Abstract
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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
