Physics
Scientific paper
Jan 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...69...27r&link_type=abstract
Solar Physics, vol. 69, Jan. 1981, p. 27-38.
Physics
185
Magnetoacoustic Waves, Magnetohydrodynamic Waves, Solar Atmosphere, Solar Magnetic Field, Surface Waves, Wave Propagation, Fourier Analysis, Inhomogeneity, Photosphere, Pressure Effects, Propagation Velocity, Solar Corona, Thermodynamic Equilibrium
Scientific paper
The inhomogeneity that is introduced by a magnetic field in the solar atmosphere in a direction orthogonal to the field is examined. For a single magnetic interface with one field-free side, a slow surface wave can always propagate. A fast surface wave may propagate if the field-free medium is warmer than the magnetic atmosphere. For an isolated magnetic slab, the field can support the propagation of both body and surface waves. The existence and nature of these waves depends on the relative magnitudes of the sound speed and Alfven speed inside the slab and the sound speed in the field-free environment. The slow mode can always propagate, and does so both as a surface wave and as a body wave. The fast mode may propagate only in slabs that are not hotter than their surroundings (the sound speed in the field free environment greater or equal to the sound speed inside the slab), and then it is a body wave or a surface wave accordingly as the sound speed in the field-free environment is greater or less than the Alfven speed inside the slab. The special case of a slender field is also investigated, and it is demonstrated how the slender flux tube approximation relates to the more general results. The generation of resonant modes in a slender slab is briefly addressed.
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