B. Lundin et al., VLF EMISSION PRODUCED BY A RAREFIED ELECTRON-BEAM DURING ACTIVE EXPERIMENTS IN THE EARTH-IONOSPHERE - CONDITIONS OF OBSERVATION OF THE EMISSION, J GEO R-S P, 99(A8), 1994, pp. 14987-15003
The peculiarities of whistler waves spontaneously radiated by an elect
ron beam artificially injected into the Earth ionosphere are discussed
. The conditions of registration of the whistler wave packets by a rem
ote on board VLF receiver have been analyzed- they depend on mutual di
sposition of the electron gun and the VLF receiver as well as on the p
itch angle of the injected electrons. It is shown that the internal fr
equency width of the whistler signal, connected with ray representatio
n of a wave field, depends oxi the distance between the emitting regio
n of the beam and the receiver and determines the lowest bandwidth of
the VLF receiver in use. In the case of a dense plasma (when the plasm
a frequency omega(p) is much greater than the electron gyrofrequency o
mega(c)) the main results are obtained analytically. The effective val
ue of the electron collision frequency for the background plasma can b
e estimated through measurements of the maximum value of the injection
pitch angle of the beam's electrons, which leads to a steep drop in t
he level of the whistler signal. It is shown that double-pole. singula
rity in the single electron Cherenkov energy loss near the Gendrin's v
elocity appears only at a single frequency depending on the beam and t
he background plasma parameters. Thus the total growth of the energy l
oss in this case reveals an increase by a factor of the order of omega
(p)/omega(c) compared to the usual single-pole contribution. The Chere
nkov radiation from the sharp leading front of the beam does not revea
l any Mach cone structure. The peculiarities of the spectral parameter
s of the whistler emission at the Doppler-shifted resonances are also
discussed; the Mach cone exists in these cases. Thus this feature can
be responsible for the crucial difference between the registration pat
tern of high-frequency and whistler frequency emission in active exper
iments similar to ARAKS.