  In February 1997 the Japanese radio astronomy satellite Halca was launched to
provide the space-bourne element for the VSOP mission. Approximately
twenty-five percent of the mission time has been dedicated to the VSOP Survey,
a 5 GHz survey of bright, compact AGN. Both the final, calibrated, high
resolution images and plots of visibility amplitude versus uv distance for the
first 102 of the sources have been prepared and has been submitted. Papers on
the methods and the models from fitting the cumulative {\em uv} amplitudes will
also be submitted. The analysis of the second half is well underway.
