Solar storm

From Wikipedia, the free encyclopedia

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]


Solar storms include:

See also[edit]


  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.