Coronal rain
Appearance
Coronal rain is a phenomenon that occurs in the Sun's corona when hot plasma cools and condenses in strong magnetic fields and falls to the photosphere. It is usually associated with active regions.[1][2][3][4][5][6] Coronal rain formed when impulsive heating from magnetic reconnection occurs.[7]
The material that makes up the coronal rain can be up to hundreds of times cooler than the surrounding environment.[8]
References
[edit]- ^ Jauregui, Andres (21 February 2013). "Coronal Rain: Solar Flare Rains Fire On Sun In NASA VIDEO". huffingtonpost.com. Retrieved 14 March 2014.
- ^ Grossman, Lisa. "Video: Coronal Rain Shower Caught on Sun". wired.com. Retrieved 14 March 2014.
- ^ "NASA Video Shows Stunning Coronal Rainstorm on Sun". voanews.com. Archived from the original on 14 March 2014. Retrieved 14 March 2014.
- ^ Shiga, David. "Sun's rain could explain why corona heat is insane". newscientist.com. Retrieved 14 March 2014.
- ^ O'NEILL, IAN. "The Sun's Coronal Rain Puzzle Solved". news.discovery.com. Retrieved 14 March 2014.
- ^ Antolin/Verwichte, P./ and E. (Erwin). "Transverse oscillations of loops with coronal rain observed by hinode/solar optical telescope". wrap.warwick.ac.uk. Archived from the original on 14 March 2014. Retrieved 14 March 2014.
- ^ Kohutova, P.; Verwichte, E.; Froment, C. (2019-10-01). "Formation of coronal rain triggered by impulsive heating associated with magnetic reconnection". Astronomy & Astrophysics. 630: A123. arXiv:1910.07746. Bibcode:2019A&A...630A.123K. doi:10.1051/0004-6361/201936253. ISSN 0004-6361.
- ^ Pastor, Adelina. "Coronal rain". European Solar Telescope. Retrieved 2024-05-17.
External links
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