k Eruptive solar prominence Eruptive solar prominence around the suns limb captured on the 5th January 2023. Prominences are dense clouds of plasma, or ionised gas, in the Suns outer layer, the corona. Upon erupting, the flares become part of the solar wind. They may be associated with strong magnetic activity inside the Sun, and some flares are powerful enough that, on reaching Earth, they can disrupt telecommunications and satellite systems. Solar flares can extend hundreds of thousands of kilometres into space. Captured from the Dark Sky Alqueva region, Portugal., by MIGUEL CLAROSCIENCE PHOTO LIBRARY Stock Photo - Afloimages
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Eruptive solar prominence Eruptive solar prominence around the sun s limb captured on the 5th January 2023. Prominences are dense clouds of plasma, or ionised gas, in the Sun s outer layer, the corona. Upon erupting, the flares become part of the solar wind. They may be associated with strong magnetic activity inside the Sun, and some flares are powerful enough that, on reaching Earth, they can disrupt telecommunications and satellite systems. Solar flares can extend hundreds of thousands of kilometres into space. Captured from the Dark Sky Alqueva region, Portugal., by MIGUEL CLARO SCIENCE PHOTO LIBRARY
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Eruptive solar prominence

Eruptive solar prominence around the sun's limb captured on the 5th January 2023. Prominences are dense clouds of plasma, or ionised gas, in the Sun's outer layer, the corona. Upon erupting, the flares become part of the solar wind. They may be associated with strong magnetic activity inside the Sun, and some flares are powerful enough that, on reaching Earth, they can disrupt telecommunications and satellite systems. Solar flares can extend hundreds of thousands of kilometres into space. Captured from the Dark Sky Alqueva region, Portugal., by MIGUEL CLARO/SCIENCE PHOTO LIBRARY

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