Search Publications

Turbulent convective flows in the solar photospheric plasma

Giannattasio, F.; Berrilli, F.; Consolini, G. +3 more

> The origin of the 22-year solar magnetic cycle lies below the photosphere where multiscale plasma motions, due to turbulent convection, produce magnetic fields. The most powerful intensity and velocity signals are associated with convection cells, called granules, with a scale of typically 1 Mm and a lifetime of a few minutes. Small-scale mag…