Asymptotic WKBJ-studies of solar dynamo waves: 1D and 2D cases (Q2776165)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Asymptotic WKBJ-studies of solar dynamo waves: 1D and 2D cases |
scientific article; zbMATH DE number 1714379
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Asymptotic WKBJ-studies of solar dynamo waves: 1D and 2D cases |
scientific article; zbMATH DE number 1714379 |
Statements
30 March 2003
0 references
short waves
0 references
alpha-omega-effect dynamo model
0 references
WKBJ method
0 references
differentially rotating spherical shell
0 references
Asymptotic WKBJ-studies of solar dynamo waves: 1D and 2D cases (English)
0 references
The WKBJ method is used to study short waves in thin layers which arise in an alpha-omega-effect dynamo model, in a differentially rotating spherical shell. The author obtains two non-overlapping independent dynamo waves. The first wave propagates equatorwards over low latitudes, while the second wave propagates polewards over high latitudes.NEWLINENEWLINEFor the entire collection see [Zbl 0973.00055].
0 references
