An Exact Test of Generalized Ray Theory in Local Helioseismology
| dc.creator | Hansen, Shelley C. | |
| dc.creator | Cally, Paul S. | |
| dc.date | 2009-02-10 | |
| dc.date.accessioned | 2026-07-07T12:39:49Z | |
| dc.date.available | 2026-07-07T12:39:49Z | |
| dc.description | Generalized Ray Theory (GRT) 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. | |
| dc.description | 11 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/0902.1581 | |
| dc.identifier | http://arxiv.org/abs/0902.1581 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/219248 | |
| dc.subject | Solar and Stellar Astrophysics | |
| dc.title | An Exact Test of Generalized Ray Theory in Local Helioseismology | |
| dc.type | text |