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Coronal radiative losses

Index Coronal radiative losses

In astronomy and in astrophysics, for radiative losses of the solar corona, it is meant the energy flux radiated from the external atmosphere of the Sun (traditionally divided into chromosphere, transition region and corona), and, in particular, the processes of production of the radiation coming from the solar corona and transition region, where the plasma is optically-thin. [1]

5 relations: Corona, Index of physics articles (C), List of plasma physics articles, Nanoflares, Sunlight.

Corona

A corona (Latin, 'crown') is an aura of plasma that surrounds the Sun and other stars.

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Index of physics articles (C)

The index of physics articles is split into multiple pages due to its size.

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List of plasma physics articles

This is a list of plasma physics topics.

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Nanoflares

A nanoflare is a very small episodic heating event which happens in the corona, the external atmosphere of the Sun.

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Sunlight

Sunlight is a portion of the electromagnetic radiation given off by the Sun, in particular infrared, visible, and ultraviolet light.

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References

[1] https://en.wikipedia.org/wiki/Coronal_radiative_losses

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