Crynodeb
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.
| Iaith wreiddiol | Saesneg |
|---|---|
| Teitl | Magnetic fields and solar processes |
| Is-deitl | The 9th European Meeting on Solar Physics : 12-18 September 1999, Florence, Italy (SP) |
| Cyhoeddwr | European Space Agency |
| Tudalennau | 81-86 |
| Nifer y tudalennau | 6 |
| Cyfrol | 448 |
| ISBN (Argraffiad) | 9789290927921, 9290927925 |
| Statws | Cyhoeddwyd - Rhag 1999 |
| Cyhoeddwyd yn allanol | Ie |
| Digwyddiad | The 9th European Meeting on Solar Physics - Florence, Yr Eidal Hyd: 12 Medi 1999 → 18 Medi 1999 |
Cynhadledd
| Cynhadledd | The 9th European Meeting on Solar Physics |
|---|---|
| Teitl cryno | ESPM-9 |
| Gwlad/Tiriogaeth | Yr Eidal |
| Dinas | Florence |
| Cyfnod | 12 Medi 1999 → 18 Medi 1999 |
Ôl bys
Gweld gwybodaeth am bynciau ymchwil 'The Influence of a Steady State on p-and f-Modes'. Gyda’i gilydd, maen nhw’n ffurfio ôl bys unigryw.Dyfynnu hyn
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