Open AccessAn interpretation of banded magnetospheric radio emissions
Author(s) -
Benson R. F.,
Osherovich V. A.,
Fainberg J.,
F.Vinas A.,
Ruppert D. R.
Publication year - 2001
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2000ja000162
Subject(s) - magnetosphere , ionosphere , physics , plasma , spectral line , atomic physics , electron , ion , electron precipitation , computational physics , atmospheric sciences , geophysics , nuclear physics , astronomy , quantum mechanics
Recently published Active Magnetospheric Particle Tracer Explorers/Ion Release Module (AMPTE/IRM) banded magnetospheric emissions, commonly referred to as “( n + 1/2) f ce ” emissions, where f ce is the electron gyrofrequency, are analyzed by treating them as analogous to sounder‐stimulated ionospheric emissions. We show that both individual spectra of magnetospheric banded emissions and a statistically derived spectra observed over the 2‐year lifetime of the mission can be interpreted in a self‐consistent manner. The analysis, which predicts all spectral peaks within 4% of the observed peaks, interprets the higher‐frequency emissions as due to low group velocity Bernstein‐mode waves and interprets the lower‐frequency emissions as eigenmodes of cylindrical‐electromagnetic plasma oscillations. The demarcation between these two classes of emissions is the electron plasma frequency f pe where an emission is often observed. This f pe emission is not necessarily the strongest. None of the observed banded emissions were attributed to the upper hybrid frequency. We present Alouette 2 and ISIS 1 plasma resonance data and model electron temperature ( T e ) values to support the argument that the frequency spectrum of ionospheric sounder‐stimulated emissions is not strongly temperature dependent and thus that the interpretation of these emissions in the ionosphere is relevant to other plasmas (such as the magnetosphere) where N e and T e can be quite different but where the ratio f pe / f ce is identical. The N e values deduced from the spectral interpretation do not agree with the values determined from the AMPTE/IRM three‐dimensional plasma instrument. The latter, which represent a lower bound, are found to be higher than the former by a factor of 3.2 – 3.5. All values were less than 1 cm −3 , a domain known for measurement difficulties. One possible explanation is that the wave and plasma techniques respond to different components of a non‐Maxwellian magnetospheric electron distribution.