NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured images of the events. 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 , the U.S. government's official source for space weather forecasts, alerts, watches and warnings.
X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc.
The X9.3 flare was the largest flare so far in the current solar cycle, the approximately 11-year-cycle during which the sun’s activity waxes and wanes. The current solar cycle began in December 2008, and is now decreasing in intensity and heading toward solar minimum. This is a phase when such eruptions on the sun are increasingly rare, but history has shown that they can nonetheless be intense.
Credit: NASA’s Goddard Space Flight Center/Scott Wiessenger
Music: "Networked" from Killer Tracks
This video is public domain and along with other supporting visualizations can be downloaded from the Scientific Visualization Studio at:
If you liked this video, subscribe to the NASA Goddard YouTube channel:
Or subscribe to NASA’s Goddard Shorts HD Podcast:
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To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at , the U.S. government's official source for space weather forecasts, alerts, watches and warnings.
X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc.
The X9.3 flare was the largest flare so far in the current solar cycle, the approximately 11-year-cycle during which the sun’s activity waxes and wanes. The current solar cycle began in December 2008, and is now decreasing in intensity and heading toward solar minimum. This is a phase when such eruptions on the sun are increasingly rare, but history has shown that they can nonetheless be intense.
Credit: NASA’s Goddard Space Flight Center/Scott Wiessenger
Music: "Networked" from Killer Tracks
This video is public domain and along with other supporting visualizations can be downloaded from the Scientific Visualization Studio at:
If you liked this video, subscribe to the NASA Goddard YouTube channel:
Or subscribe to NASA’s Goddard Shorts HD Podcast:
Follow NASA’s Goddard Space Flight Center
· Facebook:
· Flickr
· Google+
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