Solar Active Regions

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Sun, Solar Activity

Scientific paper

Solar active regions form where the tops of loops of magnetic flux, shaped like the Greek letter omega (Ω), emerge into the solar atmosphere where they can be seen. These Ω loops are thought to be generated by the solar dynamo, located deep within the Sun (see DYNAMOS: SOLAR AND STELLAR). The appearance of active regions depends greatly on the radiation used to image them, as well as the angle at...

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