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921.
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923.
The Current Systems of the Jovian Magnetosphere and Ionosphere and Predictions for Saturn 总被引:3,自引:0,他引:3
Margaret Galland Kivelson 《Space Science Reviews》2005,116(1-2):299-318
924.
The Geospace Double Star Project (DSP) consists of two small satellites operating in the near-earth equatorial and polar regions, respectively. The goals of DSP are: (1) to provide high-resolution field, particle, and wave measurements in some important near-earth active regions which have not been covered by current ISTP missions, such as the near-earth plasma sheet and its boundary layer, the ring current, the radiation belts, the dayside magnetopause boundary layer, and the polar region; (2) to investigate the trigger mechanisms of magnetic storms, magnetospheric substorms, and magnetospheric particle events,as well as the responses of geospace storms to solar activities and interplanetary disturbances; (3) to set up the models describing the spatial and temporal variations of the near-earth space environment.To realize the above goals, the equatorial satellite TC-1 and the polar satellite TC-2 will accommodate, respectively, eight instruments on board. TC-1was launched successfully in December 2003 while the polar satellite (TC-2)will be launched in July 2004. The orbit of the equatorial satellite TC-1 consists of a perigee at 550 km, an apogee at 60 000 km, and an inclination of about 28.5; while the orbit of the polar satellite will have a perigee of 700 km, an apogee of 40 000 km, and an inclination of about 90. The two satellites will take coordinated measurements with Cluster Ⅱ and will first form a "six-point exploration" in geospace.The operational status of TC-1 are introduced in this paper. 相似文献
925.
航天发射用磁悬浮助推发射系统概念研究 总被引:4,自引:2,他引:4
针对日益增加的航天发射成本问题和安全、可靠、低成本航天发射方式的需求,阐述了磁悬浮助推发射概念及其优越性.初步分析了磁悬浮助推发射系统组成及各分系统功能.通过比较电磁悬浮(EMS)和超导电动(EDS)两种磁悬浮系统性能,结果表明EDS是更适合于磁悬浮助推发射的磁悬浮系统方案.通过助推发射能量需求初步分析,直线电机加速能量供给系统是难题之一,需要重点解决.采用飞行弹道分析方法,说明地面助推水平起飞单级入轨运载器方案的可行性及特点.与其它航天助推发射方式比较,磁悬浮助推发射在提高入轨载荷和降低发射成本方面具有优势. 相似文献
926.
David S. Myers 《Space Policy》1985,1(3):298-310
A state's posture on remote sensing of the Earth by orbiting satellites varies depending upon whether it is a ‘sensing’ or a ‘sensed’ state, upon its present economic status, and upon its economic and political history. This article considers the international legal questions related to remote sensing and discusses the political aspects with special emphasis upon the views of the Third World. The author concludes that, unless Third World states and others who support them alter their views somewhat, it is probable that remote sensing of natural resources will continue without specific legal guidelines. 相似文献
927.
M. F. Kessler 《Space Science Reviews》1995,74(1-2):57-65
The Infrared Space Observatory (ISO), a fully approved and funded project of the European Space Agency (ESA), is an astronomical satellite, which will operate at wavelengths from 2.5–240 m. ISO will provide astronomers with a unique facility of unprecedented sensitivity for a detailed exploration of the universe ranging from objects in the solar system right out to distant extragalactic sources. The satellite essentially consists of a large cryostat containing at launch over 2000 litres of superfluid helium to maintain the Ritchey-Chrétien telescope, the scientific instruments and the optical baffles at temperatures between 2 K and 8 K. The telescope has a 60-cm diameter primary mirror and is diffraction-limited at a wavelength of 5 m. A pointing accuracy of a few arc seconds is provided by a three-axis-stabilisation system consisting of reaction wheels, gyros and optical sensors. ISO's instrument complement consists of four instruments, namely: an imaging photo-polarimeter (2.5–240 m), a camera (2.5–17 m), a short wavelength spectrometer (3–45 m) and a long wavelength spectrometer (43–196 m). These instruments are being built by international consortia of scientific institutes and have been delivered to ESA for in-orbit operations. ISO will be launched in September 1995 by an Ariane 4 into an elliptical orbit (apogee 70000 km and perigee 1000 km) and will be operational for at least 18 months. In keeping with ISO's role as an observatory, the majority of its observing time is being made available to the general astronomical community via a Call for Observing Proposals. 相似文献
928.
Alfano-Negron(1993)提出的空间目标接近分析算法将最小相对距离及其对应时刻和进出误差椭球时刻的求解问题均转化为插值多项式求根问题.A-N算法在判断三次多项式根的存在性、筛选合理实根时存在缺陷,可能导致多余计算.由A-N算法提出的准则不能直接计算插值时间步长并可能导致丢根,对此根据多项式插值误差理论提出了一种自适应的插值时间步长选取方法.相比原始A-N算法,完善后的A-N算法计算结果更加可靠.与精确的逐秒比较结果相比,改善后的A-N算法计算速度远高于逐秒比较,具有较高精度,更适合于有实时计算要求的任务. 相似文献
929.
930.
固体发动机高空模拟试验瞬时真空推力的修正分析与计算 总被引:1,自引:0,他引:1
分析了当环境压强分布不均时,用固体发动机高空模拟试验实测瞬时推力修正计算瞬时真空推力问题;同时,根据一种发动机(SRMI)的试验现象,分析了引起发动机推力偏斜的因素,就这些因素对推力的影响给出了定量计算公式。 相似文献