Coronal holes are regions of the Sun's corona that emit low levels of ultraviolet and X-ray radiation compared to their surroundings. They are composed...
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Stellar corona (redirect from Coronal activity)
the corona is more or less confined to the equatorial regions, with coronal holes covering the polar regions. However, during the Sun's active periods...
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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...
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interaction region (CIR), a high-speed stream of solar wind originating from a coronal hole. The frequency of geomagnetic storms increases and decreases with the...
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Sun (section Coronal heating)
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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produced an X1.0-class and multiple M-class solar flares and launched several coronal mass ejections (CMEs) toward Earth. On 9 May, the active region produced...
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Helmet streamer (redirect from Coronal streamer)
are open, oppositely directed magnetic fields which are anchored to coronal holes lower in the corona. The white-light emissions of helmet streamers is...
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Solar jet (redirect from Coronal jet)
quiet-Sun region, a coronal hole, or the Sun's poles, they are sometimes known as active region jets, quiet-Sun jets, coronal hole jets, or polar jets...
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non-existent. However, as the pole of Vega is facing Earth and a polar coronal hole may be present, confirmation of a corona as the likely source of the...
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In solar physics, a coronal loop is a well-defined arch-like structure in the Sun's atmosphere made up of relatively dense plasma confined and isolated...
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result from enhancements in the speed of the solar wind from coronal holes and coronal mass ejections. These disturbances alter the trajectories of charged...
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Van Allen 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...
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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 storms...
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Solar prominence (redirect from Coronal cloud)
thousands of kilometers into space. Some prominences may give rise to coronal mass ejections. Exact mechanism of prominence generation is an ongoing...
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Outline of astronomy (section Black holes)
Spicule Moreton wave Solar corona Solar transition region Coronal hole Coronal loop Coronal mass ejection Solar prominence Helmet streamer Solar variation...
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Solar wind (section Coronal mass ejection)
also emitting a slow solar wind. The fast solar wind originates from coronal holes, which are funnel-like regions of open field lines in the Sun's magnetic...
55 KB (6,597 words) - 19:10, 21 October 2024
November 2018: Voyager 2 crosses the heliopause, departing the heliosphere. Coronal mass ejection Fermi glow Martha, Gale (1 April 2013). "The Sun's Heliosphere"...
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Chromosphere Plage Spicule Moreton wave Corona Transition region Coronal hole Coronal loop Coronal mass ejection Nanoflare Prominence Helmet streamer Supra-arcade...
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Chromosphere Plage Spicule Moreton wave Corona Transition region Coronal hole Coronal loop Coronal mass ejection Nanoflare Prominence Helmet streamer Supra-arcade...
14 KB (1,894 words) - 21:58, 8 September 2024
Chromosphere Plage Spicule Moreton wave Corona Transition region Coronal hole Coronal loop Coronal mass ejection Nanoflare Prominence Helmet streamer Supra-arcade...
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Solar phenomena (section Coronal mass ejections)
solar wind, radio wave flux, solar flares, solar tornadoes, coronal mass ejections, coronal heating and sunspots. These phenomena are believed to be generated...
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2019). "Highly structured slow solar wind emerging from an equatorial coronal hole". Nature. 576 (7786): 237–242. Bibcode:2019Natur.576..237B. doi:10...
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in the corona, characterization of coronal mass ejection onset, and determination of the structure of coronal holes. Before mid-2010, EIT obtained an Fe...
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occur in active regions and are often, but not always, accompanied by coronal mass ejections, solar particle events, and other eruptive solar phenomena...
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signals will arrive from that general direction. An active region or coronal hole may persist for some 27 days resulting in a second aurora when the Sun...
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Flux transfer event Solar phenomena Solar cycle max min Solar storm Coronal hole CME Solar prominence Solar flare Solar particle event Radio emission...
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from the original on 16 November 2023. Retrieved 16 November 2023. "Coronal hole faces Earth". Space Weather Live. Archived from the original on 21 September...
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other active region phenomena such as coronal loops, prominences, and reconnection events. Most solar flares and coronal mass ejections originate in these...
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Flux transfer event Solar phenomena Solar cycle max min Solar storm Coronal hole CME Solar prominence Solar flare Solar particle event Radio emission...
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Baliunas, S; Posmentier, E.S; Okeke, P (2000). "Variations of solar coronal hole area and terrestrial lower tropospheric air temperature from 1979 to...
12 KB (1,037 words) - 20:57, 18 October 2024