  The VSOP mission is a Japanese-led project to study radio sources with
sub-milliarcsecond angular resolution using an orbiting 8-m telescope, HALCA
and global arrays of Earth-based telescopes. Approximately 25% of the observing
time has been devoted to a survey of compact AGN at 5 GHz which are stronger
than 1 Jy -- the VSOP AGN Survey. This paper, the second in a series, describes
the data calibration, source detection, self-calibration, imaging and modeling,
and gives examples illustrating the problems specific to space VLBI. The VSOP
Survey web-site which contains all results and calibrated data is described.
