We present 15 images from the global mm-VLBI sessions in 1990 April at
100 GHz and 1993 April at 86 GHz. These observations probe the centra
l engines of the 16 observed AGN's with up to 50 mu as resolution. Amo
ng other sources previously observed with lambda 3 mm VLBI we present
the first lambda 3 mm maps of 0735+178, 0748+126, 1055+018, 2145+067,
and CTA102, in total we have been able to image 13 out of the 16 obser
ved sources. 6 out of the 13 imaged sources observed exhibit curvature
and rapid structural changes, although the low dynamic range in two t
hirds of the maps limits the detection of weak features. Most of the s
ources have unresolved cores even at this high resolution. There is su
bstantial evidence that the observed sources can be grouped into two g
eneral groups: A misaligned population with parsec scale jets in the f
orm of low pitch helices and an aligned population with straight jets
with small changes in PA due to intrinsic bends.