We present the results of simultaneous VLBI observations of the quasar
3C395 at 2.3 and 8.4 GHz. Our maps show two well defined components (
A and B) together with a weaker component in between (C2). The positio
n of component C2 is compatible with the position of a component obser
ved at epoch 1986.9 (component Cl). We can interpret this positional c
oincidence i) assuming that component C2 and component C1 are just the
same one, and hence C2 is stationary, or ii) considering that compone
nt C2 has travelled from the core to its current position, which now i
s coincident with the position of component C1 observed in 1986.9. The
latter interpretation is supported by the total flux density evolutio
n of 3C395. Based on this idea, we also present a model for 3C395 and
numerical simulations of the time evolution of the emission of the com
pact structure at 2.3, 4.9 and 8.4 GHz which allow us to construct sim
ulated maps of 3C395. The model and numerical simulations also provide
a quantitative positional shift for the opaque core at 2.3 GHz with r
espect to 8.4 GHz which helps us to construct a spectral-index map of
the source. Finally, our re-analysis of intermediate resolution VLBI o
bservations at 0.6 GHz contribute to clarify the behavior of the jet b
eyond the cm-VLBI structure.