Nonlinear coupling of O- and X-mode radio emission and Alfven waves in the solar corona

Details Nonlinear coupling of O- and X-mode radio emission and Alfven waves in the solar corona Nonlinear coupling of O- and X-mode radio emission and Alfven waves in the solar corona

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..537..287s&link_type=abstract

WAVES IN DUSTY, SOLAR, AND SPACE PLASMAS. AIP Conference Proceedings, Volume 537, pp. 287-294 (2000).

Physics

1

Magnetohydrodynamic Waves, Magnetohydrodynamics And Plasmas, Magnetohydrodynamic And Fluid Equation

Scientific paper

The nonlinear coupling of extraordinary and ordinary waves via kinetic Alfven waves (KAWs) is investigated on the basis of two fluid magnetohydrodynamics. The equation governing the time dependence of electric field of excited O-mode is found. We estimate the time of effective coupling between modes and corresponding interaction distance in solar corona. Our theoretical results show that the X- and O-mode couplings via Alfven waves can be efficient depolarization mechanism for the coronal radioemission. .

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