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    "title": "Active Sun in Early May, 2022",
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            "description": "Solar flares are powerful bursts of energy. Flares and solar eruptions can impact radio communications, electric power grids, navigation signals, and pose risks to spacecraft and astronauts.<br><br>This flare is classified as an X-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. More info on how flares are classified can be found here.<br><br>To see how such space weather may affect Earth, please visit NOAA’s Space Weather Prediction Center https://spaceweather.gov/, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts. NASA works as a research arm of the nation’s space weather effort. NASA observes the Sun and our space environment constantly with a fleet of spacecraft that study everything from the Sun’s activity to the solar atmosphere, and to the particles and magnetic fields in the space surrounding Earth.",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of an X1.1 solar flare – as seen in the bright flash in the upper right portion of the image – on May 3, 2022 at 13:25 UTC. The image is a wavelength of extreme ultraviolet light – 171 angstrom –  that highlights coronal loop structures and which is colorized yellow.<p>Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of an M 5.3 solar flare on May 3, 2022. The image shows a blend 171 and 131 angstrom light: extreme ultraviolet light that highlights the extremely hot material in flares, and which is colorized in yellow. Credit: NASA/SDO",
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            "page_type": "Visualization",
            "title": "Solar X-flare. May 3, 2022",
            "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.These imagery cover the time frame of an X1.1 flare (lower left). || ",
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                "alt_text": "The solar flare as seen in AIA 131 Angstrom filter. No correction is applied for the instrument Point-Spread Function (PSF).",
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