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\\nCoronal Mass Ejections (Source: Solar Dynamics Observatory)
Solar flares are sometimes accompanied by coronal mass ejections (CMEs). CMEs are also formed by reorganization of the Sun’s magnetic field lines. They consist of energetic charged particles which travel at high speed, taking about 15-18 hours to several days to reach our planet.
\\n\\nCoronal Mass Ejections (Source: NASA/SDO)
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