k Solar flare, SDO ultraviolet image Solar flare, Solar Dynamics Observatory SDO ultraviolet image. The flare upper right is erupting from a sunspot. This is an X1.8class solar flare, erupting from sunspot 1402. The flare began at 1312 ET 1812 UTC on 27 January 2012 and peaked 25 minutes later. The flare caused a strong radio blackout. The accompanying coronal mass ejection CME was tracked by NASAs Goddard Space Weather Center. The SDO is an Earthorbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun and its atmosphere not seen in visible light is seen at a wavelength of 171 angstroms extreme ultraviolet. Editorial Stock Photo - Afloimages
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Solar flare, SDO ultraviolet image Solar flare, Solar Dynamics Observatory  SDO  ultraviolet image. The flare  upper right  is erupting from a sunspot. This is an X1.8 class solar flare, erupting from sunspot 1402. The flare began at 13:12 ET  18:12 UTC  on 27 January 2012 and peaked 25 minutes later. The flare caused a strong radio blackout. The accompanying coronal mass ejection  CME  was tracked by NASA s Goddard Space Weather Center. The SDO is an Earth orbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun and its atmosphere  not seen in visible light  is seen at a wavelength of 171 angstroms  extreme ultraviolet .
ED

Solar flare, SDO ultraviolet image

Solar flare, Solar Dynamics Observatory (SDO) ultraviolet image. The flare (upper right) is erupting from a sunspot. This is an X1.8-class solar flare, erupting from sunspot 1402. The flare began at 13:12 ET (18:12 UTC) on 27 January 2012 and peaked 25 minutes later. The flare caused a strong radio blackout. The accompanying coronal mass ejection (CME) was tracked by NASA's Goddard Space Weather Center. The SDO is an Earth-orbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun and its atmosphere (not seen in visible light) is seen at a wavelength of 171 angstroms (extreme ultraviolet).

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60511194

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Creation date
08-09-2017

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