This movie from the Solar Dynamics Observatory (SDO) shows the flare in the 171 Angstrom wavelength. Credit: NASA/SDO/LMSAL › Play/Download video
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The flare is seen here near the center of this image from SDO's Atmospheric Imaging Assembly instrument. The graph at the bottom represents GOES data showing the increase in x-ray emission as the flare erupted. Credit: NASA/SDO/LMSAL/GOES
At 9:35 PM ET on September 5, 2011, the sun emitted an Earth-directed M5.3 class flare as measured by the GOES satellite. The flare erupted from a region of the sun that appears close to dead center from Earth's perspective, an active region designated number 1283. The flare caused a slight increase of solar energetic protons some 26,000 miles above Earth's surface.
A coronal mass ejection (CME) -- another solar phenomenon that can send solar particles into space -- was associated with this flare. The CME is a relatively slow one, traveling at under 200 miles per second.
Further updates on the event will be provided as they become available.
What is a solar flare? What is a coronal mass ejection?