The background of VLF wave-particle experiments from Siple Station, Antarctica, including wave-induced precipitation is briefly reviewed. Single frequency ducted signals that exceed a certain \u27threshold\u27 intensity are observed at the conjugate point (Roberval, Quebec) to be amplified 30-50dB, with temporal growth rates of 30-200dB/s. Following saturation, variable frequency emissions are triggered. When a second signal is added to the first, with a frequency spacing Df<100Hz, signal growth is reduced and sidebands are generated at frequencies separated from the carriers by integer multiples (up to seven) of Df. The sidebands are attributed to short emissions triggered by the beats between the two input carriers. Mid-latitude magnetosp...
International audienceThe results of detailed spectral analyses and direction finding for both VLF a...
A magnetospheric substorm is manifested in a variety of phenomena observed both in space and on the ...
The burst precipitation of energetic electrons (≥40 keV), induced by interactions with lightning‐gen...
The phenomenon of artificially triggered VLF emissions was first reported in 1964. Caused by a plasm...
Spectrograms of broad-band ELF/VLF goniometer data obtained from ground based measurements made at H...
Spectrograms of broad-band ELF/VLF goniometer data obtained from ground based measurements made at H...
Highlights of recent Stanford University VLF research in the Antarctic include new observations of w...
Controlled experiments with dedicated ground-based ELF/VLF (0.3-30 kHz) transmitters are invaluable ...
VLF wave-wave interaction experiments were carried out by injecting various forms of VLF pulses into...
Magnetospheric whistler mode waves in the magnetosphere, both natural and man-made (such as those tr...
Recent topics of VLF observations at Syowa Station, Antarctica, are summarized. In the frequency-tim...
24-30The morphological features of VLF hiss observed at the auroral and low latitude stations are ...
Power Line Harmonic Radiation and associated emissions observed at Siple [1, 2] are compared with li...
This work is concerned with the numerical modelling of VLF emissions triggered in the equatorial re...
Observations of VLF hiss narrow-band intensities (5.0±0.2 kHz, 12.0±0.5 kHz, and 50.0±1.0 kHz), hori...
International audienceThe results of detailed spectral analyses and direction finding for both VLF a...
A magnetospheric substorm is manifested in a variety of phenomena observed both in space and on the ...
The burst precipitation of energetic electrons (≥40 keV), induced by interactions with lightning‐gen...
The phenomenon of artificially triggered VLF emissions was first reported in 1964. Caused by a plasm...
Spectrograms of broad-band ELF/VLF goniometer data obtained from ground based measurements made at H...
Spectrograms of broad-band ELF/VLF goniometer data obtained from ground based measurements made at H...
Highlights of recent Stanford University VLF research in the Antarctic include new observations of w...
Controlled experiments with dedicated ground-based ELF/VLF (0.3-30 kHz) transmitters are invaluable ...
VLF wave-wave interaction experiments were carried out by injecting various forms of VLF pulses into...
Magnetospheric whistler mode waves in the magnetosphere, both natural and man-made (such as those tr...
Recent topics of VLF observations at Syowa Station, Antarctica, are summarized. In the frequency-tim...
24-30The morphological features of VLF hiss observed at the auroral and low latitude stations are ...
Power Line Harmonic Radiation and associated emissions observed at Siple [1, 2] are compared with li...
This work is concerned with the numerical modelling of VLF emissions triggered in the equatorial re...
Observations of VLF hiss narrow-band intensities (5.0±0.2 kHz, 12.0±0.5 kHz, and 50.0±1.0 kHz), hori...
International audienceThe results of detailed spectral analyses and direction finding for both VLF a...
A magnetospheric substorm is manifested in a variety of phenomena observed both in space and on the ...
The burst precipitation of energetic electrons (≥40 keV), induced by interactions with lightning‐gen...