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Magnetic fields of low-mass stars and planets are thought to originate from self-excited dynamo action in their convective interiors. Observations reveal a variety of field topologies ranging from lar...
Helicity of Solar Active Regions from a Dynamo Model      MHD—Sun  activity—Sun  magnetic fields—sunspots       font style='font-size:12px;'> 2010/9/16
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...
Some Recent Developments in Solar Dynamo Theory      Sun  magnetic field  sunspots  solar cycle  MHD       font style='font-size:12px;'> 2010/9/16
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...
Global Solar Dynamo Models: Simulations and Predictions      Sun  magnetic fields  solar cycle  dynamo  predictio       font style='font-size:12px;'> 2010/9/15
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...
The Earth’s global magnetic field is generated in its metallic core, located nearly 3,000 kilometers beneath the planet’s surface. The field has existed on Earth for at least 3.5 billion years and off...
Some Recent Developments in Solar Dynamo Theory     Sun:magnetic field-sunspots-solar  cycle-MHD       font style='font-size:12px;'> 2009/5/7
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...
Helicity of Solar Active Regions from a Dynamo Model     MHD  Sun:activity  Sun:magnetic fields  sunspots       font style='font-size:12px;'> 2009/5/7
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...
Global Solar Dynamo Models:Simulations and Predictions     Sun  magnetic fields: solar cycle  dynamo  prediction       font style='font-size:12px;'> 2009/5/5
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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