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We calculate helicities of solar active regions based on the idea that poloidal flux lines get wrapped around a toroidal flux tube rising through the convection zone, thereby giving rise to the helici...
We discuss the current status of solar dynamo theory and describe the dynamo model developed by our group. The toroidal magnetic field is generated in the tachocline by the strong differential rotatio...
Flux-transport type solar dynamos have achieved considerable success in correctly simulating many solar cycle features, and are nowbeing used for prediction of solar cycle timing and amplitude.We firs...
We discuss the current status of solar dynamo theory and describe the dynamo model developed by our group. The toroidal magnetic field is generated in the tachocline by the strong differential rotatio...
We calculate helicities of solar active regions based on the idea that poloidal flux lines get wrapped around a toroidal flux tube rising through the convection zone, thereby giving rise to the helici...
Flux-transport type solar dynamos have achieved considerable success in correctly simulating many solar cycle features, and are nowbeing used for prediction of solar cycle timing and amplitude.We fi...

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