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SPACE-SUN-SOLAR FLARE
This image obtained August 27, 2014 shows a close-up of a moderate Sun flare of light on August 24, 2014 in the 131 and 171 Angstrom wavelengths. The former wavelength, usually colorized in teal, highlights the extremely hot material of a flare. The latter, usually colorized in gold, highlights magnet loops in the sun's atmosphere. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. This flare is classified as an M5 flare. M-class flares are ten times less powerful than the most intense flares, called X-class flares. AFP PHOTO/NASA/SDO/HANDOUT = RESTRICTED TO EDITORIAL USE - MANDATORY CREDIT "AFP PHOTO / NASA/SDO/ HANDOUT" - NO MARKETING NO ADVERTISING CAMPAIGNS - NO A LA CARTE SALES/DISTRIBUTED AS A SERVICE TO CLIENTS =
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Detalii fotografie |
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-, SPACE |
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Sursa: |
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AFP / Mediafax Foto |
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Fotograf: |
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HANDOUT |
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Data: |
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27 August 2014 |
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Dimensiuni: |
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1726 x 1694 (579.88 KB) |
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