Hinteregger H F, Shapiro I I, Robertson D S, Knight C A, Ergas R A, Whitney A R, Rogers A E, Moran J M, Clark T A, Burke B F
Science. 1972 Oct 27;178(4059):396-8. doi: 10.1126/science.178.4059.396.
Very-long-baseline interferometry experiments, involving observations of extragalactic radio sources, were performed in 1969 to determine the vector separations between antenna sites in Massachusetts and West Virginia. The 845.130-kilometer baseline was estimated from two separate experiments. The results agreed with each other to within 2 meters in all three components and with a special geodetic survey to within 2 meters in length; the differences in baseline direction as determined by the survey and by interferometry corresponded to discrepancies of about 5 meters. The experiments also yielded positions for nine extragalactic radio sources, most to within 1 arc second, and allowed the hydrogen maser clocks at the two sites to be synchronized a posteriori with an uncertainty of only a few nanoseconds.
1969年进行了甚长基线干涉测量实验,该实验涉及对河外射电源的观测,目的是确定马萨诸塞州和西弗吉尼亚州天线站点之间的矢量间距。通过两个独立实验估算出了845.130公里的基线。所有三个分量的结果相互之间的误差在2米以内,与一项特殊大地测量的长度误差在2米以内;测量和干涉测量确定的基线方向差异对应约5米的偏差。这些实验还得出了九个河外射电源的位置,大多数位置的误差在1弧秒以内,并使得两个站点的氢脉泽时钟能够事后同步,不确定度仅为几纳秒。