The interaction of a radially bounded electron beam spiraling in a magnetop
lasma with a quasi-monochromatic whistler at the Cherenkov and Doppler-shif
ted resonance conditions is investigated. For the linear stage of the inter
action, the instability growth rate as well as the radial flux of wave ener
gy emitted by the thin spiral beam are calculated. Compared to previous wor
ks considering a cylindrical beam or electrostatic lower hybrid waves, the
present study gives the possibility to extend the investigation of the whis
tler-beam interaction to wider ranges of physical parameters, and, in parti
cular, to situations where the beam is injected obliquely with respect to t
he ambient magnetic field. The main physical process occurring during the d
issipative beam-wave interaction-that is, which takes into account the ener
gy leakage out of the bounded beam volume-is the nonlinear self-organizatio
n of part of the beam electrons which leads to the formation of dynamically
stable bunches that are continuously decelerated or accelerated while keep
ing resonance with the emitted wave. In a long time evolution, bunches are
the main cause which supports the wave emission whereas the nonresonant bea
m electrons practically do not exchange energy with the wave. It is shown t
hat the efficiency of the electromagnetic wave emission by a thin spiral be
am is less at the cyclotron resonances than at the Cherenkov resonance. (C)
2001 American Institute of Physics.