Prominence.
prominences
prominence
They are solar prominences.
solar flare
They are called the prominence.
The reddish loops of gas observed in sunspot regions are known as solar prominences. These prominences are large, bright features that extend outward from the Sun's surface, often associated with sunspots and magnetic field lines. They consist of hot plasma and can appear as arcs or loops, showcasing the Sun's magnetic activity. Their dynamic nature can lead to eruptions, contributing to solar flares and coronal mass ejections.
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.
The explosions that occur when loops in sunspot regions suddenly connect are called solar flares. These flares are powerful bursts of energy and radiation that are released from the Sun's surface. Solar flares can have various effects on Earth, including disrupting communication systems and causing geomagnetic storms.
solar flare
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.
The layer of the Sun where eruptions occur due to the sudden connection of loops in sunspot regions is the corona. These eruptions, known as solar flares, are caused by the release of magnetic energy stored in the corona. The interactions and reconnections of magnetic field lines in this outer atmosphere can lead to significant bursts of energy and matter into space.