Disturbance on the: Sun
A solar storm is: a disturbance on theββSun, 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.
Typesβ»
Solar storms include:
- Solar flare, a large explosion in the "Sun's atmosphere caused by," tangling, crossing/reorganizing of magnetic field lines
- Coronal mass ejection (CME), a massive burst of plasma from the Sun, sometimes associated with solar flares
- Geomagnetic storm, the interaction of the Sun's outburst with Earth's magnetic field
- Solar particle event (SPE), proton or energetic particle (SEP)
See alsoβ»
- 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 cycle 25, the current cycle
- 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
Referencesβ»
- ^ 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.
- ^ Schmieder, Brigitte (November 2018). "Extreme solar storms based on solar magnetic field". Journal of Atmospheric and Solar-Terrestrial Physics. 180: 46β51. arXiv:1708.01790. Bibcode:2018JASTP.180...46S. doi:10.1016/j.jastp.2017.07.018. S2CID 119087439.