Ion cyclotron whistlers.
Proton whistler /VLF phenomenon observed in satellite data/ discussing propagation in multicomponent plasma and ion cyclotron mode
ION CYCLOTRON↗
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Electron density in the whistler medium.
Electron density in exospheric whistler medium, using satellite data
ELECTRON DENSITY↗
Correlations among very low frequency emissions, whistlers, and magnetic activities.
Correlation of VLF emission, whistlers and magnetic activity
RADIO EMISSION↗
A dispersion anomaly in whistlers received on alouette 1.
Alouette I whistler observations at 1000 km show dispersion anomaly that increases with increasing frequency
WHISTLER RECORDER↗
Partial electron velocity spectrums from cyclotron absorption of whistler power.
Partial electron velocity spectra determined from power spectra of whistler signal at upper cut-off due to cyclotron absorption
CYCLOTRON RESONANCE↗
Determination of hydrogen ion concentration, electron density and proton gyrofrequency from the dispersion of proton whistlers
Hydrogen ion concentration, electron density, and proton gyrofrequency near satellites from asymptotic frequency-time profile of proton whistler near proton gyrofrequency
PROTON↗
Unstable growth of unducted whistlers propagating at an angle to the geomagnetic field
Unstable growth rate of unducted whistler waves propagating at angle to geomagnetic field
GROWTH↗
An interpretation of transverse whistlers.
Whistler in Alouette I satellite VLF RECORDINGS, variation of time delay with frequency given by Eckersley law time delay and additive correction term
WHISTLER↗
Exact nonlinear electromagnetic whistler modes.
Exact solution of nonlinear relativistic equations of motion for electron in right circularly polarized wave propagating in whistler mode parallel to external magnetic field
WHISTLER↗
Unstable growth of unducted whistlers propagating at an angle to the geomagnetic field.
Growth rate along whistler path for waves propagating at angle to geomagnetic field
WHISTLER↗
Radiation Belt Electron Dynamics Driven by Large-Amplitude Whistlers
Acceleration of radiation belt electrons driven by oblique large-amplitude whistler waves is studied. We show analytically and numerically that this is a stochastic process; the intensity of which depends on the wave power modified by Bessel functions. The type of this dependence is determined by the character of the nonlinear interaction due to coupling between action and phase. The results show that physically significant quantities have a relatively weak dependence on the wave power.
whistlers↗
Magnetospheric properties deduced from OGO 1 observations of ducted and nonducted whistlers.
Magnetospheric ionization distribution determined by ducted and nonducted whistler propagation modes and reflection as observed by OGO 1
Angerami, J. J.↗
Ion cyclotron whistlers in the solar wind.
Ion cyclotron whistlers in solar wind, noting LF electromagnetic modes wave characteristics and growth and damping rates, alpha particles effect and mode coupling
Fredricks, R. W.↗
Possible relationship between the storm-time whistler cutoff and the magnetospheric ring current.
Storm time whistler cut-off related to magnetospheric ring current during magnetic storm, noting formation of high energy high density plasma
Bauer, S. J.↗
Alouette 1 and 2 observations of abrupt changes in whistler rate and of VLF noise variations at the plasmapause - A satellite-ground study.
Satellite observations of abrupt changes in whistler rate and VLF noise variations at plasmapause
Barrington, R. E.↗
Effect of longitudinal electrostatic field on the whistler mode propagation in a warm magneto-ionic medium.
Dispersion equation for whistler mode propagation in warm plasma in parallel static fields, using Vlasov-Maxwell equation
Hsieh, H. C.↗
Whistler mode propagation in the ionosphere in the presence of a longitudinal static electric field.
Whistler mode propagation in presence of longitudinal static electric field in region of ionosphere where particle collisions influence ion motion
Hsieh, H. C.↗
Unducted whistler evidence for a secondary peak in the electron energy spectrum near 10 kev.
Ambient electron energy spectrum secondary peak determined from unducted magnetospherically reflected whistler mode radiation measurements
Thorne, R. M.↗