Abstract
The influence of a steady equilibrium state on p- and f- modes is evaluated theoretically for a simple model of the solar plasma, consisting of a polytrope and steady solar interior, above which is an isothermal magnetic atmosphere. Frequency changes and Doppler shifts in phase factors, due to the presence of a steady interior, are calculated analytically in the long-wavelength approximation using hypergeometric functions. The obtained dispersion relation is solved numerically for other cases.
Original language | English |
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Title of host publication | Magnetic fields and solar processes |
Subtitle of host publication | The 9th European Meeting on Solar Physics : 12-18 September 1999, Florence, Italy (SP) |
Publisher | European Space Agency |
Pages | 81-86 |
Number of pages | 6 |
Volume | 448 |
ISBN (Print) | 9789290927921, 9290927925 |
Publication status | Published - Dec 1999 |
Externally published | Yes |
Event | The 9th European Meeting on Solar Physics - Florence, Italy Duration: 12 Sept 1999 → 18 Sept 1999 |
Conference
Conference | The 9th European Meeting on Solar Physics |
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Abbreviated title | ESPM-9 |
Country/Territory | Italy |
City | Florence |
Period | 12 Sept 1999 → 18 Sept 1999 |
Keywords
- Helioseismology
- p- and f- Modes
- Steady Flow