Miloslav Druckmüller, Peter Aniol, Vojtech Rušin, Ľubomír Klocok, Karel Martišek, Martin Dietzel

Miloslav Druckmüller, Peter Aniol, Vojtech Rušin, Ľubomír Klocok, Karel Martišek, Martin Dietzel

The solar corona is the magnetically dominated atmosphere of the sun, reaching millions of miles into space. Paradoxically, the corona is many times hotter than the solar 'surface' (the photosphere) and solar physicists are currently trying to understand why this is the case.

The photosphere has an average temperature of approximately 6000 degrees Celsius, whereas the corona can be millions of degrees Celsius. This is analogous to the air surrounding a hot light bulb being hotter than the bulb itself; in reality, the air surrounding the bulb is cooler than the bulb's glass surface, and it gets cooler the further you move your hand away.

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There are many ideas as to why the sun's atmosphere is hotter than the solar surface, but the leading theories all have a common theme: the coronal heating mechanism has something to do with the powerful magnetic field lines that thread through the corona.

Physicists have found observational evidence for magnetic waves that propagate from the sun and through the corona. These waves possibly 'resonate' with the plasma, heating it up to multi-million degree temperatures. Other theories suggest the magnetic field lines 'snap' and then reconnect, releasing energy as small flares (called 'nanoflares'), heating the plasma.

Although the sun's atmosphere is many times hotter than the sun itself, it is also many times thinner. As a result, it produces very little light and it can only be observed if the glare of the sun is blocked out. In this fantastically detailed photograph, the moon has covered the disk of the sun from sight, allowing the solar corona to glow.

This photograph of a total solar eclipse was taken by Miloslav Druckmüller and colleagues from Brno University of Technology, Czech Republic, during an eclipse on July 22, 2009. They were located on Enewetak Atoll in the Marshall Islands.

The sun was completely blocked by the moon (a period known as 'totality') for 5 minutes and 41 seconds. In that time, Druckmüller was able to take a series of images that were combined and processed to produce this final product. Features usually hidden from view can now be seen including lunar impact craters and the intricate detail of the magnetic field lines inside the corona.

For further image details, equipment used and a spectacular high-resolution photograph, visit Miloslav Druckmüller's eclipse webpage.

Thanks to Mary Mactavish for the tip.