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Solar storm

From Wikipedia, the free encyclopedia
Disturbance on the Sun

Asolar storm is a disturbance on theSun, which can emanate outward across theheliosphere, affecting the entireSolar System, includingEarth and itsmagnetosphere, and is the cause ofspace weather in the short-term with long-term patterns comprisingspace climate.[1][2]

Types

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Solar storms include:

See also

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  • List of solar storms
  • Aurora, a luminous phenomenon induced by ionization and excitation of constituents of a planet's upper atmosphere
  • Heliophysics, the scientific study of the Sun and region of space affected by the Sun
  • Magnetic cloud, a transient disturbance in the solar wind
  • Solar cycle, an 11-year cycle of sunspot activity
  • Solar prominence, a plasma and magnetic structure in the Sun's corona
  • Solar wind, the stream of particles and plasma emanating from the Sun
  • Active region, where most solar flares and coronal mass ejections originate

References

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  1. ^Hanaoka, Yoichiro; Watanabe, Kyoko; Yashiro, Seiji (2023). Kusano, Kanya (ed.).Solar-Terrestrial Prediction. Singapore: Springer. p. 251.doi:10.1007/978-981-19-7765-7_9.ISBN 978-981-19-7765-7.
  2. ^Schmieder, Brigitte (November 2018)."Extreme solar storms based on solar magnetic field".Journal of Atmospheric and Solar-Terrestrial Physics.180:46–51.arXiv:1708.01790.Bibcode:2018JASTP.180...46S.doi:10.1016/j.jastp.2017.07.018.S2CID 119087439.
Solar atmosphere
Interplanetary space
Magnetosphere
Planetary atmosphere
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