VLBI stations
Development of VLBI stations dedicated to the KSP including a new building
started in FY1993. The observation system consists of three parts, i.e.,
(1) data acquisitions (2) system monitoring, and (3) remote controlling.
Current timetable of development of each KSP station is as follows.
Timeable of Each Station's Development
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KOGANEI KASHIMA MIURA TATEYAMA
year Center Sub-Center
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Data acquisition Data acquisition
Mar., 1995
System System Data
monitoring monitoring acquisition
Concentrated (System
controlling monitoring?)
July, 1995
1996 Concentrated System Data
controlling monitoring acquisition
System
monitoring
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Data processing and analysis system
VLBI data are processed and analyzed routinly at Koganei Central station.
New correlator dedicated to the KSP is under development. So is
software for data processing and analysis. Presently tests combining both
hardware and software are going on. We will enter the routine operation
phase of the correlator in FY1995.
Test observations on the Koganei-Kashima baseline
We carry out test observations on this baseline to check the whole
performance of the KSP VLBI system. First fringes were succesfully detected
on July 25, 1994. The first full 24-hour experiment was carried out on
August 29, 1994. Daily observations, whose main purpose
is system performance check, have been carried out since
January, 1995.