Prominerces
The reddish loops of gas that link parts of sunspot regions are known as solar prominences. These large, bright features extend outward from the Sun's surface and are composed of plasma, a hot ionized gas. Prominences are often associated with the Sun's magnetic field and can be seen during solar eclipses as they rise above the solar limb. They can vary in size and shape and may last from days to weeks before dissipating.
Different parts of the Sun rotate at different speeds, which is how we know that the Sun isn't a solid. The equatorial regions of the Sun rotate in about 27 days, but the polar regions take a little longer; about 33 days.
Virtual Prototypes
The six main regions of Earth are Africa, Asia, Europe, North America, South America, and Oceania (Australia and the Pacific islands). These regions are commonly used in geography to categorize different parts of the world based on their location and characteristics.
Prominerces
prominence
prominence
These loops are called penumbral fibrils. They are structures of hot gas in the sun's photosphere that connect different parts of sunspots, contributing to the magnetic activity and energy transfer within those regions.
They are solar prominences.
Prominence.
Yes
It has to be solar flares, supra-sunspots, solar wind, or prominences.
regions
Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.
Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.
The reddish loops of gas that link parts of sunspot regions are known as solar prominences. These structures are made of plasma and can extend thousands of kilometers into the solar atmosphere, known as the corona. Prominences are often associated with the magnetic fields around sunspots and can be seen during solar eclipses or using specialized telescopes. Their dynamic nature can lead to eruptions, which are called solar flares.