Comments on "Full-sphere simulations of circulation-dominated solar dynamo: Exploring the parity issue" - Reply
Data(s) |
01/07/2005
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Resumo |
We respond to Dikpati et al.'s criticism of our recent solar dynamo model. A different treatment of the magnetic buoyancy is the most probable reason for their different results. |
Formato |
application/pdf |
Identificador |
http://eprints.iisc.ernet.in/27762/1/Astro.pdf Choudhuri, AR and Nandy, D and Chatterjee, P (2005) Comments on "Full-sphere simulations of circulation-dominated solar dynamo: Exploring the parity issue" - Reply. In: Astronomy & Astrophysics, 437 (2). 703 -704. |
Publicador |
EDP Sciences |
Relação |
http://www.aanda.org/index.php?option=article&access=doi&doi=10.1051/0004-6361:20052934 http://eprints.iisc.ernet.in/27762/ |
Palavras-Chave | #Physics |
Tipo |
Journal Article PeerReviewed |