Solar atmospheric dynamics

Physics

Scientific paper

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Atmospheric Physics, Chromosphere, Solar Atmosphere, Solar Corona, Gravity Waves, Magnetohydrodynamic Waves, Solar Physics, Vector Analysis

Scientific paper

This study, aimed at calculating the heating of the solar chromosphere and corona, started with the analysis of magneto-acoustic-gravity wave vector surfaces. To permit non-linear calculation of the excitation and propagation of these waves the equations of motion were written for an imposed horizontal structure -- namely six waves of the same wavelength propagating in an hexagonal pattern.

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