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Substantial Coronal Holes

NASA's Solar Dynamics Observatory spies a pair of large coronal holes which rotated into view over the past few days (Oct. 20-21, 2016).
PIA15378
Credits: NASA/GSFC/Solar Dynamics Observatory
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Description

A pair of large coronal holes rotated into view over the past few days (Oct. 20-21, 2016). Coronal holes appear dark in certain wavelengths of extreme ultraviolet light, such as in the wavelength used here. These holes are areas of open magnetic field that spew solar wind into space. Sometimes, when they are facing Earth, they can cause geomagnetic disturbances that generate aurora. The lines you see were drawn to represent how solar scientists are modeling the magnetic field lines.

Movies
PIA15378_PFSS_211__holes_big.mp4
PIA15378_PFSS_211__holes_sm.mp4

SDO is managed by NASA's Goddard Space Flight Center, Greenbelt, Maryland, for NASA's Science Mission Directorate, Washington. Its Atmosphere Imaging Assembly was built by the Lockheed Martin Solar Astrophysics Laboratory (LMSAL), Palo Alto, California.