A Coronal loop.
The fiery arms or loops extending from the sun's surface are called solar prominences. These are large, bright features that extend outward from the sun's surface, often in a loop shape, and are composed of plasma. Solar prominences are associated with the sun's magnetic field and can last for several hours to days before dissipating.
A loop of relatively cool gas on the surface of the sun is known as a solar prominence. These features are composed of ionized gas, or plasma, and are often observed as large, bright arcs or loops that extend outward from the sun's surface. Solar prominences are held in place by the sun's magnetic fields and can last for days or weeks before dissipating or collapsing back to the sun's surface. They are typically cooler than the surrounding solar atmosphere, which contributes to their distinct appearance.
yes they are
In the Sun's radiative zone, energy is transferred through radiation, where photons are absorbed and re-emitted by particles, taking a long time—up to thousands of years—to reach the outer layers. In the convective zone, energy transfer occurs via convection, where hot plasma rises to the surface, cools, and then sinks, creating a continuous cycle that efficiently transports energy to the Sun’s surface. This combination of radiative and convective processes ensures that energy generated in the core eventually reaches the surface, where it can radiate into space.
The reddish loops of gas seen in outer space are called prominences. Prominences are dense, cooler plasma suspended above the Sun's surface by magnetic forces, giving them their distinct loop-like appearance.
It is a very bright mass of roiling gas or plasma.
The fiery arms or loops extending from the sun's surface are called solar prominences. These are large, bright features that extend outward from the sun's surface, often in a loop shape, and are composed of plasma. Solar prominences are associated with the sun's magnetic field and can last for several hours to days before dissipating.
The Sun does not have a "crust"; the surface of the Sun is 12,000 degree-hot hydrogen plasma.
The path of photons through the Sun's plasma is called radiative diffusion. Photons travel through the Sun's plasma by bouncing off charged particles in a random walk pattern until they reach the surface and are emitted as sunlight.
Corona is a type of plasma "atmosphere" of the Sun
Chromosphere
photosphere
Tears in the suns corona provide an exit for solar winds. Solar wind are a released stream of plasma from the sun.
You can see Solar Flares in the Suns' Corona. corona (apex)
sunspots
"The core is made of hot, dense gas in the plasmic state"
You can still get free parking on the suns surface.