They are solar prominences.
prominences
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.
Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.
The loop of gas that links different parts of sunspot regions is called a filament. Filaments are cooler and denser structures that appear as dark lines against the brighter surface of the Sun. These structures are supported by magnetic fields and can sometimes erupt, leading to solar flares or coronal mass ejections.
An example of a sunspot is the group of dark spots visible on the Sun's surface, caused by intense magnetic activity. Sunspots appear darker than their surrounding regions due to their lower surface temperatures. They usually occur in regions of strong magnetic fields on the solar surface.
prominence
prominences
Prominence.
Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.
Yes
Magnetic field lines.
Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.
solar flare
They are called the prominence.
The loop of gas that links different parts of sunspot regions is called a filament. Filaments are cooler and denser structures that appear as dark lines against the brighter surface of the Sun. These structures are supported by magnetic fields and can sometimes erupt, leading to solar flares or coronal mass ejections.
Sunspot regions appear as dark areas in X-ray images of the Sun, as they are cooler compared to the surrounding active regions. This contrast helps in distinguishing sunspots from other solar features that emit more X-rays. The size and shape of the sunspot region in X-ray images depend on its magnetic field strength and orientation.
An example of a sunspot is the group of dark spots visible on the Sun's surface, caused by intense magnetic activity. Sunspots appear darker than their surrounding regions due to their lower surface temperatures. They usually occur in regions of strong magnetic fields on the solar surface.