  We continue our study (Grechnev et al. (2013), doi:10.1007/s11207-013-0316-6;
Paper I) on the 18 November 2003 geoffective event. To understand possible
impact on geospace of coronal transients observed on that day, we investigated
their properties from solar near-surface manifestations in extreme ultraviolet,
LASCO white-light images, and dynamic radio spectra. We reconcile near-surface
activity with the expansion of coronal mass ejections (CMEs) and determine
their orientation relative to the earthward direction. The kinematic
measurements, dynamic radio spectra, and microwave and X-ray light curves all
contribute to the overall picture of the complex event and confirm an
additional eruption at 08:07 - 08:20 UT close to the solar disk center presumed
in Paper I. Unusual characteristics of the ejection appear to match those
expected for a source of the 20 November superstorm but make its detection in
LASCO images hopeless. On the other hand, none of the CMEs observed by LASCO
seem to be a promising candidate for a source of the superstorm being able to
produce, at most, a glancing blow on the Earth's magnetosphere. Our analysis
confirms free propagation of shock waves revealed in the event and reconciles
their kinematics with "EUV waves" and dynamic radio spectra up to decameters.
