The granules in the photosphere are convection cells that transport heat from the interior of the Sun to its surface. They appear as bright areas surrounded by darker lanes and are typically about 1,000 kilometers in diameter. Granules are constantly forming, evolving, and disappearing as part of the Sun's dynamic atmosphere.
The photosphere of the Sun is the layer that contains granules and supergranules. Granules are small convective cells on the surface of the Sun, while supergranules are larger scale convective cells that are composed of multiple granules.
The bubbling characteristic of the photosphere is called solar granulation. These granules are caused by the convective motion of plasma beneath the surface of the Sun, creating cells of rising hot plasma and sinking cooler plasma that appear as granules on the photosphere.
The photosphere is the visible surface of the Sun, which appears as granules (the tops of convection cells). The "supergranules" are a pattern into which the granules may be clumped, and can be considered either structurally part of the photosphere or part of the convection zone that lies directly beneath it. Some sources extend the term "supergranulation" to include both the photosphere and the chromosphere (which does not, however, use convection).
Those are called granules. Granules are small convection cells on the surface of the sun, caused by hot gas rising and cooler gas sinking. They are typically about 1000 kilometers in diameter and last for about 5 to 10 minutes.
The layer of the Sun's atmosphere that produces its characteristic color is called the photosphere. It is the visible surface of the Sun and emits light in the form of electromagnetic radiation, giving the Sun its bright yellowish appearance. The photosphere is where sunspots and solar features like granules can be observed. Above the photosphere lies the chromosphere and the corona, which have different properties and appearances.
The photosphere of the Sun is the layer that contains granules and supergranules. Granules are small convective cells on the surface of the Sun, while supergranules are larger scale convective cells that are composed of multiple granules.
The bubbling characteristic of the photosphere is called solar granulation. These granules are caused by the convective motion of plasma beneath the surface of the Sun, creating cells of rising hot plasma and sinking cooler plasma that appear as granules on the photosphere.
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 evidence in the photosphere of the type of energy transport occurring beneath it is mainly through the observation of granulation patterns. Granules are the tops of convective cells that transport energy from the interior of the Sun to its surface. The size and shape of these granules give insights into the convective processes happening beneath the photosphere.
The photosphere is the visible surface of the Sun, which appears as granules (the tops of convection cells). The "supergranules" are a pattern into which the granules may be clumped, and can be considered either structurally part of the photosphere or part of the convection zone that lies directly beneath it. Some sources extend the term "supergranulation" to include both the photosphere and the chromosphere (which does not, however, use convection).
Those are called granules. Granules are small convection cells on the surface of the sun, caused by hot gas rising and cooler gas sinking. They are typically about 1000 kilometers in diameter and last for about 5 to 10 minutes.
The pattern of rising hot gas cells all over the photosphere is called granulation. These granules are caused by convective currents beneath the solar surface that transport heat from the interior to the outer layers of the Sun.
the sun has a photosphere.
the photosphere does nothing
The part of the sun that is going to emit the most visible light is going to be the Photosphere
Next to the Photosphere is the Subsurface flows.
photosphere.