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Reply to the Comments of Dikpati et al.

Choudhuri, AR and Nandy, D and Chatterjee, P (2005) Reply to the Comments of Dikpati et al. In: Astronomy & Astrophysics, 437 (2). pp. 703-704.

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We respond to Dikpati et al.'s (2005) criticism of our recent solar dynamo model (Chatterjee et al. 2004). A different treatment of the magnetic buoyancy is the most probable reason for their different results.

Item Type: Journal Article
Publication: Astronomy & Astrophysics
Publisher: EDP Sciences
Additional Information: Copyright for this article belongs to EDP Sciences.
Keywords: Sun:activity;Sun:magnetic fields
Department/Centre: Division of Physical & Mathematical Sciences > Physics
Date Deposited: 04 Jan 2006
Last Modified: 19 Sep 2010 04:22
URI: http://eprints.iisc.ac.in/id/eprint/4610

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