Stochastic description of inflationary spacetimes emulates the growth of va
cuum fluctuations by an effective stochastic ''noise field" which drives th
e dynamics of the volume-smoothed inflation. We investigate statistical pro
perties of this field and find its correlator to be a function of distance
measured in units of the smoothing length. Our results apply for a wide cla
ss of smoothing window functions and are different from previous calculatio
ns by Starobinsky and others who used a sharp momentum cutoff. We also disc
uss the applicability of some approximate noise descriptions to simulations
of stochastic inflation.