C.Boucher ,左传惠

摘要(Abstract)：

当前,大地测量在量测和模型两方面都已达到这样一种精度,即地球大小、形状和重力场随时间的变动,在地球动力学中基本上都必须加以考虑。因此,在描述一个地面参照系的点位和重力场函数时,应同时描述它的随时间的变动。为此,在模型中必须顾及到相对论效应。现代万有引力理论,如爱因斯坦的广义相对论,在太阳系中可表达为参数化的后—牛顿(PPN)(Parametrized Post-newtonian)公式。在地球动力学中的相对论模型就应对质点运动这样一类基本问题给出一个令人满意的解答。相对论效应也存在于地面参考系和重力场的定义之中。它们也广泛出现在地面测量(重力测量、惯性技术)和空间测量(激光测卫、激光测月、VLBI、卫星无线电电子跟踪……)之中。

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作者(Author): C.Boucher ,左传惠

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