Advection-dominated solar dynamo model with two-cell meridional flow and a positiveα -effect in the tachocline-Reference-Cited by-同舟云学术

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Advection-dominated solar dynamo model with two-cell meridional flow and a positiveα -effect in the tachocline

Published:2006-08 Issue:7 Volume:327 Page:680-685
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr.

Author:

Bonanno A.,Elstner D.,Belvedere G.

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. Three-dimensional stability of the solar tachocline

2. Parity properties of an advection-dominated solar $\mathsf{\alpha^2 \Omega}$-dy na mo

3. Helioseismic Measurements of the Subsurface Meridional Flow

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1. Dynamo models of the solar cycle;Living Reviews in Solar Physics;2020-06-17

2. A NEW SIMPLE DYNAMO MODEL FOR STELLAR ACTIVITY CYCLE;The Astrophysical Journal;2016-06-14

3. Observing Dynamos in Cool Stars;Space Sciences Series of ISSI;2015

4. Magnetic Polarity Reversals in the Core;Treatise on Geophysics;2015

5. Observing Dynamos in Cool Stars;Space Science Reviews;2014-09-05

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