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Coronal mass ejection information


Coronal mass ejections are usually visible in white-light coronagraphs.

A coronal mass ejection (CME) is a significant ejection of magnetic field and accompanying 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.

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Coronal mass ejection

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A coronal mass ejection (CME) is a significant ejection of magnetic field and accompanying plasma mass from the Sun's corona into the heliosphere. CMEs...

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July 2012 solar storm

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2012 was a solar storm involving an unusually large and strong coronal mass ejection that occurred on July 23, 2012. It missed Earth with a margin of...

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Carrington Event

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stations. The geomagnetic storm was most likely the result of a coronal mass ejection (CME) from the Sun colliding with Earth's magnetosphere. The geomagnetic...

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Solar wind

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conjunction with an episodic ejection of material and magnetic flux from the Sun's atmosphere, known as a coronal mass ejection. The following day, a powerful...

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Solar prominence

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thousands of kilometers into space. Some prominences may give rise to coronal mass ejections. Exact mechanism of prominence generation is an ongoing target of...

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List of solar storms

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on the Sun, most often from coronal mass ejections (CMEs) and solar flares from active regions, or, less often, from coronal holes. Minor to active solar...

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Coronal hole

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from coronal holes encounter the Earth, they can cause major displays of aurorae. Near solar minimum, when activity such as coronal mass ejections is less...

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Aurora

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from enhancements in the speed of the solar wind from coronal holes and coronal mass ejections. These disturbances alter the trajectories of charged particles...

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Solar cycle

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levels of solar radiation and ejection of solar material, the number and size of sunspots, solar flares, and coronal loops all exhibit a synchronized...

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Stellar corona

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large solar flares and prominences are coronal mass ejections (CME). These are enormous emissions of coronal material and magnetic field that travel...

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Solar flare

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in active regions and are often, but not always, accompanied by coronal mass ejections, solar particle events, and other eruptive solar phenomena. The...

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The Maze Runner

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author James Dashner. It takes place in a world suffering from a coronal mass ejection and whose surviving civilians fight to avoid an apocalyptic illness...

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Geomagnetic storm

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The disturbance that drives the magnetic storm may be a solar coronal mass ejection (CME) or (much less severely) a co-rotating interaction region (CIR)...

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Sun

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Discoveries included the first observations of coronal mass ejections, then called "coronal transients", and of coronal holes, now known to be intimately associated...

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Weather

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S2CID 4402268. Bill Christensen. Shock to the (Solar) System: Coronal Mass Ejection Tracked to Saturn. Archived 1 January 2011 at the Wayback Machine...

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Stellar mass loss

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significant mass loss and can be influenced by a number of factors, including: Gravitational attraction of a binary companion Coronal mass ejection-type events...

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Helmet streamer

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appear more symmetrically around the Sun. Upon the eruption of a coronal mass ejection (CME), the overlying helmet streamer deforms becoming the CME's...

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Solar storm

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caused by tangling, crossing or reorganizing of magnetic field lines Coronal mass ejection (CME), a massive burst of plasma from the Sun, sometimes associated...

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Solar phenomena

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forms, including solar wind, radio wave flux, solar flares, coronal mass ejections, coronal heating and sunspots. These phenomena are believed to be generated...

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Ejection

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(disambiguation) Ejector (disambiguation) Coronal mass ejection, an ejection of material from a Sun's corona Ejection fraction, the fraction of blood pumped...

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Solar particle event

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atmosphere during a solar flare or in interplanetary space by a coronal mass ejection shock. Other nuclei such as helium and HZE ions may also be accelerated...

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Van Allen radiation belt

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Probe team, it was stated that this third belt is a product of coronal mass ejection from the Sun. It has been represented as a separate creation which...

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Moreton wave

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plasma and magnetism, moving at 250 km/s, in conjunction with a big coronal mass ejection in February 2009. Moreton measured the waves propagating at a speed...

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Solar mass

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atmosphere of the Sun are ejected directly into outer space as the solar wind and coronal mass ejections. The original mass of the Sun at the time it...

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Bastille Day solar storm

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Bastille Day. It involved a solar flare, a solar particle event, and a coronal mass ejection which caused a severe geomagnetic storm. On 14 July 2000 from about...

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ESA Vigil

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wind streams. The Vigil mission will improve the assessment of Coronal Mass Ejection (CME) motion and density, speed/energy, arrival time and impact...

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Nanoflare

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portal Star portal Chromosphere Stellar corona Coronal cloud Coronal loops Coronal mass ejection Coronal radiative losses Current sheet Magnetic reconnection...

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