Corona
Solar prominences are large looping structures of hot, glowing gas that extend from the Sun’s surface into the outer atmosphere, or corona. They can be seen during total solar eclipses or with special equipment that blocks out the brightness of the Sun. Prominences are caused by complex magnetic interactions within the Sun.
Prominences are ribbons of gas on the sun, similar to solar flares, that shoot upwards millions of miles into space. They are usually shaped like a loop. They are attached to the sun's photosphere, and extend into the corona.
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.
known as solar prominences. These structures are formed by the interaction of the Sun's magnetic field with ionized gases like hydrogen. Solar prominences can extend outwards from the Sun for thousands of kilometers and can be observed during a total solar eclipse.
Solar prominence are seen in the photosphere of the sun that goes further in the corona. These prominences can reach out over thousands of kilometers.
Corona
Prominences
Solar prominences are large looping structures of hot, glowing gas that extend from the Sun’s surface into the outer atmosphere, or corona. They can be seen during total solar eclipses or with special equipment that blocks out the brightness of the Sun. Prominences are caused by complex magnetic interactions within the Sun.
Spicules are small, needle-like structures found in sponges, while prominences refer to the large, arching structures seen on the Sun's surface.
Prominences are ribbons of gas on the sun, similar to solar flares, that shoot upwards millions of miles into space. They are usually shaped like a loop. They are attached to the sun's photosphere, and extend into the corona.
Prominences are magnetic structures on the Sun trapped by the Sun's magnetic field. They are made up of hot plasma and are often seen as loops or arcs extending from the Sun's surface into its outer atmosphere.
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.
known as solar prominences. These structures are formed by the interaction of the Sun's magnetic field with ionized gases like hydrogen. Solar prominences can extend outwards from the Sun for thousands of kilometers and can be observed during a total solar eclipse.
Sun spots and prominences.
Solar prominences are plasma rings that extend from the surface of the Sun, on outward.
Prominences seen straight on are called filaments. They are seen as silhouette against the solar disk. Prominences refers to features that are cloud-like in the solar atmosphere.