• Thumbnail for Coronal hole
    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...
    8 KB (878 words) - 05:49, 22 June 2024
  • Thumbnail for Stellar corona
    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...
    62 KB (7,677 words) - 17:36, 18 October 2024
  • Thumbnail for Coronal mass ejection
    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...
    58 KB (6,828 words) - 11:32, 12 September 2024
  • Thumbnail for Geomagnetic storm
    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...
    49 KB (5,586 words) - 00:17, 3 November 2024
  • Thumbnail for Sun
    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...
    165 KB (18,112 words) - 01:49, 14 November 2024
  • Thumbnail for May 2024 solar storms
    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...
    49 KB (3,613 words) - 07:04, 20 November 2024
  • Thumbnail for Helmet 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...
    10 KB (995 words) - 03:43, 15 August 2024
  • 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...
    5 KB (540 words) - 13:46, 17 May 2024
  • Thumbnail for Vega
    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...
    96 KB (10,142 words) - 03:14, 19 November 2024
  • Thumbnail for Coronal loop
    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...
    13 KB (1,691 words) - 16:17, 9 September 2024
  • Thumbnail for Aurora
    result from enhancements in the speed of the solar wind from coronal holes and coronal mass ejections. These disturbances alter the trajectories of charged...
    117 KB (13,050 words) - 08:59, 20 November 2024
  • 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...
    38 KB (4,436 words) - 00:56, 8 November 2024
  • Thumbnail for List of solar storms
    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...
    56 KB (4,611 words) - 10:16, 7 November 2024
  • Thumbnail for Solar prominence
    thousands of kilometers into space. Some prominences may give rise to coronal mass ejections. Exact mechanism of prominence generation is an ongoing...
    17 KB (1,885 words) - 16:40, 29 October 2024
  • Thumbnail for Outline of astronomy
    Spicule Moreton wave Solar corona Solar transition region Coronal hole Coronal loop Coronal mass ejection Solar prominence Helmet streamer Solar variation...
    43 KB (3,397 words) - 22:56, 20 October 2024
  • Thumbnail for Solar wind
    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
  • Thumbnail for Heliosphere
    November 2018: Voyager 2 crosses the heliopause, departing the heliosphere. Coronal mass ejection Fermi glow Martha, Gale (1 April 2013). "The Sun's Heliosphere"...
    63 KB (6,605 words) - 10:19, 19 October 2024
  • Thumbnail for Radiative zone
    Chromosphere Plage Spicule Moreton wave Corona Transition region Coronal hole Coronal loop Coronal mass ejection Nanoflare Prominence Helmet streamer Supra-arcade...
    11 KB (1,732 words) - 00:52, 27 October 2024
  • Thumbnail for Solar core
    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
  • Thumbnail for Convection zone
    Chromosphere Plage Spicule Moreton wave Corona Transition region Coronal hole Coronal loop Coronal mass ejection Nanoflare Prominence Helmet streamer Supra-arcade...
    7 KB (837 words) - 22:35, 8 September 2024
  • Thumbnail for Solar phenomena
    solar wind, radio wave flux, solar flares, solar tornadoes, coronal mass ejections, coronal heating and sunspots. These phenomena are believed to be generated...
    48 KB (5,267 words) - 07:35, 19 November 2024
  • Thumbnail for Parker Solar Probe
    2019). "Highly structured slow solar wind emerging from an equatorial coronal hole". Nature. 576 (7786): 237–242. Bibcode:2019Natur.576..237B. doi:10...
    91 KB (8,301 words) - 05:44, 11 November 2024
  • in the corona, characterization of coronal mass ejection onset, and determination of the structure of coronal holes. Before mid-2010, EIT obtained an Fe...
    7 KB (1,041 words) - 16:35, 5 April 2024
  • Thumbnail for Solar flare
    occur in active regions and are often, but not always, accompanied by coronal mass ejections, solar particle events, and other eruptive solar phenomena...
    49 KB (5,229 words) - 09:01, 29 October 2024
  • Thumbnail for TV and FM DX
    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...
    31 KB (4,090 words) - 06:37, 2 October 2024
  • Thumbnail for Heliophysics
    Flux transfer event Solar phenomena Solar cycle max min Solar storm Coronal hole CME Solar prominence Solar flare Solar particle event Radio emission...
    12 KB (1,370 words) - 20:46, 23 October 2024
  • Thumbnail for Solar cycle 25
    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...
    60 KB (2,964 words) - 18:13, 26 October 2024
  • Thumbnail for Sunspot
    other active region phenomena such as coronal loops, prominences, and reconnection events. Most solar flares and coronal mass ejections originate in these...
    41 KB (4,236 words) - 10:40, 19 November 2024
  • Thumbnail for Heliospheric current sheet
    Flux transfer event Solar phenomena Solar cycle max min Solar storm Coronal hole CME Solar prominence Solar flare Solar particle event Radio emission...
    13 KB (1,334 words) - 18:07, 8 September 2024
  • Thumbnail for Pius N. Okeke
    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