The structure of atmospheric turbulence and its relationship to the re
fractive index discontinuities responsible for the scattering of radio
waves are discussed. Emphasis is placed more on the nature of the int
ermittent scatterers observed at upper mesospheric/lower thermospheric
altitudes than on volume scattering. The preferred model is of transi
ent patches composed of vortex strings. An overview of the methods use
d to estimate the rate of dissipation of turbulent energy using MF rad
ar data which emphasizes the advantages of imaging Doppler interferome
try is presented, together with a review of pertinent laboratory inves
tigations of coherent structures. An attempt is made to remove the con
tamination by gravity waves from imaging Doppler interferometry fluctu
ating velocity data. Emphasis is given to the fact that all radar meas
urements of turbulent intensity to date are upper estimates, not only
because of the presence of gravity wave fluctuations contaminating the
data, but also because the turbulence itself is not stationary and ho
mogeneous but intermittent in both space and time. The intermittent na
ture of the turbulence, in which the refractive index discontinuities
responsible for the radar backscatter are associated with decaying, ho
mogeneous turbulent coherent structures, is in contrast to the theory
of volume scattering, which assumes the radar pulse volume to be parti
ally filled with stationary, homogeneous turbulence.