Coronal Loops in an Active Region of the Sun
An active region of the sun just rotating into the view of NASA's Solar
Dynamics Observatory gives a profile view of coronal loops over about a two-day
period, from Feb. 8-10, 2014. Coronal loops are found around sunspots and in
active regions. These structures are associated with the closed magnetic field
lines that connect magnetic regions on the solar surface. Many coronal loops
last for days or weeks, but most change quite rapidly. This image was taken in
extreme ultraviolet light.
Image Credit: NASA/Solar Dynamics
Observatory
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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