We obtained an H-2 1-0 S(1) image of the south-east ridge in the super
nova remnant IC 443 by using a Fabry-Perot imager. The H-2 emitting re
gion was resolved into many clumps which had not been seen by previous
observations with larger beams. The H-2 image was compared with a 21-
cm H I map in order to investigate the H-2 excitation mechanism. Altho
ugh the H-2 emitting area roughly overlaps the H I area, no one-to-one
correlation between the peaks of H-2 and H I is found. This morpholog
y indicates that although the H I 21-cm line is due to molecular disso
ciation by J-shocks, the H-2 emission peaks are caused by C-shocks in
dense clumps. Consequently, the coexistence of C-shocks and J-shocks i
s suggested to be present at the molecular ridge of IC 443.