{ "id": 4322, "url": "https://svs.gsfc.nasa.gov/4322/", "page_type": "Visualization", "title": "The Multiple CMEs of June, 2015", "description": "A view of multiple CMEs which erupted from the Sun in the latter half of June 2015. 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Different colors of a red, green, blue color palette are used to designate different physical variables from the simulation. When the three colors combine, they create a dramatic example of how the coronal mass ejection (CME) is different from the solar wind.



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Again on June 25, 2015, a mid-level solar flare peaked at 4:16 a.m. EDT.NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. 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. To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at http://spaceweather.gov, the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This first flare is classified as an M6.6 flare and the second was M7.9. M-class flares are a tenth the size of the most intense flares, the X-class flares. The number provides more information about its strength. 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