We present results of two-epoch intercontinental VLBI observations at
6 cm wavelength of LSI +61 degrees 303 during an outburst in 1993. In
the first epoch, the total flux density of LSI +61 degrees 303 varied
from 76 to 131 mJy and the derived size of the emitting region was abo
ut 3 mas. In the second epoch, four days later, the flux density of LS
I +61 degrees 303 was very stable, at a level of 60 mJy. The flux sta
bility along all the second session allowed us to carry out standard h
ybrid mapping. The VLBI map obtained exhibits an extended structure of
about 7 mas with an unresolved component at the center of the extende
d structure. The results derived from both observing sessions seem to
agree with a source expanding with time from 2-3 to 7 mas, at a veloci
ty of similar to 2200 km s(-1). In addition, our results suggest the e
xistence of a quiescent component associated with the core.