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2012) instrument onboard the NASA Solar Dynamics Observatory (SDO; It is one of three instruments on SDO, along with the Helioseismic and Magnetic Imager (HMI; With its high spatial (0.6 per pixel) and temporal (up to 12 seconds for most channels) resolution, AIA has greatly enhanced our understanding of our closest star in a number of different areas, including the initiation of flares and coronal mass ejections as well as the quiescent heating of the corona, the outermost layer of the Sun's atmosphere. AIA is a narrowband imaging instrument comprised of four separate telescopes that collectively observe the full-disk of the Sun at ten different wavelengths: seven extreme ultraviolet (EUV) wavelengths, two far UV wavelengths, and one visible wavelength. It produces nearly 60,000 images per day with a new 4K-by-4K image produced by each EUV channel every 12 seconds. The image data are provided to the community by the Joint Science Operations Center (JSOC) at Stanford
Barnes et al. (Mon,) studied this question.
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