  The VSOP mission is a Japanese-led project to study radio sources with
sub-milliarcsec resolution using an orbiting 8 m telescope, HALCA, along with
global arrays of Earth-based telescopes. Approximately 25% of the observing
time is devoted to a survey of compact AGN which are stronger than 1 Jy at 5
GHz-the VSOP AGN Survey. This paper, the third in the series, presents the
results from the analysis of the first 102 Survey sources. We present high
resolution images and plots of visibility amplitude versus projected baseline
length. In addition, model-fit parameters to the primary radio components are
listed, and from these the angular size and brightness temperature for the
radio cores are calculated. For those sources for which we were able to
determine the source frame core brightness temperature, a significant fraction
(53 out of 98) have a source frame core brightness temperature in excess of
10^12 K. The maximum source frame core brightness temperature we observed was
1.2 X 10^13 K. Explaining a brightness temperature this high requires an
extreme amount of relativistic Doppler beaming. Since the maximum brightness
temperature one is able to determine using only ground-based arrays is of the
order of 10^12 K, our results confirm the necessity of using space VLBI to
explore the extremely high brightness temperature regime.
