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July 1, 1988Journal of Geophysical Research Atmospheres

Ordinary mode auroral kilometric radiation fine structure observed by DE 1

R. F. Benson M. M. Mellott Richard Huff D. A. Gurnett

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Abstract

The fine structure observed with intense right‐hand extraordinary ( R‐X ) mode auroral kilometric radiation (AKR) has received major theoretical attention. Data from the Dynamics Explorer 1 plasma wave instrument indicate that left‐hand ordinary ( L‐O ) mode AKR possesses similar fine structure. Several theories have been proposed to explain the fine structure of the R‐X mode AKR. In order to account for the L‐O mode fine structure, these theories will have to be modified to produce the L‐O mode directly or will have to rely on mode conversion processes from the R‐X to the L‐O mode.

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Cite This Study

Benson et al. (1988) studied this question.

synapsesocial.com/papers/6a6f8d4ac2d7c3090826c8a9 https://doi.org/10.1029/ja093ia07p07515

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