有效载荷(计算)
维纳斯
地球轨道
时间轴
计算机科学
行星
天体生物学
定轨
行星科学
大气(单位)
航空航天工程
轨道(动力学)
无线电掩星
环境科学
气象学
遥感
物理
卫星
地质学
天文
航天器
工程类
地理
电离层
计算机网络
网络数据包
考古
作者
D. V. Titov,H. Svedhem,D. Koschny,Raymond Hoofs,S. Barabash,Jean‐Loup Bertaux,P. Drossart,V. Formisano,B. Häusler,Oleg Korablev,W. J. Markiewicz,D. Nevejans,M. Pätzold,G. Piccioni,T.L. Zhang,Donald Merritt,Olivier Witasse,Joe Zender,Andrea Accomazzo,Mark Sweeney,D. Trillard,Miho Janvier,A. Clochet
标识
DOI:10.1016/j.pss.2006.04.017
摘要
Venus Express is the first European mission to the planet Venus. Its payload consists of seven instruments and will investigate the atmosphere, the plasma environment, and the surface of Venus from orbit. Science planning is a complex process that takes into account requests from all experiments and the operational constraints. The planning of the science operations is based on synergetic approach to provide good coverage of science themes derived from the main mission goals. Typical observations in a single orbit—so-called "science cases" are used to build the mission science activity plan. The nominal science mission (from June 4, 2006 till October 2, 2007) is divided in nine phases depending on observational conditions, occurrences of the solar and Earth occultation, and particular science goals. The observation timelines for each phase were developed in a coordinated way to optimize the payload activity, maximize the overall mission science return, and to fit into the available mission budgets.
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