Abstract
The combined effect of a subsurface steady homogeneous flow and a chromospheric uniform magnetic field on the solar p- and f-modes is evaluated theoretically for a simple model of the Sun. The derived dispersion relation is solved analytically in limit of the long wavelength approximation and is evaluated numerically for arbitrary wavelengths. The influence of an equilibrium flow is more dominant in limit of small wavenumbers. For arbitrary wavelengths the effect of a magnetic field might be stronger than frequency shifts caused by a steady homogeneous flow.
| Original language | English |
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| Title of host publication | Symposium - International Astronomical Union |
| Subtitle of host publication | Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions |
| Publisher | Cambridge University Press |
| Pages | 208-210 |
| Number of pages | 3 |
| Volume | 203 |
| DOIs | |
| Publication status | Published - 2001 |
| Externally published | Yes |