Extreme ultraviolet light streams out of an X-class solar flare as seen in this image captured on March 29, 2014, by NASA's Solar Dynamics Observatory. This image blends two wavelengths of light 304 and 171 Angstroms, which help scientists observe the lower levels of the sun's atmosphere. More info The sun emitted a significant solar flare, peaking at 1 48 p.m. EDT March 29, 2014, and NASA's Solar Dynamics Observatory captured images 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 impacted Earth, please visit NOAA's Space Weather Prediction Center at a href= http //spaceweather.gov rel= nofollow spaceweather.gov /a , the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This f

Extreme ultraviolet light streams out of an X-class solar flare as seen in this image captured on March 29, 2014, by NASA's Solar Dynamics Observatory. This image blends two wavelengths of light 304 and 171 Angstroms, which help scientists observe the lower levels of the sun's atmosphere. More info The sun emitted a significant solar flare, peaking at 1 48 p.m. EDT March 29, 2014, and NASA's Solar Dynamics Observatory captured images 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 impacted Earth, please visit NOAA's Space Weather Prediction Center at a href= http //spaceweather.gov rel= nofollow spaceweather.gov /a , the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This f
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of Extreme ultraviolet light streams out of an X-class solar flare as seen in this image captured on March 29, 2014, by NASA's Solar Dynamics Observatory. This image blends two wavelengths of light 304 and 171 Angstroms, which help scientists observe the lower levels of the sun's atmosphere. More info The sun emitted a significant solar flare, peaking at 1 48 p.m. EDT March 29, 2014, and NASA's Solar Dynamics Observatory captured images 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 impacted Earth, please visit NOAA's Space Weather Prediction Center at a href= http //spaceweather.gov rel= nofollow spaceweather.gov /a , the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This f by Piemags/PL Photography Limited is available for licensing today.
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Image Number: 6145-45256910Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Dynamic Solar PhenomenaContributor:PiemagsModel Release:NoProperty Release:NoResolution:4096×4096