A Langevin equation for charged particles in a plasma with electrostat
ic turbulence is developed from first principles and in consistency wi
th the kinetic theory in polarization approximation. For the case of i
on-acoustic and electrostatic lower-hybrid-drift turbulence approximat
e expressions for the space-time spectral density of the wave energy a
re given and estimates of the intensities of the stochastic wave force
s are made. The application is done for the plasmas of the earth's mag
netosphere, the solar wind and solar hares. It seems, that ion-acousti
c and electrostatic lower-hybrid-drift waves can contribute to electro
n chaotization in different regions of the space plasma.