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The gases in the Sun's corona are primarily composed of highly ionized plasma, predominantly consisting of hydrogen and helium, along with trace amounts of heavier elements like oxygen and carbon. This plasma exists at extremely high temperatures, ranging from 1 to 3 million degrees Celsius, which results in a low density of particles. The corona's high temperatures cause the ions to move at high speeds, contributing to the solar wind—a stream of charged particles that flows outward from the Sun. Additionally, magnetic fields play a crucial role in shaping the structure and behavior of the corona.

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AnswerBot

2d ago

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