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The Canadian Geophysical Long Baseline Interferometer

Published online by Cambridge University Press:  03 August 2017

J.L. Yen ,
P. Leone ,
G.A. Watson ,
R. Wiedfeldt ,
J. Zao ,
W.H. Cannon ,
P. Mathieu ,
H. Tan ,
J. Popelar  and
J. A. Galt
J.L. Yen
Affiliation:
University of Toronto, Toronto, Ontario, Canada
P. Leone
Affiliation:
University of Toronto, Toronto, Ontario, Canada
G.A. Watson
Affiliation:
University of Toronto, Toronto, Ontario, Canada
R. Wiedfeldt
Affiliation:
University of Toronto, Toronto, Ontario, Canada
J. Zao
Affiliation:
University of Toronto, Toronto, Ontario, Canada
W.H. Cannon
Affiliation:
York University, Toronto, Ontario, Canada
P. Mathieu
Affiliation:
York University, Toronto, Ontario, Canada
H. Tan
Affiliation:
York University, Toronto, Ontario, Canada
J. Popelar
Affiliation:
Department of Energy, Mines & Resources, Ottawa, Ontario, Canada
J. A. Galt
Affiliation:
Dominion Radio Astrophysical Observatory, Penticton B.C., Canada

Extract

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A new VLBI system has been developed and put into operation. The system has three distinctive characteristics as compared with current VLBI practice, namely, the use of a wavefront clock at each station, the capability of a burst mode operation with high speed sampling, and the use of multiple 12 Mb/s data recording channels on commercial VCR's. The main use of the system is to be in geophysical investigations where these new features may prove of value.

Type
Instrumentation and Analysis
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 489 - 490
Copyright
Copyright © Reidel 1988