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11.
人造地球卫星初轨计算的单位矢量法 总被引:5,自引:1,他引:5
本文在建立两组单位矢量系统R*,S*,φ*和ρ*,A*,h*的基础上,给出了初轨计算的新的条件方程形式以及对不等精度、不同类型的观测资料的加权处理方法,这对充分发挥高精度测距资料ρ和测速资料ρ·的作用十分有利。实测计算表明,本方法基本解决了初轨计算中轨道半长轴不易定准的困难,并具有定轨精度高、适用范围广、稳定性能好等优点,对静止卫星转移轨道入轨段超短弧段测量资料的初轨计算,作用尤为明显。 相似文献
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简要说明了风云一号(FY-1)极轨气象卫星的总体情况。介绍了FY-1C星运行5年。D星运行2年后的测控、电源、热控、敖传、扫描辐射计和星载数据收集与分发(DCDS)分系统、有效载荷空间粒子成分监测器。以及姿控和星载计算机的在轨运行情况。在轨测试结果表明,两星的在轨运行、功能和性能符合任务书的要求。最后总结了长寿命高可靠稳定优质业务运行的FY-1C,D星的创新点、主要成绩,并给出了部分应用情况。 相似文献
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FY—1C极轨气象卫星的进展 总被引:3,自引:1,他引:3
在概述美国和俄罗斯等国外极轨气象卫星发展概况的基础上,介绍了中国极轨与静止轨道两种气象卫星的业务应用卫星体系,重点介绍了“风云一号”(02星)即FY-1C极轨气象卫星的任务、总体设计、技术特点、关键技术以及所取得的进展。最后简述了新一代有轨气象卫星FY-3的发展设想。 相似文献
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自1984年开始,中国研制的系列远地点发动机共9次参加卫星发射,均获成功,表现出很高的可靠性,高空比冲达到2834N·s/kg,质量比为0.895,性能达到了先进水平。该文介绍了远地点发动机的特点、技术水平和主要经验。其中采用丁羟推进剂、玻璃纤维壳体和碳/碳复合材料喉衬被证明为成功的技术选择。在研制过程中,在高空比冲的预示和测量,玻璃纤维壳体基体树脂的研制,高空点火和安全点火机构的研制,防止发动机自旋引起的烧蚀等技术问题方面,积累了丰富经验。对于在高空工作的发动机具有现实参考意义。 相似文献
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星载SAR模糊特性及其工程设计 总被引:4,自引:0,他引:4
分析了星载合成孔径雷达产生模糊的机理及其与系统参数的关系,叙述了在宽广可视观测带曲,达到较好图像模糊度特性的优化设计原则,并提出了星载SAR模糊性能的工程设计方法。 相似文献
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S. M. Krimigis D. G. Mitchell D. C. Hamilton S. Livi J. Dandouras S. Jaskulek T. P. Armstrong J. D. Boldt A. F. Cheng G. Gloeckler J. R. Hayes K. C. Hsieh W.-H. Ip E. P. Keath E. Kirsch N. Krupp L. J. Lanzerotti R. Lundgren B. H. Mauk R. W. McEntire E. C. Roelof C. E. Schlemm B. E. Tossman B. Wilken D. J. Williams 《Space Science Reviews》2004,114(1-4):233-329
The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R
S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm2 sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm2 sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm2 sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm2 sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R
S every 2–3 h (every ∼10 min from ∼20 R
S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date. 相似文献
17.
飞行任务对卫星轨道提出指标要求,这些指标决定了卫星轨道参数的容许偏差范围。结合太阳同步(准)回归轨道卫星的轨道特性,针对覆盖重叠率、太阳同步等指标,使用解析方法讨论了大气阻力摄动影响下轨道参数的容许偏差,通过分析可以初步确定轨道控制策略及能量需求,最终为轨道保持方法的设计提供参考和依据。 相似文献
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编队飞行卫星群构型保持及初始化 总被引:3,自引:0,他引:3
导出了基于相对轨道要素的编队飞行卫星群轨道相对运动控制的轨道机动方程;提出了编队飞行卫星群轨道相对运动控制的轨道机动控制策略,利用不同方向的脉冲控制相对运动的轨道参数,包括轨道平面内机动和轨道平面外机动控制。根据相对轨道要素的变轨机动控制,进行编队飞行卫星群构型的初始化。这样的构型初始化可以视作一次特殊的变轨机动控制,很容易实现编队飞行构型的初始化机动。 相似文献