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1:02
MSN
Space
Big Coronal Mass Ejection From Sun's Farside Via SOHO Spacecraft
The ESA/NASA Solar and Heliospheric Observatory (SOHO) captured a coronal mass ejection erupt from the far side of the Sun. Credit: ESA/NASA/SOHO | edited by Space.com's Steve Spaleta
5 months ago
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The most distinctive feature on the Sun from Oct. 31 - Nov. 2 was a good-sized coronal hole nearly centered on the Sun’s face. The coronal hole — which appears as a dark area in this extreme ultraviolet image captured by our Solar Dynamics Observatory — is an area of open magnetic field from which high-speed solar wind rushes out into space. Coronal holes are a common occurrence, and such solar wind can trigger effects like auroras when it interacts with Earth’s magnetic field. https://go.nasa.g
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• Coronal Rain • forms when hotter plasma in the Sun’s corona cools down and becomes denser. Like raindrops on Earth, coronal rain is pulled down to the surface by gravity. Because the plasma is electrically charged, it follows the magnetic field lines, which make huge arches/loops, instead of falling in a straight line. This image is a snapshot from a 23-minute time-lapse video which is comprised of the highest resolution images ever made of coronal rain. The scientists show in the paper that t
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