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India in Asia and Brazil in Latin America are regarded as the most promising global economies. This paper examines the openings and possibilities for space technology collaboration between India and Latin American states under the larger rubric of science and technology collaboration. While the distance and language barriers between the two regions have proved a hindrance in the past, the paper proceeds with an assumption that, in the 21st century, such barriers should not be a limitation on developing strategic, economic, and science and technology partnerships among nation-states. The paper argues that the Latin American states are keen to have their own satellites because of their significant utility in the socioeconomic sector and this offers an opportunity to India to use cooperation in space technologies as a powerful tool for engagement in Latin America. 相似文献
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S. M. Giuliatti Winter O. C. Winter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,33(12):2298-2302
The system formed by the F ring and two close satellites, Prometheus and Pandora, has been analysed since the time that Voyager visited the planet Saturn. During the ring plane crossing in 1995 the satellites were found in different positions as predicted by the Voyager data. Besides the mutual effects of Prometheus and Pandora, they are also disturbed by a massive F ring. Showalter et al. [Icarus 100 (1992) 394] proposed that, the core of the ring has a mass which corresponds to a moonlet varying in size from 15 to 70 km in radius which can prevent the ring from spreading due to dissipative forces, such as Poynting–Robertson drag and collisions. We have divided this work into two parts. Firstly we analysed the secular interactions between Prometheus–Pandora and a massive F ring using the secular theory. Our results show the variation in eccentricity and inclination of the satellites and the F ring taking into account a massive ring corresponding to a moonlet of different sizes. There is also a population of dust particles in the ring in the company of moonlets at different sizes [Icarus 109 (1997) 304]. We also analysed the behaviour of these particles under the effects of the Poynting–Robertson drag and radiation pressure. Our results show that the time scale proposed for a dust particle to leave the ring is much shorter than predicted before even in the presence of a coorbital moonlet. This result does not agree with the confinement model proposed by Dermott et al. [Nature 284 (1980) 309]. In 2004, Cassini mission will perform repeated observations of the whole system, including observations of the satellites and the F ring environment. These data will help us to better understand this system. 相似文献
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带柔性部件卫星耦合动力学建模理论及仿真 总被引:1,自引:0,他引:1
本文利用Jourdain速度变分原理和集中质量有限元法建立了太阳帆板变形运动与星体大范围刚体运动之间的相互耦合的程式化动力学方程;用数值方法仿真了系统的动力学性能,给出了三种卫星动力学模型并比较了三种卫星动力学模型之间的差异;指出了目前工程实际中所用动力学模型的不足,进而提出了合理的卫星耦合动力学模型。 相似文献
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编队飞行小卫星空间状态测量方法研究 总被引:1,自引:0,他引:1
介绍了编队飞行小卫星特点,提出了小卫星空间状态测量方案。着重论述了星间相对状态自主测量方法,计算了伪码和载波相位跟踪环路、时钟基准频差以及测量设备延迟带来的星间相对距离测量误差,讨论了降低误差的方法。在对误差项进行综合分析后,得出相对距离测量误差可达到厘米级的结论。 相似文献