Steps for building a calibrated flux-transport dynamo for the Sun
Given the complexity involved in a flux-transport-type dynamo driven by both Babcock - Leighton and tachocline α effects, we present here a step-by-step procedure for building a flux-transport dynamo model calibrated to the Sun as a guide for anyone who wishes to build this kind of model. We show that a plausible sequence of steps to reach a converged solution in such a dynamo consists of (i) numerical integration of a classical α - ω dynamo driven by a tachocline α effect, (ii) continued integration with inclusion of meridional circulation to convert the model into a flux-transport dynamo driven by only a tachocline α effect, (iii) final integration with inclusion of a Babcock - Leighton surface α effect, resulting in a flux-transport dynamo that can be calibrated to obtain a close fit of model output with solar observations.
document
http://n2t.net/ark:/85065/d7tm7bb2
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2007-03-01T00:00:00Z
Copyright 2007 Springer Netherlands.
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