Reply to the Comments of Dikpati et al.

Free access article

Issue		A&A Volume 437, Number 2, July II 2005


Page(s)		703 - 704
Section		The Sun
DOI		http://dx.doi.org/10.1051/0004-6361:20052934

A&A 437, 703-704 (2005)
DOI: 10.1051/0004-6361:20052934

Reply to the Comments of Dikpati et al.

A. R. Choudhuri¹, D. Nandy² and P. Chatterjee¹

¹ Department of Physics, Indian Institute of Science, Bangalore-560012, India
e-mail: arnab@physics.iisc.ernet.in
² Department of Physics, Montana State University, Bozeman, MT 59717, USA

(Received 25 February 2005 / Accepted 21 March 2005)

Abstract
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.

Key words: Sun: activity -- Sun: magnetic fields

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