The Sun’s Surface in Stunning Detail

The Swedish Solar Telescope, run by the Institute for Solar Physics, can see at a resolution of up to 1.1 arc-seconds.

This corresponds to 70 km on the solar surface, meaning it can see details the size of a 10 cent euro coin at a distance of about 40 km. This was achieved by use of an adaptive optics system. The system relies on the EoSens ® CL by Mikrotron for high-speed imaging.
- See more at: http://mvrpl.com/eoSens-CL-high-speed-recording-camera-Case-Study-article-57.html#.VVGJ9PCBy1kThe Swedish Solar Telescope, run by the Institute for Solar Physics, can see at a resolution of up to 1.1 arc-seconds. This corresponds to 70 km on the solar surface, meaning it can see details the size of a 10 cent euro coin at a distance of about 40 km. This was achieved by use of an adaptive optics system. The system relies on the EoSens ® CL by Mikrotron for high-speed imaging.

The Swedish Solar Telescope, run by the Institute for Solar Physics, can see at a resolution of up to 1.1 arc-seconds. This corresponds to 70 km on the solar surface, meaning it can see details the size of a 10 cent euro coin at a distance of about 40 km. This was achieved by use of an adaptive optics system. The system relies on the EoSens ® CL by Mikrotron for high-speed imaging. 

Located on the Canary Island of La Palma, the Swedish 1-meter Solar Telescope (SST) is the world’s leading facility for high resolution observations of the Sun. It is operated by the Institute for Solar Physics (ISF), which is part of Stockholm University’s department for Astrophysics. Research at the institute primarily aims to gain knowledge about the outer layer of the solar atmosphere, which is dominated by magnetic fields. How do magnetic fields arise? How are they formed and ultimately destroyed or removed from the solar surface? How do they affect the Sun‘s outer atmosphere? How do they give rise to solar storms and the radiant energy that the Sun emits?

Read more Article on http://goo.gl/Q5YGCk


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