the loop of gas is called prominence.
They are solar prominences.
The two parts of a sunspot are the dark central region called the umbra and the lighter surrounding region called the penumbra. The umbra is cooler than the surrounding regions and is where the magnetic field is most intense.
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.
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.
Those are known as umbral dots or light bridges. They are regions of intense magnetic fields on the Sun's surface that appear as bright, thread-like structures connecting different parts of sunspots. These features are often associated with increased solar activity and can be indicators of sunspot evolution.
prominence
Yes
They are solar prominences.
Magnetic field lines.
Prominence.
The two parts of a sunspot are the dark central region called the umbra and the lighter surrounding region called the penumbra. The umbra is cooler than the surrounding regions and is where the magnetic field is most intense.
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.
The basic parts of the sun are CORONA,SUNSPOT,and PROMINENCE.
It has to be solar flares, supra-sunspots, solar wind, or prominences.
regions
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.
Those are known as umbral dots or light bridges. They are regions of intense magnetic fields on the Sun's surface that appear as bright, thread-like structures connecting different parts of sunspots. These features are often associated with increased solar activity and can be indicators of sunspot evolution.