File:SDO 20231020 000646 4096 0171 (AIA).jpg
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English: AIA 0171 channel is especially good at showing coronal loops - the arcs extending off of the Sun where plasma moves along magnetic field lines. The brightest spots seen here are locations where the magnetic field near the surface is exceptionally strong.
Where: Quiet corona and upper transition region Wavelength: 171 angstroms (0.0000000171 m) = Extreme Ultraviolet Primary ions seen: 8 times ionized iron (Fe IX) Characteristic temperature: 1 million K (1.8 million F) |
| Date | Taken on 20 October 2023, 00:06:46 |
| Source | 20231020_000646_4096_0171 |
| Author | Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. |
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This media is a product of the Solar Dynamics Observatory Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory |
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This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20231020_000646_4096_0171. This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing. Other languages:
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 05:15, 20 October 2023 | | 4,096 × 4,096 (2.72 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/browse/2023/10/20/20231020_000646_4096_0171.jpg via Commons:Spacemedia |
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