Jan. 24th, 2012
Solar Dynamics Observatory captured the flare, shown here in teal as that is the color typically used to show light in the 131 angstrom wavelength, a wavelength in which it is easy to view solar flares. The flare began at 10:38 PM ET on Jan. 22, peaked at 10:59 PM and ended at 11:34 PM. Credit: NASA/SDO/AIA The Solar Heliospheric Observatory captured the coronal mass ejection (CME) in this video (which shows the sun's activity from January 19 to January 23). The end of the movie shows the interference caused by the onslaught of fast, energetic solar particles emitted from the sun. Credit: SOHO/ESA & NASA SOHO view of M9 flare.Credit: SOHO/ESA & NASA Solar Dynamics Observatory captured the flare, shown here in bronze as that is the color typically used to show light in the 193 angstrom wavelength. The flare began at 10:38 PM ET on Jan. 22, peaked at 10:59 PM and ended at 11:34 PM. Credit: NASA/SDO/AIA Solar Dynamics Observatory captured the flare, shown here in teal as that is the color typically used to show light in the 131 angstrom wavelength. The flare began at 10:38 PM ET on Jan. 22, peaked at 10:59 PM and ended at 11:34 PM. Credit: NASA/SDO/AIA Solar Dynamics Observatory captured the flare, shown here in red/orange as that is the color typically used to show light in the 304 angstrom wavelength. The flare began at 10:38 PM ET on Jan. 22, peaked at 10:59 PM and ended at 11:34 PM. Credit: NASA/SDO/AIA Interview with Antti Pulkkinen, NASA Solar Scientist. What makes this event different from other recent CMEs and flares?For complete transcript, click here. Interview with Antti Pulkkinen, NASA Solar Scientist. The three stages of this event. For complete transcript, click here. Interview with Antti Pulkkinen, NASA Solar Scientist. How will this event affect the Earth? For complete transcript, click here. Interview with Antti Pulkkinen, NASA Solar Scientist. Will we see more events like this one in the future? For complete transcript, click here. The sun erupted late on January 22, 2012 with an M8.7 class flare, an earth-directed coronal mass ejection (CME), and a burst of fast moving, highly energetic protons known as a "solar energetic particle" event. The latter has caused the strongest solar radiation storm since September 2005 according to NOAA's Space Weather Prediction Center. Related pages
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