Biggest Solar Storm Since 2005

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.