KnowraSolar dynamoLinked fromLinked fromThe 15 pages that link to Solar dynamo, each with the reason it gives.All 15Broader topic 1Related 9Narrower topic 5Solar cycleRelated: Differential rotation and convection drive the magnetic-field changes that structure the cycle.Solar magnetic fieldRelated: Differential rotation and convection continually regenerate the field.SunRelated: Its magnetic cycles drive sunspots, flares, and changes in solar activity.HelioseismologyRelated: Helioseismic flow maps constrain dynamo models, but the mechanism generating the solar cycle remains unsettled.Convection zoneRelated: Convection supplies moving, electrically conducting plasma that helps drive the solar magnetic cycle.Radiative zoneRelated: The shear at the radiative–convective boundary contributes to models of the solar magnetic cycle.Solar physicsRelated: It explains the magnetic cycle that underlies sunspots and many forms of solar activity.Space physicsRelated: Its operation sets the magnetic cycles that shape long-term heliospheric conditions.HeliophysicsRelated: Its details govern the origin and evolution of the solar cycle.