Comments on "Full-sphere simulations of circulation-dominated solar dynamo: Exploring the parity issue" - Reply


Autoria(s): Choudhuri, AR; Nandy, D; Chatterjee, P
Data(s)

01/07/2005

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