This newly-released image from NASA changes all that. Captured by the Solar Dynamics Observatory, the effects of processing can show some of the structures usually obscured by the sun's blinding light.

© Rex Features / NASA
The original frames feature the 171 Angstrom wavelength of extreme ultraviolet, which shows plasma in the solar atmosphere.
Known as the corona, the temperature of this plasma is around 600,000 Kelvin and its loops are held in place by magnetic fields.
These loops are concentrated in active regions where the field is strongest, and they usually appear visibly as sunspots.
Want some more? Well, the people at NASA have made a wonderful video representing 24 hours of activity on September 25, 2011.



