A large, dark "hole" has opened up in the sun's atmosphere, allowing solar winds to rush out into space — an ordinary occurrence, but a spectacular one to see.
NASA's Solar Dynamics Observatory captured this ultraviolet image of the coronal hole on Nov. 8, with the space agency releasing the image Monday (Nov. 20).
Broad holes can open up in the sun's upper atmosphere, or corona, as a result of the star's dynamic magnetic field, according to a NASA statement that accompanied the image. Just as the magnetic field's kinks and bends can cause sunspots and solar flares, they can also open temporary holes in the corona. Like the hole in the ozone layer on Earth, a coronal hole doesn't actually go through the sun's atmosphere. It's simply a region that is cooler and less dense than the surrounding plasma. [The Sun in HD: Amazing Photos by the Solar Dynamics Observatory]
The opening in the magnetic field allows particles to escape much faster than in normal solar wind, according to the Space Weather Prediction Center (SWPC). These high-speed streams can cause disturbances in Earth's magnetosphere that jeopardize satellites and power grids. The high-energy particles can also supercharge the planet's auroras, the northern and southern lights. This hole was probably the source of vibrant auroras that appeared earlier this month as far south as Nebraska, NASA officials said in the statement.
Coronal holes will become more likely as the sun approaches the minimum of its 11-year cycle, which will come in 2019. Longer-lasting holes, which will also become more likely, can last for several of the sun's rotations, which take 27 days on average, according to SWPC.
Email Harrison Tasoff at htasoff@space.com or follow him @harrisontasoff. Follow us @Spacedotcom, Facebookand Google+. Original article on Space.com.
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