File:SDO 20171001 1024 0335 (AIA).ogv
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[edit]DescriptionSDO 20171001 1024 0335 (AIA).ogv |
English: AIA 0335 channel (as well as AIA 211) highlights the active region of the outer atmosphere of the Sun - the corona. Active regions, solar flares, and coronal mass ejections will appear bright here. The dark areas - or coronal holes - are places where very little radiation is emitted, yet are the main source of solar wind particles.
Where: Active regions of the corona Wavelength: 335 angstroms (0.0000000335 m) = Extreme Ultraviolet Primary ions seen: 15 times ionized iron (Fe XVI) Characteristic temperature: 2.8 million K (5 million F) |
Date | Taken on 1 October 2017 |
Source | 20171001_1024_0335 |
Author | Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. |
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 |
This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20171001_1024_0335. 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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current | 02:38, 13 February 2024 | 4.8 s, 1,024 × 1,024 (2.14 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2017/10/01/20171001_1024_0335.ogv via Commons:Spacemedia |
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