Glossary term: Eyección de masa coronal (CME)
Description: Una eyección de masa coronal (o CME por sus siglas en inglés) es la expulsión explosiva de plasma solar y su campo magnético desde el Sol (y otras estrellas similares) hacia la heliosfera (o astrosfera en el caso de otras estrellas). Las CME son explosiones magnéticas, normalmente asociadas a erupciones solares. Una CME es una eyección física de material, a diferencia de una «erupción», que se limita a la radiación visible. Las CME varían ampliamente en cuanto a estructura, densidad y velocidad. Las CME que impactan en la Tierra pueden provocar importantes tormentas geomagnéticas.
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See this term in other languages
Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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In Other Languages
- Árabe: قذف الكتلة الإكليلي (CME)
- Alemán: Koronaler Massenauswurf (CME)
- Inglés: Coronal Mass Ejection (CME)
- Francés: Éjection de masse coronale (EMC ou CME en anglais)
- Italiano: Espulsione di massa coronale (CME)
- Japonés: コロナ質量放出 (external link)
- Coreano: 코로나질량방출(CME)
- Portugués de Brasil: Ejeção de massa coronal (CME)
- Chino simplificado: 日冕物质抛射（CME）
- Chino tradicional: 日冕物質拋射（CME）
Related Media
A Coronal Mass Ejection
Caption: A burst of solar material can be seen erupting from the Sun in this view, illustrating a coronal mass ejection (CME)—a large eruption of plasma and magnetic field from the Sun’s outer atmosphere, or corona. These CMEs are caused by magnetic explosions in the Sun's corona. During a CME, huge amounts of electrically charged particles are launched into space at great speeds, carrying part of the Sun’s magnetic field with them. These events are driven by changes in the Sun’s magnetic structure and release vast clouds of hot gas that travel outward into the solar system. When a CME moves through space, it can interact with a planet’s magnetic field and atmosphere, sometimes creating spectacular auroras or, in strong cases, interfering with artificial satellites and power systems.
CMEs are often associated with a temporary brightening of the region of the Sun where the CME originated. This is known as a solar flare. Stars other than the Sun can also have CMEs and flares.
This image was taken by NASA's Solar Dynamics Observatory (SDO). This is a space mission to monitor the Sun. The image here is taken at a special wavelength which partially ionised helium emits strongly at.
Credit: NASA/Goddard/SDO
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License: PD Public Domain icons
