Photosphere
The layer that surrounds the radiation zone of the sun is the convection zone. In this zone, energy is transferred by the movement of hot plasma rising and cooler plasma sinking, creating a convection current. This process allows energy to be transported from the core to the surface of the sun.
The layers of the sun from inside out are the core, radiative zone, convective zone, photosphere, chromosphere, and corona. The core is the densest layer, with a density of about 150 g/cm3. As you move outward, the density decreases, with the corona being the least dense layer.
From the Sun's core, energy moves through the radiative zone, across the tachocline (transition layer) to the convective zone, and then to the outer convective zone with its visible granulation.
From outermost layer to innermost layer: corona, chromosphere, photosphere, subsurface flows, convection zone, radiative zone, inner core.
The portion of the sun in which energy moves from atom to atom in the form of waves is called the?
In the convection Zone!
The layer that surrounds the radiation zone of the sun is the convection zone. In this zone, energy is transferred by the movement of hot plasma rising and cooler plasma sinking, creating a convection current. This process allows energy to be transported from the core to the surface of the sun.
The convection zone.
The convection zone
The convection zone in a star like the Sun is located just beneath the photosphere. It is the layer where energy generated in the star's core is transported to the surface via convection currents, providing the energy needed for the star to shine.
The layers of the sun from inside out are the core, radiative zone, convective zone, photosphere, chromosphere, and corona. The core is the densest layer, with a density of about 150 g/cm3. As you move outward, the density decreases, with the corona being the least dense layer.
From the Sun's core, energy moves through the radiative zone, across the tachocline (transition layer) to the convective zone, and then to the outer convective zone with its visible granulation.
From outermost layer to innermost layer: corona, chromosphere, photosphere, subsurface flows, convection zone, radiative zone, inner core.
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.
The convection zone.
The sun has many different layers that make up the sun: Core Radiation Zone Convection Zone Photosphere- sunspots Chromosphere Transition Region Corona The Core is the layer that stores all of the sun's energy. The Radiation Zone transfers the energy that the Core passes. The Convection Zone carries the sun's energy to the surface. The Photosphere is the visible surface of the sun. The Chromosphere is a thin surface above the Photosphere. The Corona is the sun's atmospheric layer.
They are the Convection Zone, Radiative Zone, then the Core.