Back Plasmawolk Afrikaans انبعاث كتلي إكليلي Arabic Каранальныя выкіды масы Byelorussian Коронално изхвърляне на маса Bulgarian Ejecció de massa coronal Catalan Výron koronální hmoty Czech Gigantisk soludbrud Danish Koronaler Massenauswurf German Στεμματική εκπομπή μάζας Greek Eyección de masa coronal Spanish
A coronal mass ejection (CME) is a significant ejection of plasma mass from the Sun's corona into the heliosphere. CMEs are often associated with solar flares and other forms of solar activity, but a broadly accepted theoretical understanding of these relationships has not been established.
If a CME enters interplanetary space, it is referred to as an interplanetary coronal mass ejection (ICME). ICMEs are capable of reaching and colliding with Earth's magnetosphere, where they can cause geomagnetic storms, aurorae, and in rare cases damage to electrical power grids. The largest recorded geomagnetic perturbation, resulting presumably from a CME, was the solar storm of 1859. Also known as the Carrington Event, it disabled parts of the newly created United States telegraph network, starting fires and electrically shocking some telegraph operators.
Near solar maxima, the Sun produces about three CMEs every day, whereas near solar minima, there is about one CME every five days.