Coronal mass ejection

Coronal mass ejection

A coronal mass ejection (CME) is a significant release of plasma and accompanying magnetic field 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. Near solar maxima, the Sun produces about three CMEs every day, whereas near solar minima, there is about one CME every five days.

Comment
enA coronal mass ejection (CME) is a significant release of plasma and accompanying magnetic field 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. Near solar maxima, the Sun produces about three CMEs every day, whereas near solar minima, there is about one CME every five days.
Date
enMay 2022
Depiction
Aurora Australis From ISS.jpg
Large coronal mass ejection on 2000-02-27 from SOHO LASCO C3 coronagraph.jpg
Magnificent CME Erupts on the Sun - August 31.jpg
Has abstract
enA coronal mass ejection (CME) is a significant release of plasma and accompanying magnetic field 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 at the time newly created United States telegraph network, starting fires and 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.
Hypernym
Burst
Is primary topic of
Coronal mass ejection
Label
enCoronal mass ejection
Link from a Wikipage to an external page
www.scientificamerican.com/article.cfm%3Fid=bracing-for-a-solar-superstorm
www.sidc.be/cactus/catalog/LASCO/2_5_0/dataoverview/ascii_out.txt
www.sidc.be/cactus/catalog/LASCO/2_5_0/dataoverview/CME_and_SSN_rate.png
solar.physics.montana.edu/press/faq.html
science.nasa.gov/science-news/science-at-nasa/2008/06may_carringtonflare/
science.nasa.gov/science-news/science-at-nasa/2008/27may_cartwheelcme/
www.swpc.noaa.gov/
clusterlaunch.esa.int/science-e/www/object/index.cfm%3Ffobjectid=41817
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File:Large coronal mass ejection on 2000-02-27 from SOHO LASCO C3 coronagraph.jpg
File:Magnificent CME Erupts on the Sun - August 31.jpg
File:Solar Storm on August 1, 2010.OGG
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SameAs
Coronal mass ejection
Ejeção de massa coronal
Ejecció de massa coronal
Éjection de masse coronale
Espulsione di massa coronale
Eyección de masa coronal
Gigantisk soludbrud
KDWq
Koroa-masaren eiekzio
Koronakidobódás
Koronale Massenausworf
Koronaler Massenauswurf
Koronalne eksplozije
Koronalni izbačaji masa
Koronalni izbačaji masa
Koronalny wyrzut masy
Koronamasseutbrudd
Koronamassutkastning
Krooni massi purse
Lentingan jisim korona
Lontaran massa korona
m.01lv71
Plasmawolk
Plasmawolk
Q129890
Taçküre kütle atımı
Výron koronálnej hmoty
Výron koronální hmoty
Στεμματική εκπομπή μάζας
Каранальныя выкіды масы
Коронално изхвърляне на маса
Корональные выбросы массы
Корональні викиди маси
انبعاث كتلي إكليلي
خروج جرم از تاج خورشیدی
कोरोना द्रव्य उत्क्षेपण
കൊറോണൽ മാസ് ഇജക്ഷൻ
コロナ質量放出
日冕物質抛射
코로나 질량 방출
Section
enyes
SeeAlso
Solar phenomena
Solar prominence
Subject
Category:Articles containing video clips
Category:Solar phenomena
Category:Stellar phenomena
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Large coronal mass ejection on 2000-02-27 from SOHO LASCO C3 coronagraph.jpg?width=300
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