Solar atmospheric dynamics

Computer Science – Sound

Scientific paper

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Chromosphere, Solar Atmosphere, Solar Physics, Computerized Simulation, Finite Difference Theory, Gravity Waves, Heating, Mathematical Models, Radiative Transfer, Shock Waves, Sound Waves

Scientific paper

We have studied the heating of the solar chromosphere and transition region by acoustic waves. We find they are incapable of transporting sufficient energy through the chromosphere to heat the transition region and corona. We are developing a radiative fluid dynamic computer code to study acoustic heating of the chromosphere and the effect of acoustic waves on line profiles. In order to study heating by other types of wave motions we have analyzed the wave vector surface of the Magneto-Acoustic-Gravity Waves and are developing a 'modal' computer code to study their propagation and dissipation.

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