In the convection zone, material close to the surface rises as heat moves outward from the lower layers of the surface. Upon the release of the heat of the gas at the surface, the gas drops down again as it replaced by the hotter gases below.
Convective zone.
Sunspots are regions of strong magnetic activity, which inhibits convection from below. The combination of the up-and down movement of gases within the Sun's convective zone and the movement of the sun's rotation produces magnetic fields. These magnetic fields slow down activity in the convective zone. Slower convection means that less gas is transferring heat from the core of the sun to the photosphere. Therefore, regions of the photosphere near strong magnetic fields are up to 3000 degrees Celsius cooler than surrounding areas.
Deuterium is an isotope of hydrogen, not a region of the sun.
False. The abyssal zone is not noted for its warm temperatures that are created by escaping gases.
Energy that is conducted via electromagnetic waves is conducted via radiation. The corresponding portion of the sun that moves energy this way is the radiative zone, located between the core and the convective zone.
Magnetic Fields
it does
The Sun is entirely made out of gases (mainly Hydrogen), but in a sate called 'plasma'. In the core of the Sun the plasma radiates, above this in the convective zone the plasma transfers heat to the surface by a process of convection.
The core, the radiative zone, and the convective zone.
Rainbow
The core, the radiative zone, and the convective zone.
The radiative zone, the convective zone, and the photosphere.
The core, the radiative zone, and the convective zone.
they are in the convective zone
Matter, obviosly.
Convective zone.
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.