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| Artist impression of NASA’s Interface Region Imaging Spectrograph (IRIS) [Credit: NASA] |
The interface region lies between the sun's 11,000-degree Fahrenheit, white-hot, visible surface, the photosphere, and the much hotter multi-million-degree upper corona. Interactions between the violently moving plasma and the sun's magnetic field in this area may be the source of the energy that heats the corona to some hundreds and occasionally thousands of times hotter than the sun's surface.
IRIS mission trailer video showing an active solar surface [Credit:NASA]
IRIS will orbit Earth and use its ultraviolet telescope to obtain high-resolution solar images and spectra. IRIS observations along with advanced computer models will deepen our understanding of how heat and energy move through the lower atmosphere of the sun and other sun-like stars.
For more information about NASA's IRIS mission, please visit: http://www.nasa.gov/iris
Source: NASA [May 20, 2013]






