k Coronal hole, SDO image Coronal hole. Extreme ultraviolet UV image of a coronal hole dark blue region in the Suns atmosphere. In a coronal hole the Suns magnetic field white lines opens up, which allows solar winds to escape. This cornoal hole is facing directly towards Earth and is sending highspeed solar winds in the planets direction. This could cause polar geomagnetic storms that generate aurorae. Image obtained by NASAs Solar Dynamics Observatory on 12th October 2015. Stock Photo - Afloimages
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Coronal hole, SDO image Coronal hole. Extreme ultraviolet UV image of a coronal hole dark blue region in the Sun s atmosphere. In a coronal hole the Sun s magnetic field white lines opens up, which allows solar winds to escape. This cornoal hole is facing directly towards Earth and is sending high speed solar winds in the planet s direction. This could cause polar geomagnetic storms that generate aurorae. Image obtained by NASA s Solar Dynamics Observatory on 12th October 2015.
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Coronal hole, SDO image

Coronal hole. Extreme ultraviolet (UV) image of a coronal hole (dark blue region) in the Sun's atmosphere. In a coronal hole the Sun's magnetic field (white lines) opens up, which allows solar winds to escape. This cornoal hole is facing directly towards Earth and is sending high-speed solar winds in the planet's direction. This could cause polar geomagnetic storms that generate aurorae. Image obtained by NASA's Solar Dynamics Observatory on 12th October 2015.

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