Final answer:
The convection zone inside the sun is characterized by large cells of rising and sinking gases that transport heat to the sun's surface.
Step-by-step explanation:
One characteristic of the convection zone inside the sun is large cells of rising and sinking gases. These giant convection cells transport energy from the edge of the radiative zone to the surface, similar to how heat circulates in a pot of boiling oatmeal. Hot plasma from the bottom of the convection zone rises to the surface, cools, then sinks to create a continuous flow. This process efficiently carries heat from the interior of the Sun to its surface.