The table gives the properties of the magnetic field in the
solar source region and at 1 AU for 27 events whose solar
sources have been unanimously identified by different
researchers. The different pieces of information concerning
solar source identification were put together by Jie about
10 days before the meeting. Since then the number of events
with unanimously identified solar sources has increased but
due to time limitations I considered only the first 27 of
them. The remaining events will be studied after the meeting.

The first column gives the number of the event.

The second column gives the chirality (i.e. handedness) of the
magnetic field in the source region. Data from various instruments
have been used (SXT, EIT, Ha).

The third column shows the polarity of the leading field in the
low corona predicted by the Coronal Flux Rope model (North or
South).

The fourth column gives the structure of the magnetic cloud's
magnetic field. In each entry, the first, middle and last letter
corresponds to the leading, center, and trailing polarity of
the MC's  field (in GSE coordinates). 

The fifth column presents the chirality of the MC's field.

No entry appears in columns 4 and 5 when the event was not 
associated with a MC at 1 AU.

The sixth column gives the orientation of the Sun's large-scale
bipolar magnetic field (North or South). Between March 2000
and October 2001, the behavior of the Sun's polar field had
not been settled and several reversals occurred (either in 
the north pole or south pole).