Aspect angle dependence of backscatter intensity of 1-m auroral plasma waves

Details Aspect angle dependence of backscatter intensity of 1-m auroral plasma waves Aspect angle dependence of backscatter intensity of 1-m auroral plasma waves

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jgr....93.4119n&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 93, May 1, 1988, p. 4119-4124.

Physics

9

Atmospheric Scattering, Auroral Zones, Backscattering, E Region, Plasma Waves, Electric Fields, Ionospheric Disturbances, Radar Data

Scientific paper

The backscatter intensities of primary and secondary 1-m unstable plasma waves in the auroral E region were measured as functions of the magnetic aspect angle for electric field values between 25 and 30 mV/m, using observations made by the Scandinavian Twin Auroral Radar Experiment system. In this study, the flow angle measurements were available, making it possible to determine separately for the primary and the secondary waves the attenuation of the backscattered signal. The results suggest a difference in the backscatter altitude of primary and secondary waves, with primary waves dominating at the higher altitudes.

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