Ordinary mode auroral kilometric radiation fine structure observed by DE 1

Details Ordinary mode auroral kilometric radiation fine structure observed by DE 1 Ordinary mode auroral kilometric radiation fine structure observed by DE 1

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jgr....93.7515b&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 93, July 1, 1988, p. 7515-7520.

Physics

11

Auroras, Dynamics Explorer 1 Satellite, Kilometric Waves, Auroral Arcs, Cyclotron Radiation, Fine Structure, Spectrum Analysis

Scientific paper

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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