The frequency maxima of electron cyclotron harmonic (ECH) waves provide str
ong responses to sounding in various plasma regimes in the solar system. Th
e frequency maxima correspond to waves for which the group velocity and thu
s the energy propagation velocity in the plasma frame of reference is zero.
A particle-in-cell (PIC) code is employed to show that the propagation of
wave energy at a non-zero velocity, necessary to couple energy from a stati
onary antenna to the plasma, is accomplished by propagating wave precursors
. The undamped waves at the frequency maxima of the ECH branches are nonpro
pagating hence the waves remain localized. It is demonstrated that the nonp
ropagating waves, built up by the wave precursors, are standing waves. The
standing wave generation is followed from the linear to nonlinear regimes.
For nonlinear emission amplitudes the emission causes a plasma density depl
etion close to the antenna. The depletion is shown to trigger a modulationa
l instability in which the ECH wave collapses. The generated nonlinear stan
ding wave also develops an electromagnetic component which couples the elec
trostatic ECH waves to the fast extraordinary wave. (C) 1999 American Insti
tute of Physics. [S1070-664X(99)00707-7].