In this paper we examine the dynamic response of a magnetoplasma to an
external time-dependent current source in the context of electronmagn
etohydrodynamics (EMHD). A combined analytic and numerical technique i
s developed to address this problem. The set of cold electron plasma a
nd Maxwell's equations are first solved analytically in the (k,omega)
space. Inverse Laplace and three-dimensional complex Fast Fourier Tran
sform techniques are used subsequently to numerically transform the ra
diation fields and plasma currents from the (k,omega) space to the (r,
t) space. The results show that the electron plasma responds to a time
-varying current source imposed across the magnetic field by exciting
whistler/helicon waves and forming an expanding local current loop, dr
iven by field-aligned plasma currents. The current loop consists of tw
o antiparallel field-aligned current channels concentrated at the ends
of the imposed current and a cross-field Hall current region connecti
ng these channels. The characteristics of the current closure region a
re determined by the background plasma density, the magnetic field, an
d the time scale of the current source. The results are applied to the
ionospheric generation of extremely low-frequency (ELF) and very low-
frequency (VLF) radiation using amplitude modulated high-frequency hea
ting. It is found that contrary to previous suggestions the dominant r
adiating moment of the ELF/VLF ionospheric source is an equivalent hor
izontal magnetic dipole. (C) 1996 American Institute of Physics.