File:SDO 20171224 001141 4096 0193 (AIA).jpg

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DescriptionSDO 20171224 001141 4096 0193 (AIA).jpg	English: AIA 0193 channel highlights the outer atmosphere of the Sun - called the corona - as well as hot flare plasma. Hot active regions, solar flares, and coronal mass ejections will appear bright here. The dark areas - called coronal holes - are places where very little radiation is emitted, yet are the main source of solar wind particles. Where: Corona and hot flare plasma Wavelength: 193 angstroms (0.0000000193 m) = Extreme Ultraviolet Primary ions seen: 11 times ionized iron (Fe XII) Characteristic temperature: 1.25 million K (2.25 million F)
Date	Taken on 24 December 2017, 00:11:41
Source	20171224_001141_4096_0193
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

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Solar Dynamics Observatory
Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory

This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20171224_001141_4096_0193.

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