轨道转移这一多约束优化问题,在遗传算法中加入动态罚函数.在此理论基础上作了从地球同步轨道出发到火星同步轨道转移和从地球出发与火星交会两个算例,仿真结果表明了该方法在太阳帆转移轨道全局优化中的有效性. 相似文献
10.
本文试验研究了一种可控环量帆翼,利用壁面切向喷流来移动帆翼圓尾缘分离点位置,可获得比普通帆翼更高的推力系数。文中介绍了展弦比为1的三维可控环量帆翼的试验研究。试验表明,这种可控环量帆翼在较小的喷流动量系数下,即可获得较大的升力增益。在喷流动量系数 C_μ=0.1时,零攻角升力系数已达0.9,在有攻角的情况下,升力系数最大可达2.2。同时,由于帆翼尾部壁面团向喷流的 Coanda 效应,这种可控环量帆翼的阻力亦较大。在喷流动量系数 C_μ=0.1时,零攻角阻力系数为0.3。文章对这种可控环量帆翼在船舶上的应用进行了讨论,并对其性能的进一步改进作了分析和探讨。 相似文献