“集群-集群”VLBI模式的相位参考

M.J. Rioja , E. Stevens , L. Gurvits , W. Alef , R.T. Schilizzi , T. Sasao , Y. Asaki
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引用次数: 9

摘要

具有多个天线单元的站点之间的VLBI,由一个共同的本地振荡器馈电,具有以一种新的方式求解天体测量和大地测量参数的前景。Cluster-Cluster观测模式允许在从一个站点到另一个站点的子元素之间的单独“子基线”上同时观测多个源。微分分析得益于完全消除了非几何贡献的时间结构(例如仪器项和传播介质)。介绍了1995年6月WSRT和VLA阵列利用该技术对观测结果进行分析的现状。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Phase-referencing in “cluster-cluster” VLBI mode

VLBI between sites with multiple antenna elements, fed from a common local oscillator, holds the prospect of solving for astrometric and geodetic parameters in a new way. The Cluster-Cluster observing mode allows simultaneous observations of multiple sources on the separate “sub-baselines” between sub-elements from one site to the other. The differential analysis benefits from the total cancelation of the temporal structure of the non-geometric contributions (e.g. instrumental terms and the propagation medium). We describe the current status of the analysis of observations in June 1995 using this technique with the WSRT and VLA arrays.

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