REAL

On the Compatibility of a Flux Transport Dynamo with a Fast Tachocline Scenario

Karak, BB and Petrovay, Kristóf (2013) On the Compatibility of a Flux Transport Dynamo with a Fast Tachocline Scenario. SOLAR PHYSICS, 282 (2). pp. 321-334. ISSN 0038-0938

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Abstract

The compatibility of the fast-tachocline scenario with a flux-transport dynamo model is explored. We employ a flux-transport dynamo model coupled with simple feedback formulae relating the thickness of the tachocline to the amplitude of the magnetic field or to the Maxwell stress. The dynamo model is found to be robust against the nonlinearity introduced by this simplified fast-tachocline mechanism. Solar-like butterfly diagrams are found to persist and, even without any parameter fitting, the overall thickness of the tachocline is well within the range admitted by helioseismic constraints. In the most realistic case of a time-and latitude-dependent tachocline thickness linked to the value of the Maxwell stress, both the thickness and its latitudinal dependence are in excellent agreement with seismic results. In nonparametric models, cycle-related temporal variations in tachocline thickness are somewhat larger than admitted by helioseismic constraints; we find, however, that introducing a further parameter into our feedback formula readily allows further fine tuning of the thickness variations.

Item Type: Article
Uncontrolled Keywords: MODEL; CYCLE; MAGNETIC-FIELD; Confinement; ZONES; MERIDIONAL CIRCULATION; DIFFERENTIAL ROTATION; TACHOCLINE; FAST SOLAR TACHOCLINE; Dynamo; MINIMUM;
Subjects: Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika
SWORD Depositor: MTMT SWORD
Depositing User: MTMT SWORD
Date Deposited: 17 Jun 2024 14:01
Last Modified: 17 Jun 2024 14:01
URI: https://real.mtak.hu/id/eprint/197687

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