The Astrophysical Journal · 1989 · 26 citations · 0 references
Natural SciencesAstronomyPhysicsAcousticsAstrophysicsSolar AstronomyAnisotropic MediaElectromagnetic WavesMagnetohydrodynamicsSolar Magnetic FieldsSolar OscillationsSolar RadiationCompressive LoadsMode DampingPhotospheric Magnetic FieldsPhotospheric MagnetismRadiative Transfer ModelingSolar Acoustic OscillationsSolar MagnetohydrodynamicsSolar Oscillation Frequencies
Using the Mihalas and Mihalas (1983) treatment of the radiation field, the dispersion relation for linear compressive plane waves in a homogeneous, unstratified, uniformly magnetized, radiating fluid has been obtained. In the opticallly thick limit, the present relation is shown to predict two weakly damped anisotropic radiation-modified magnetoacoustic modes and a strongly damped radiation-diffusion mode. The theory has been applied to the example of the interaction of the solar acoustic oscillations with discrete photospheric magnetic structures such as sunspots, pores, and knots.