共查询到20条相似文献,搜索用时 31 毫秒
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The Satellite Instructional Television Experiment (SITE) was a unique effort aimed at studying the possibilities of satellite broadcasting for education and national development. This one-year joint India-USA project was carried out in 1975–1976 using the ATS-6 spacecraft. This paper briefly describes the experiment and its major findings. It goes on to distill the learning experiences derived from SITE and analyses the extent to which these have influenced the design and configuration of India's domestic satellite system, INSAT. INSAT-1B, which will serve as a replacement for the short-lived INSAT-1A, will be launched shortly and will be operational by the end of 1983. Its payload includes two S-band TV transponders capable of broadcasting directly to augmented TV sets. The paper examines which lessons of SITE are being applied in the planning and operationalisation of the TV system and discusses why others are not being taken account of. Major issues confronting TV system planners in developing countries like India are highlighted and the possible role of satellite broadcasting discussed in this context. The paper concludes by outlining an “ideal scenario” for a large, multilingual country like India, towards which TV planners could attempt to strive. 相似文献
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The problem of optimization of a spacecraft transfer to the Apophis asteroid is investigated. The scheme of transfer under analysis includes a geocentric stage of boosting the spacecraft with high thrust, a heliocentric stage of control by a low thrust engine, and a stage of deceleration with injection to an orbit of the asteroid’s satellite. In doing this, the problem of optimal control is solved for cases of ideal and piecewise-constant low thrust, and the optimal magnitude and direction of spacecraft’s hyperbolic velocity “at infinity” during departure from the Earth are determined. The spacecraft trajectories are found based on a specially developed comprehensive method of optimization. This method combines the method of dynamic programming at the first stage of analysis and the Pontryagin maximum principle at the concluding stage, together with the parameter continuation method. The estimates are obtained for the spacecraft’s final mass and for the payload mass that can be delivered to the asteroid using the Soyuz-Fregat carrier launcher. 相似文献
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S. Yu. Ulybyshev 《Cosmic Research》2016,54(4):303-312
We present a method for designing nonuniform satellite systems for continuous global coverage using a combination of equatorial and near-polar satellite segments in circular orbits. Equations are derived to determine the basic design parameters of the satellite system itself and the conditions of its closure at the joint of near-polar and equatorial segments. We analyze specific features of near-polar and equatorial satellite systems and their advantages and disadvantages compared with existing classes of near-polar phased and kinematically correct satellite systems. We estimate the minimum required number of spacecrafts in satellite systems for a given fold of coverage and present calculated dependences for classes of near-polar phased and equatorial satellite systems with different types of closure. For the class of kinematically correct satellite systems, we analyze the characteristics of systems with a minimum spacecraft flight height and reveal that the number of satellites in the orbital plane depends on the flight height for different folds of coverage. We bring examples of the best near-polar equatorial satellite systems of global coverage for different folds and a class of satellite systems with a fixed number of spacecrafts and orbital planes in them. 相似文献
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《Acta Astronautica》2001,48(5-12):767-776
Our laboratory is proceeding with a project to design and fabricate a nano satellite named “Gekkabijin” as “CanSat” project. This project was agreed at USSS'98 as a Japan-U.S. joint venture to make satellites for educational purpose. CanSat is, as can be imaged from the name, a Coke can shaped and sized satellite. Our CanSat “Gekkabijin” was designed to deploy a thin flexible membrane using centrifugal force. Before we can launch a CanSat into space, we had a chance to put it into sub-orbit with a support from a U.S. amateur rocket group in the name of ARLISS Project. ARLISS Project has already taken place twice in 1999 and 2000 and we carried out 6 missions. This paper describes the objectives, satellite design, experiment results and lessons learned of University of Tokyo CanSat Project. 相似文献
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Health scorecard of spacecraft platforms: Track record of on-orbit anomalies and failures and preliminary comparative analysis 总被引:1,自引:0,他引:1
Choosing the “right” satellite platform for a given market and mission requirements is a major investment decision for a satellite operator. With a variety of platforms available on the market from different manufacturers, and multiple offerings from the same manufacturer, the down-selection process can be quite involved. In addition, because data for on-obit failures and anomalies per platform is unavailable, incomplete, or fragmented, it is difficult to compare options and make an informed choice with respect to the critical attribute of field reliability of different platforms. In this work, we first survey a large number of geosynchronous satellite platforms by the major satellite manufacturers, and we provide a brief overview of their technical characteristics, timeline of introduction, and number of units launched. We then analyze an extensive database of satellite failures and anomalies, and develop for each platform a “health scorecard” that includes all the minor and major anomalies, and complete failures—that is failure events of different severities—observed on-orbit for each platform. We identify the subsystems that drive these failure events and how much each subsystem contributes to these events for each platform. In addition, we provide the percentage of units in each platform which have experienced failure events, and, after calculating the total number of years logged on-orbit by each platform, we compute its corresponding average failure and anomaly rate. We conclude this work with a preliminary comparative analysis of the health scorecards of different platforms.The concept of a “health scorecard” here introduced provides a useful snapshot of the failure and anomaly track record of a spacecraft platform on orbit. As such, it constitutes a useful and transparent benchmark that can be used by satellite operators to inform their acquisition choices (“inform” not “base” as other considerations are factored in when comparing different spacecraft platforms), and by satellite manufacturers to guide their testing and reliability improvement programs. Finally, it is important to keep in mind that these health scorecards should be considered dynamic documents to be updated on a regular basis if they are to remain accurate and relevant for comparative analysis purposes, as new information will impact their content. 相似文献
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20世纪上海航天器电源技术的进展 总被引:7,自引:2,他引:7
较为系统地介绍了作为航天器电源的锌银电池组和硅太阳电池阵/镉镍蓄电池组联合供电系统的组成、主要性能参数及其技术特点。阐述了近半个世纪以来,上海航天技术研究院在航天器电源研制技术方面所取得的成就及其在国内卫星、飞船和国外卫星领域的应用情况。指出了航天器电源技术今后的发展方向。 相似文献
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低地球轨道航天器对接放电研究 总被引:2,自引:1,他引:1
文章介绍了低轨道航天器对接放电的产生机理,通过模拟试验、电路仿真和理论分析,研究了低轨道航天器对接产生静电放电的可能性、条件、放电强度、持续时间及其影响,并提出防止静电放电危害的措施,为工程应用提出参考建议。 相似文献
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卫星充电和尾迹效应会对周围的等离子体造成扰动,进而影响星上电磁和等离子测量 载荷的测量精度。利用卫星与等离子体相互作用模拟软件SPIS,并采用DEMETER卫星的 一组在轨测试的等离子参数,采用粒子分室法模拟了低轨道卫星的尾迹效应特性。结果显示 ,卫星的表面充电电位为-0.72 V,负的充电电位一定程度上减小了尾迹效应的影响,尾 迹效应对等离子体的扰动在尾迹一侧约为2.5 m,离子撞击侧约为0.7 m,其余两个 侧面约为1.1 m,即等离子鞘层呈桃形分布,且在尾迹区存在离子浓度为零的空白区和 浓度较小的稀薄区,而在尾迹区也是电子浓度的稀薄区,但不存在电子浓度为零的空白区。
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The problem of optimization of the interplanetary trajectory of flight for a multistage spacecraft with high- and low-thrust engines into the Jupiter satellite orbit is considered. Low-thrust engines (stationary plasma engines) are used on a heliocentric flight segment. Their operation is maintained with electric power supply from solar batteries. The principal feasibility of the realization of such a project is shown, and estimations of the mass of a spacecraft placed into Jupiter's satellite orbit are presented. 相似文献
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许多空间实验和电子计算机预测已经揭示,在极光电子环境中大型航天器的充电电位会高达6000--7000V。对采用大功率太阳阵的航天器而言,其相对于空间等离子体的悬浮电位将因太阳阵工作电压的提高而增加。例如表面材料因遭受离子轰击和电弧放电而老化、剥蚀、由于材料再沉积而使表面污染增加以及航天器电子系统因静电放电而受到严重的干扰和破坏等。因而对载人航天和长寿命空间站而言,解决航天器带电问题不可等闲视之。对 相似文献
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