k Artwork of solar prominence on surface of sun Solar prominence. Illustration of a loopshaped solar prominence erupting from the surface of the Sun. Solar prominences consist of plasma charged particles produced when atoms of hydrogen are torn apart by immense heat. The eruptions are usually confined within tubeshaped magnetic fields, resulting in loops like this one. The yellow area at lower right is the photosphere, the Suns surface. Above this is a red layer of hydrogen gas called the chromosphere. The Sun is powered by a gigantic, uncontrolled nuclear fusion explosion in its core, where temperatures reach at least 14 million degrees C. It loses mass at a rate of around four million tons per second. Stock Photo - Afloimages
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Artwork of solar prominence on surface of sun Solar prominence. Illustration of a loop shaped solar prominence erupting from the surface of the Sun. Solar prominences consist of plasma   charged particles produced when atoms of hydrogen are torn apart by immense heat. The eruptions are usually confined within tube shaped magnetic fields, resulting in loops like this one. The yellow area at lower right is the photosphere, the Sun s surface. Above this is a red layer of hydrogen gas called the chromosphere. The Sun is powered by a gigantic, uncontrolled nuclear fusion explosion in its core, where temperatures reach at least 14 million degrees C. It loses mass at a rate of around four million tons per second.
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Artwork of solar prominence on surface of sun

Solar prominence. Illustration of a loop-shaped solar prominence erupting from the surface of the Sun. Solar prominences consist of plasma - charged particles produced when atoms of hydrogen are torn apart by immense heat. The eruptions are usually confined within tube-shaped magnetic fields, resulting in loops like this one. The yellow area at lower right is the photosphere, the Sun's surface. Above this is a red layer of hydrogen gas called the chromosphere. The Sun is powered by a gigantic, uncontrolled nuclear fusion explosion in its core, where temperatures reach at least 14 million degrees C. It loses mass at a rate of around four million tons per second.

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