The sun is nearing the peak of its magnetic activity cycle, leading to more sunspots, storms, and potential danger for Earth due to the ionized gas-induced magnetism.
The sun's magnetic field is generated by ionized gas in its interior, with each locally generated field shaping a parcel of the solar interior, contributing to the overall 11-year solar magnetic cycle.
The sun's dynamics involve hot material rising to the surface, cooling, and sinking again in thermal convection, similar to water in a teakettle, transferring heat from the solar interior to space.
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