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Solar prominences

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15y ago

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Related Questions

Are reddish loops of gas called prominences link sunspots?

no


What are reddish loops of gas that connect sunspot regions?

prominences


What are reddish loops of gas that connect different parts of sunspots regions?

prominence


What is reddish loops of gas that connect different parts of sunspots regions?

Prominerces


What are reddish loops of gas that connect different parts of sunspot regions?

prominence


What are reddish loops of gas that connect differint parts of sunspot regions?

Prominence.


What or reddish loops of gas that connects different parts of sunspot regions?

They are solar prominences.


What are reddish loops of gas that connect different parts of sunspot region?

Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.


What are reddish loops of gas that connects different parts of sunspot region?

Solar prominences, they are loops of plasma captured by magnetic flux lines linking individual sunspots.


What Reddish loops of gas that link parts of sunspot 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.


What are the reddish loops of gas that link parts of sunspot reigons?

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.


What are reddish loop of gas quick connect different part of the sunspot regions?

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.