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 |
|---|---|
| Pages (from-to) | 193 - 202 |
| Number of pages | 10 |
| Journal | Solar Physics |
| Volume | 255 |
| Issue number | 2 |
| Publication status | Published - 2009 |