Colliding plasmas can excite strong Langmuir turbulence in which colle
ctive correlations affect the probability distribution P(E) of the ele
ctric microfield. This can be modeled by including long-range correlat
ions but not dynamics over lengths much greater than lambda(D). Earlie
r work yielded a characteristic distribution P(E) is-proportional-to E
(d-1) exp(-E2/<E2>), with d the dimensionality of the electric field a
nd [E2] proportional to the square of the correlated particle density.
Ions scatter from this localized strong turbulence at rates greatly e
xceeding classical collisions for solar coronal conditions, while labo
ratory ion beams have no appreciable scatter beyond the Coulomb rate.