Key Stone Project

Regular VLBI observation in the Keystone Project is terminated at the end of November, 2001 since the project is time-limited. We appreciate your kind cooperation. Note that our data base is still obtainable via internet.

KSP VLBI Data / Baseline Length

This page presents the estimated baseline lengths based on the latest solution done at Fri Mar 22 08:21:42 JST 2002.

Since the beginning of July in 2001, the geodetic solution might be suffered by radio interferences. The data in this period is under investigation. Hence, the results are subject to change by the re-analysis. Thank you for your understanding.

Press here to see the ASCII data file.

KASHIMA-KOGANEI Baseline (since August, 1994)

KASHIMA-KOGANEI Baseline (since January, 2000)

KASHIMA-MIURA Baseline (since May, 1995)

KASHIMA-MIURA Baseline (since January, 2000)

KASHIMA-TATEYAMA Baseline (since September, 1996)

KASHIMA-TATEYAMA Baseline (since January, 2000)

KOGANEI-MIURA Baseline (since May, 1995)

KOGANEI-MIURA Baseline (since January, 2000)

KOGANEI-TATEYAMA Baseline (since September, 1996)

KOGANEI-TATEYAMA Baseline (since January, 2000)

TATEYAMA-MIURA Baseline (since September, 1996)

TATEYAMA-MIURA Baseline (since January, 2000)

Please feedback your comments and requests to yosh(AT) by e-mail. Information provided from this WWW server may be freely extracted for personal use. Any HTML documents on this WWW server may be pointed to from your own personal pages without permission. If you wish to redistribute or publish any of the information provided here, you have to request permission in advance. Please consult with the Key Stone Project's representatives by sending your request to the e-mail address written above.

Last Update: Fri Mar 22 08:21:42 JST 2002

Key Stone Project Homepage
Radio Astronomy Applications Section Homepage