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Solar storm

A solar storm is a disturbance on the Sun, which can emanate outward across the heliosphere, affecting the entire Solar System, including Earth and its magnetosphere, and is the cause of space weather in the short-term with long-term patterns comprising space 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.