Nandy, Dibyendu ; Rai Choudhuri, Arnab (2000) The role of magnetic buoyancy in a Babcock-Leighton type solar dynamo Journal of Astrophysics and Astronomy, 21 (3-4). pp. 381-385. ISSN 0250-6335
|
PDF
- Publisher Version
87kB |
Official URL: http://www.ias.ac.in/jarch/jaa/21/381-385.pdf
Related URL: http://dx.doi.org/10.1007/BF02702429
Abstract
We study the effects of incorporating magnetic buoyancy in a model of the solar dynamo-which draws inspiration from the Babcock-Leighton idea of surface processes generating the poloidal field. We present our main results here.
Item Type: | Article |
---|---|
Source: | Copyright of this article belongs to Indian Academy of Sciences. |
Keywords: | MHD-Sun: Interior; Magnetic Fields |
ID Code: | 66541 |
Deposited On: | 24 Oct 2011 07:26 |
Last Modified: | 18 May 2016 14:02 |
Repository Staff Only: item control page