Excitation of Solar Acoustic Oscillations
| dc.creator | Kumar, Pawan | |
| dc.date | 1996-12-11 | |
| dc.date.accessioned | 2026-07-07T02:22:33Z | |
| dc.date.available | 2026-07-07T02:22:33Z | |
| dc.description | The stochastic excitation of solar oscillations due to turbulent convection is reviewed. A number of different observational results that provide test for solar p-mode excitation theories are described. I discuss how well the stochastic excitation theory does in explaining these observations. The location and properties of sources that excite solar p-modes are also described. Finally, I discuss why solar g-modes should be linearly stable, and estimate the surface velocity amplitudes of low degree g-modes assuming that they are stochastically excited by the turbulent convection in the sun. | |
| dc.description | 19 pages, LaTeX, 7 figues. Invited review to appear in the IAU symposium # 181 "Sounding Solar and Stellar Interiors", eds. F.X. Schmider & J. Provost | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9612120 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9612120 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10915 | |
| dc.subject | Astrophysics | |
| dc.title | Excitation of Solar Acoustic Oscillations | |
| dc.type | text |