A two-dimensional full Fokker-Planck (FP) simulation code coupled with an i
deal fluid equation has been constructed. This code was applied for the num
erical simulation of the Rayleigh-Taylor (RT) instability on the directly d
riven ablation front. The simulation results show that an accelerated thin
foil is preheated by the non-local electron heat transport, the ablation fr
ont density is depleted, and the linear growth rate of the RT instability i
s suppressed strongly. By investigating the mode structure in the simulatio
n, it is found that the peak of the eigen mode shifts toward the corona reg
ion by the non-local heat conduction effects. This is the reason why the gr
owth rate is reduced. (C) 1999 Elsevier Science S.A. All rights reserved.