It goes out from the core into the radiation zone then into the convection zone where convection happens then it goes to the photosphere to become granules.
core-photosphere-chromosphere-corona
The sun's four main areas are the core, the radiative zone, the convective zone, and the photosphere. The core is where nuclear fusion occurs, generating energy. The radiative and convective zones are layers of the sun where energy is transported outward through different mechanisms. The photosphere is the visible surface of the sun.
The layers of the sun, from the center outward, are the core, the radiative zone, the convective zone, the photosphere, the chromosphere, and the corona.
The suns core is the innermost portion or the photosphere of the sun. It's the hottest layer and under the highest pressure, enabling nuclear fusion to take place, which produces the energy. The suns core temperature is estimated to be around 13.6 million degrees Kelvin.
The energy flow in the Sun's photosphere primarily involves the transfer of energy generated in its core through nuclear fusion. This energy moves outward as radiation, first through the radiative zone and then through the convective zone, where it is transported by convection currents. Once it reaches the photosphere, energy is emitted as visible light, heat, and other forms of electromagnetic radiation, providing the sunlight we observe on Earth. The photosphere acts as the visible surface of the Sun, where temperature and pressure conditions allow this energy to escape into space.
The Photosphere
In the Sun's core.
The sun has three main layers: the core, where nuclear fusion occurs; the radiative zone, where energy is transported by electromagnetic radiation; and the convective zone, where energy is transported by convection. The sun's atmosphere includes the photosphere, chromosphere, and corona.
The photosphere
The energy transport just below the sun's photosphere is mainly by convection. Convection is the process where hot material rises, cools down, and then sinks back down to be reheated, creating a cycle of energy transfer. This convection zone helps move heat from the sun's core to its surface.
photosphere
In the Sun's core.