Overview of the experiment system. 1. The main VLBI station at Kashima.

Details Overview of the experiment system. 1. The main VLBI station at Kashima. Overview of the experiment system. 1. The main VLBI station at Kashima.

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jcrl...42....5i&link_type=abstract

J. Commun. Res. Lab., Vol. 42, No. 1, p. 5 - 14

Astronomy and Astrophysics

Astronomy

Antennas: Vlb Interferometry, Network: Vlb Interferometry

Scientific paper

The Western Pacific VLBI Network was mainly organized by the VLBI stations of the Communications Research Laboratory (CRL), Kashima, Marcus Island and Minamidaito Island, and Shanghai. The 34 m antenna built at CRL's Kashima Space Research Center in 1988 has been used as the main station of the Western Pacific VLBI Network. This antenna was constructed as one of the largest antennas in Japan and its main purpose is precise geodesy. It has many advanced functions for this purpose but was also designed for multipurpose observations. It is therefore also the main tool in precise space and time measurement projects, such as the Earth rotation measurement VLBI, millisecond pulsar timing observations, and radio astronomical observations.

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