Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Department of Astronomy, IAG, University of Sao Paulo, Sao Paulo, SP, Brazil
Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model
Flux-dominated solar dynamo model with a thin shear layer
How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo?
Kinematic solar dynamo models with a deep meridional flow
The role of diffusivity quenching in flux-transport dynamo models
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