Abstract
Generalised ray theory provides a simple description of MHD mode transmission and conversion between magnetoacoustic fast and slow waves and is directly applicable to solar active regions. Here it is tested in a simple two-dimensional, isothermal, gravitationally stratified model with inclined magnetic field using previously published exact solutions and found to perform very well.
Original language | English |
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Pages (from-to) | 193 - 202 |
Number of pages | 10 |
Journal | Solar Physics |
Volume | 255 |
Issue number | 2 |
Publication status | Published - 2009 |