通过无线电干扰测量测量的跨大陆基线和地球的旋转
概括
非常长基线干涉测量 (VLBI) 实验在测量基线长度和确定地球地球时取得了高精度.
科学领域:
- 天文学和地球物理学
- 无线电天文学 无线电天文学
- 地质测量是指地质测量.
背景情况:
- 非常长基线干涉测量 (VLBI) 是一种使用广泛分离的射电望远镜观察遥远的天文物体的技术.
- 准确地测量地球的旋转和结构对于各种科学学科至关重要.
研究的目的:
- 为了评估VLBI的精度,用于测量地质测量.
- 用VLBI数据确定宇宙时间和极运动的变化.
- 为了调查检测固体地球潮的情况.
主要方法:
- 在1972年至1973年间进行了9次VLBI实验,使用距离3900公里的射电望远镜.
- 分析收集的无线电天文学数据来计算基线长度,宇宙时间和极地运动.
- 将VLBI结果与通过光学方法获得的结果进行比较.
主要成果:
- 实现了基线长度测量,根-平方平均偏差小于20厘米 (分数分布为~5x10^-8).
- 与光学方法相比,确定了宇宙时间和极运动,其平方根平均分散分别为2.9毫秒和1.3米.
- 观察到固体地球潮的证据,尽管振幅估计是不可行的.
结论:
- 在地理测量应用中,VLBI表现出高精度,包括精确的基线长度确定.
- 该研究证实了VLBI在准确跟踪地球旋转和位置变化的能力.
- 显示了固土潮检测,需要使用改进的方法进行进一步的调查.
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